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Lonati GL, Zitterbart DP, Miller CA, Corkeron P, Murphy CT, Moore MJ. Investigating the thermal physiology of critically endangered North Atlantic right whales Eubalaena glacialis via aerial infrared thermography. ENDANGER SPECIES RES 2022. [DOI: 10.3354/esr01193] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/23/2022] Open
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Miller CA, Di Fulvio A, Clarke SD, Pozzi SA. DUAL-PARTICLE DOSEMETER BASED ON ORGANIC SCINTILLATOR. Radiat Prot Dosimetry 2020; 191:319-327. [PMID: 33112389 DOI: 10.1093/rpd/ncaa151] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [MESH Headings] [Track Full Text] [Subscribe] [Scholar Register] [Received: 02/17/2020] [Revised: 08/09/2020] [Accepted: 08/15/2020] [Indexed: 06/11/2023]
Abstract
Traditionally available handheld dosemeters are generally sensitive to only one type of radiation: neutrons or photons. Some dosemeters also rely on very specific attenuation correlations between response and dose, are not scalable in size and multiple dosemeters are required to characterise mixed-particle fields. The research presented here serves as a proof-of-concept for a method to simultaneously measure dose rates from neutrons and photons using a particle discriminating organic scintillation detector without the need for spectral deconvolution. The method was compared with traditional instruments and to simulation. Isotopic photon dose rates measured with this method were within 4% of simulated truth, whereas fission spectrum neutron dose rates were measured within 21%. Measurements of dose rates from both particles agree with simulated truth better than traditional instruments. This new method allows for measurement of dose equivalent from both neutrons and photons with a single instrument and no reliance on spectral deconvolution.
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Affiliation(s)
- C A Miller
- Department of Nuclear Engineering and Radiological Sciences, University of Michigan, 2355 Bonisteel Blvd, Ann Arbor, MI 48109, USA
| | - A Di Fulvio
- Department of Nuclear, Plasma, and Radiological Engineering, University of Illinois, 104 S. Wright St., Urbana, IL 61801, USA
| | - S D Clarke
- Department of Nuclear Engineering and Radiological Sciences, University of Michigan, 2355 Bonisteel Blvd, Ann Arbor, MI 48109, USA
| | - S A Pozzi
- Department of Nuclear Engineering and Radiological Sciences, University of Michigan, 2355 Bonisteel Blvd, Ann Arbor, MI 48109, USA
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Leslie MS, Perkins-Taylor CM, Durban JW, Moore MJ, Miller CA, Chanarat P, Bahamonde P, Chiang G, Apprill A. Body size data collected non-invasively from drone images indicate a morphologically distinct Chilean blue whale (Balaenoptera musculus) taxon. ENDANGER SPECIES RES 2020. [DOI: 10.3354/esr01066] [Citation(s) in RCA: 7] [Impact Index Per Article: 1.8] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/23/2022] Open
Abstract
The blue whale Balaenoptera musculus (Linnaeus, 1758) was the target of intense commercial whaling in the 20th century, and current populations remain drastically below pre-whaling abundances. Reducing uncertainty in subspecific taxonomy would enable targeted conservation strategies for the recovery of unique intraspecific diversity. Currently, there are 2 named blue whale subspecies in the temperate to polar Southern Hemisphere: the Antarctic blue whale B. m. intermedia and the pygmy blue whale B. m. brevicauda. These subspecies have distinct morphologies, genetics, and acoustics. In 2019, the Society for Marine Mammalogy’s Committee on Taxonomy agreed that evidence supports a third (and presently unnamed) subspecies of Southern Hemisphere blue whale subspecies, the Chilean blue whale. Whaling data indicate that the Chilean blue whale is intermediate in body length between pygmy and Antarctic blue whales. We collected body size data from blue whales in the Gulfo Corcovado, Chile, during the austral summers of 2015 and 2017 using aerial photogrammetry from a remotely controlled drone to test the hypothesis that the Chilean blue whale is morphologically distinct from other Southern Hemisphere blue whale subspecies. We found the Chilean whale to be morphologically intermediate in both overall body length and relative tail length, thereby joining other diverse data in supporting the Chilean blue whale as a unique subspecific taxon. Additional photogrammetry studies of Antarctic, pygmy, and Chilean blue whales will help examine unique morphological variation within this species of conservation concern. To our knowledge, this is the first non-invasive small drone study to test a hypothesis for systematic biology.
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Affiliation(s)
- MS Leslie
- Department of Biology, Swarthmore College, 500 College Ave., Swarthmore, PA 19081, USA
| | - CM Perkins-Taylor
- Department of Biology, Swarthmore College, 500 College Ave., Swarthmore, PA 19081, USA
| | - JW Durban
- Southall Environmental Associates, Inc., 9099 Soquel Drive, Suite 8, Aptos, CA 95003, USA
| | - MJ Moore
- Biology Department, Woods Hole Oceanographic Institution, 266 Woods Hole Rd., MS #50, Woods Hole, MA 02543, USA
| | - CA Miller
- Marine Chemistry & Geochemistry Department, Woods Hole Oceanographic Institution, 266 Woods Hole Rd., MS #4, Woods Hole, MA 02543, USA
| | - P Chanarat
- WWF Thailand, Level 3, 9 Pra Dipat 10, Pra Dipat Road, Phaya Thai, Bangkok 10400, Thailand
| | - P Bahamonde
- HUB AMBIENTAL UPLA - Centro de Estudios Avanzado, Universidad de Playa Ancha, Valparaíso 2340000, Chile
- Melimoyu Ecosystem Research Institute, Avenida Kennedy 5682, Santiago de Chile 7650720, Chile
| | - G Chiang
- Melimoyu Ecosystem Research Institute, Avenida Kennedy 5682, Santiago de Chile 7650720, Chile
- CAPES-UC, Center for Applied Ecology & Sustainability, Pontificia Universidad Catolica de Chile, Santiago 8331150, Chile
| | - A Apprill
- Marine Chemistry & Geochemistry Department, Woods Hole Oceanographic Institution, 266 Woods Hole Rd., MS #4, Woods Hole, MA 02543, USA
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Weaver CP, Miller CA. A Framework for Climate Change-Related Research to Inform Environmental Protection. Environ Manage 2019; 64:245-257. [PMID: 31359093 PMCID: PMC7350535 DOI: 10.1007/s00267-019-01189-0] [Citation(s) in RCA: 2] [Impact Index Per Article: 0.4] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Key Words] [MESH Headings] [Grants] [Track Full Text] [Subscribe] [Scholar Register] [Received: 09/17/2018] [Accepted: 07/18/2019] [Indexed: 05/05/2023]
Abstract
A critical charge for science to inform environmental protection is to characterize the risks associated with climate change, to support development of appropriate responses. The nature of climate change, however, presents significant challenges that must be overcome to do so, including the need for integration and synthesis across the many disciplines that contain knowledge relevant for achieving environmental protection goals. This paper describes an interdisciplinary research framework organized around three "Science Challenges" that directly respond to the needs of environmental protection organizations. Broadly, these Science Challenges refer to the research needed to: inform actions to enhance resilience across a broad range of environmental and social stresses to environmental management endpoints; actions to limit GHG emissions and slow the underlying rate of climate change; and the transition to sustainability across the full spectrum of climate change impacts and solutions; all as situated within an overarching risk management perspective. These Challenges span all media and systems critical to effective environmental protection, highlighting the cross-cutting nature of climate change and the need to address its impacts across systems and places. While this framework uses EPA's programs as an illustrative example, the research directions articulated herein are broadly applicable across the spectrum of environmental protection organizations. Going forward, we recommend that climate-related research to inform environmental protection efforts should accelerate its evolution toward research that is inherently cross-media and cross-scale; explicitly considers the social dimensions of change; and focuses on designing solutions to the specific risks climate change poses to the environment and society.
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Affiliation(s)
- C P Weaver
- Office of Research and Development, U.S. Environmental Protection Agency, Research Triangle Park, Durham, NC, USA.
| | - C A Miller
- Office of Research and Development, U.S. Environmental Protection Agency, Research Triangle Park, Durham, NC, USA
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Wang L, Haghmoradi A, Liu J, Xi S, Hirasaki GJ, Miller CA, Chapman WG. Modeling micelle formation and interfacial properties with iSAFT classical density functional theory. J Chem Phys 2018; 146:124705. [PMID: 28388160 DOI: 10.1063/1.4978503] [Citation(s) in RCA: 18] [Impact Index Per Article: 3.0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 01/05/2023] Open
Abstract
Surfactants reduce the interfacial tension between phases, making them an important additive in a number of industrial and commercial applications from enhanced oil recovery to personal care products (e.g., shampoo and detergents). To help obtain a better understanding of the dependence of surfactantproperties on molecular structure, a classical density functional theory, also known as interfacial statistical associating fluid theory, has been applied to study the effects of surfactant architecture on micelle formation and interfacial properties for model nonionic surfactant/water/oil systems. In this approach, hydrogen bonding is explicitly included. To minimize the free energy, the system minimizes interactions between hydrophobic components and hydrophilic components with water molecules hydrating the surfactant head group. The theory predicts micellar structure, effects of surfactant architecture on critical micelle concentration, aggregation number, and interfacial tension isotherm of surfactant/water systems in qualitative agreement with experimental data. Furthermore, this model is applied to study swollen micelles and reverse swollen micelles that are necessary to understand the formation of a middle-phase microemulsion.
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Affiliation(s)
- Le Wang
- Department of Chemical and Biomolecular Engineering, Rice University, 6100 Main St., Houston, Texas 77005, USA
| | - Amin Haghmoradi
- Department of Chemical and Biomolecular Engineering, Rice University, 6100 Main St., Houston, Texas 77005, USA
| | - Jinlu Liu
- Department of Chemical and Biomolecular Engineering, Rice University, 6100 Main St., Houston, Texas 77005, USA
| | - Shun Xi
- Department of Chemical and Biomolecular Engineering, Rice University, 6100 Main St., Houston, Texas 77005, USA
| | - George J Hirasaki
- Department of Chemical and Biomolecular Engineering, Rice University, 6100 Main St., Houston, Texas 77005, USA
| | - Clarence A Miller
- Department of Chemical and Biomolecular Engineering, Rice University, 6100 Main St., Houston, Texas 77005, USA
| | - Walter G Chapman
- Department of Chemical and Biomolecular Engineering, Rice University, 6100 Main St., Houston, Texas 77005, USA
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Abstract
Background Reconstruction of clonal evolution is critical for understanding tumor progression and implementing personalized therapies. This is often done by clustering somatic variants based on their cellular prevalence estimated via bulk tumor sequencing of multiple samples. The clusters, consisting of the clonal marker variants, are then ordered based on their estimated cellular prevalence to reconstruct clonal evolution trees, a process referred to as 'clonal ordering'. However, cellular prevalence estimate is confounded by statistical variability and errors in sequencing/data analysis, and therefore inhibits accurate reconstruction of the clonal evolution. This problem is further complicated by intra- and inter-tumor heterogeneity. Furthermore, the field lacks a comprehensive visualization tool to facilitate the interpretation of complex clonal relationships. To address these challenges we developed ClonEvol, a unified software tool for clonal ordering, visualization, and interpretation. Materials and methods ClonEvol uses a bootstrap resampling technique to estimate the cellular fraction of the clones and probabilistically models the clonal ordering constraints to account for statistical variability. The bootstrapping allows identification of the sample founding- and sub-clones, thus enabling interpretation of clonal seeding. ClonEvol automates the generation of multiple widely used visualizations for reconstructing and interpreting clonal evolution. Results ClonEvol outperformed three of the state of the art tools (LICHeE, Canopy and PhyloWGS) for clonal evolution inference, showing more robust error tolerance and producing more accurate trees in a simulation. Building upon multiple recent publications that utilized ClonEvol to study metastasis and drug resistance in solid cancers, here we show that ClonEvol rediscovered relapsed subclones in two published acute myeloid leukemia patients. Furthermore, we demonstrated that through noninvasive monitoring ClonEvol recapitulated the emerging subclones throughout metastatic progression observed in the tumors of a published breast cancer patient. Conclusions ClonEvol has broad applicability for longitudinal monitoring of clonal populations in tumor biopsies, or noninvasively, to guide precision medicine. Availability ClonEvol is written in R and is available at https://github.com/ChrisMaherLab/ClonEvol.
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Affiliation(s)
- H X Dang
- McDonnell Genome Institute.,Department of Internal Medicine
| | - B S White
- McDonnell Genome Institute.,Department of Internal Medicine
| | | | | | - J Luo
- Department of Surgery.,Siteman Cancer Center
| | - R C Fields
- Department of Surgery.,Siteman Cancer Center
| | - C A Maher
- McDonnell Genome Institute.,Department of Internal Medicine.,Siteman Cancer Center.,Department of Biomedical Engineering, Washington University in St. Louis, St. Louis, USA
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Wilcock CJ, Stafford GP, Miller CA, Ryabenkova Y, Fatima M, Gentile P, Möbus G, Hatton PV. Preparation and Antibacterial Properties of Silver-Doped Nanoscale Hydroxyapatite Pastes for Bone Repair and Augmentation. J Biomed Nanotechnol 2017; 13:1168-1176. [PMID: 31251149 DOI: 10.1166/jbn.2017.2387] [Citation(s) in RCA: 18] [Impact Index Per Article: 2.6] [Reference Citation Analysis] [What about the content of this article? (0)] [Abstract] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/23/2022]
Abstract
The treatment of deep bone infections remains a significant challenge in orthopaedic and dental surgery. The relatively recent commercial manufacture of nanoscale hydroxyapatite has provided surgeons with an injectable biomaterial that promotes bone tissue regeneration, and with further modification it may be possible to incorporate antimicrobial properties into these devices. Silver-doped nanoscale hydroxyapatite pastes (0, 2, 5 and 10 mol.% silver) were prepared using a rapid mixing method. When the process was modified to prepare a 10 mol.% silver-doped material, silver phosphate was detected in addition to nanoscale hydroxyapatite. Thermal decomposition occurred more readily with greater silver content following calcination at 1000 °C for 2 h. Silver-doped nanoscale hydroxyapatite pastes showed antibacterial activity against Staphylococcus aureus and Pseudomonas aeruginosa in a dose dependent manner using both agar diffusion assays and suspension cultures. It was concluded that the enhanced antibacterial activity of the silver-doped pastes was due to the action of diffusible silver ions. Based on these results, silver-doped nanoscale hydroxyapatite pastes represent a highly promising new biomaterial system for the prevention and treatment of deep infections in bone tissue.
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Rodriguez-Escontrela I, Puerto MC, Miller CA, Soto A. Ionic liquids for low-tension oil recovery processes: Phase behavior tests. J Colloid Interface Sci 2017; 504:404-416. [DOI: 10.1016/j.jcis.2017.05.102] [Citation(s) in RCA: 28] [Impact Index Per Article: 4.0] [Reference Citation Analysis] [What about the content of this article? (0)] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Received: 04/11/2017] [Revised: 05/24/2017] [Accepted: 05/25/2017] [Indexed: 11/25/2022]
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Ademuyiwa FO, Miller CA, Li T, Sanati S, Ma CX, Weilbaecher K, Ellis MJ, Mardis ER. Abstract P1-07-11: Tumor genomic profiling of triple negative breast cancer during neoadjuvant chemotherapy: Results from a prospective trial of carboplatin and docetaxel. Cancer Res 2017. [DOI: 10.1158/1538-7445.sabcs16-p1-07-11] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/16/2022]
Abstract
Abstract
Background-The clonal evolution and effect of neoadjuvant chemotherapy on the mutational landscape of triple negative breast cancer (TNBC) is unknown. Inability to eradicate TNBC may be due to clonal progression and selection of cells fundamentally resistant to chemotherapy.In this study, we sought to decipher the genomic architecture of TNBC serially during neoadjuvant chemotherapy to distinguish pre- versus post-chemotherapy genotypes.
Methods-Tumor specimens were obtained from patients with stages II and III TNBC enrolled on an ongoing prospective neoadjuvant co-clinical trial (NCT02124902). Patients have a research biopsy at baseline, cycle 1 day 3 (optional), and at definitive surgery for those with residual disease. Patients are treated with docetaxel 75mg/m2 and carboplatin AUC6 cycled every 3 weeks X six cycles. Definitive surgery is 3-5 weeks after chemotherapy. The primary endpoint is pathologic complete response rate. Correlative studies include development of patient derived xenografts, evaluation of genomic signatures of resistance and response, and comparison of chemotherapy responses between xenografts and host patients. Five patients' serial tumor samples and germline DNA were studied by exome and transcriptome sequencing. Three of these patients had an additional on-treatment sample at cycle 1 day 3. Two patients lacked residual disease samples- one was not banked and the other could not be accurately genotyped due to low cellularity. The median sequencing depth was 90.13x. Sequencing was performed on either fresh frozen or formalin-fixed paraffin-embedded samples with high cellularity (≥50%). After identifying somatic mutations in each tumor series, we evaluated whether each mutation was persistent, emergent, or cleared by comparing pre- and post-treatment (and when possible, on-treatment) samples.
Results-All five patients had response to neoadjuvant chemotherapy based on caliper-based and pathologic (residual cancer burden I or II) measurements. All residual disease remained TNBC by standard immunohistochemistry and all samples were basal-like from PAM50 gene expression analysis. We identified 908 somatic mutations, including the expected variants in TP53 which persisted in all post-treatment samples. Non-silent somatic variants were identified in other breast cancer-related genes, including GATA1, FBXO11, PIK3R1, AXIN2, ARID1B, BRCA2, and RBCC1. In spite of the clinico-pathologic evidence of response, we observed little change in clonal architecture, as derived from the purity-corrected variant allele fractions between baseline, cycle 1 day 3, and post-chemotherapy samples. Copy number alterations were likewise stable and transcriptional-based assessment indicated that patterns of mutant allele expression in driver genes were retained throughout the course of treatment.
Conclusion-In TNBC patients undergoing neoadjuvant platinum-based chemotherapy, there were no apparent shifts in the prevalence of known breast cancer specific somatic variants during or after chemotherapy. Despite pathologic response, core genomic features appear to be preserved in TNBC patients with residual disease following chemotherapy, likely accounting for high rates of relapse in these patients.
Citation Format: Ademuyiwa FO, Miller CA, Li T, Sanati S, Ma CX, Weilbaecher K, Ellis MJ, Mardis ER. Tumor genomic profiling of triple negative breast cancer during neoadjuvant chemotherapy: Results from a prospective trial of carboplatin and docetaxel [abstract]. In: Proceedings of the 2016 San Antonio Breast Cancer Symposium; 2016 Dec 6-10; San Antonio, TX. Philadelphia (PA): AACR; Cancer Res 2017;77(4 Suppl):Abstract nr P1-07-11.
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Affiliation(s)
- FO Ademuyiwa
- Washington Uni Sch of Medcn, St. Louis, MO; Baylor College of Medicine, Houston, TX
| | - CA Miller
- Washington Uni Sch of Medcn, St. Louis, MO; Baylor College of Medicine, Houston, TX
| | - T Li
- Washington Uni Sch of Medcn, St. Louis, MO; Baylor College of Medicine, Houston, TX
| | - S Sanati
- Washington Uni Sch of Medcn, St. Louis, MO; Baylor College of Medicine, Houston, TX
| | - CX Ma
- Washington Uni Sch of Medcn, St. Louis, MO; Baylor College of Medicine, Houston, TX
| | - K Weilbaecher
- Washington Uni Sch of Medcn, St. Louis, MO; Baylor College of Medicine, Houston, TX
| | - MJ Ellis
- Washington Uni Sch of Medcn, St. Louis, MO; Baylor College of Medicine, Houston, TX
| | - ER Mardis
- Washington Uni Sch of Medcn, St. Louis, MO; Baylor College of Medicine, Houston, TX
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11
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Haggarty RA, Miller CA, Scott EM. Spatially weighted functional clustering of river network data. J R Stat Soc Ser C Appl Stat 2015; 64:491-506. [PMID: 25926710 PMCID: PMC4407953 DOI: 10.1111/rssc.12082] [Citation(s) in RCA: 14] [Impact Index Per Article: 1.6] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Key Words] [Track Full Text] [Download PDF] [Figures] [Journal Information] [Subscribe] [Scholar Register] [Received: 02/01/2013] [Revised: 07/01/2014] [Indexed: 12/03/2022]
Abstract
Incorporating spatial covariance into clustering has previously been considered for functional data to identify groups of functions which are similar across space. However, in the majority of situations that have been considered until now the most appropriate metric has been Euclidean distance. Directed networks present additional challenges in terms of estimating spatial covariance due to their complex structure. Although suitable river network covariance models have been proposed for use with stream distance, where distance is computed along the stream network, these models have not been extended for contexts where the data are functional, as is often the case with environmental data. The paper develops a method of calculating spatial covariance between functions from sites along a river network and applies the measure as a weight within functional hierarchical clustering. Levels of nitrate pollution on the River Tweed in Scotland are considered with the aim of identifying groups of monitoring stations which display similar spatiotemporal characteristics.
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Engle EK, Fisher DAC, Miller CA, McLellan MD, Fulton RS, Moore DM, Wilson RK, Ley TJ, Oh ST. Clonal evolution revealed by whole genome sequencing in a case of primary myelofibrosis transformed to secondary acute myeloid leukemia. Leukemia 2015; 29:869-76. [PMID: 25252869 PMCID: PMC4374044 DOI: 10.1038/leu.2014.289] [Citation(s) in RCA: 41] [Impact Index Per Article: 4.6] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Key Words] [MESH Headings] [Grants] [Track Full Text] [Download PDF] [Figures] [Journal Information] [Subscribe] [Scholar Register] [Received: 08/27/2014] [Revised: 09/15/2014] [Accepted: 09/18/2014] [Indexed: 12/16/2022]
Abstract
Clonal architecture in myeloproliferative neoplasms (MPNs) is poorly understood. Here we report genomic analyses of a patient with primary myelofibrosis (PMF) transformed to secondary acute myeloid leukemia (sAML). Whole genome sequencing (WGS) was performed on PMF and sAML diagnosis samples, with skin included as a germline surrogate. Deep sequencing validation was performed on the WGS samples and an additional sample obtained during sAML remission/relapsed PMF. Clustering analysis of 649 validated somatic single-nucleotide variants revealed four distinct clonal groups, each including putative driver mutations. The first group (including JAK2 and U2AF1), representing the founding clone, included mutations with high frequency at all three disease stages. The second clonal group (including MYB) was present only in PMF, suggesting the presence of a clone that was dispensable for transformation. The third group (including ASXL1) contained mutations with low frequency in PMF and high frequency in subsequent samples, indicating evolution of the dominant clone with disease progression. The fourth clonal group (including IDH1 and RUNX1) was acquired at sAML transformation and was predominantly absent at sAML remission/relapsed PMF. Taken together, these findings illustrate the complex clonal dynamics associated with disease evolution in MPNs and sAML.
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Affiliation(s)
- E K Engle
- Division of Hematology, Washington University School of Medicine, St Louis, MO, USA
| | - D A C Fisher
- Division of Hematology, Washington University School of Medicine, St Louis, MO, USA
| | - C A Miller
- The Genome Institute, Washington University School of Medicine, St Louis, MO, USA
| | - M D McLellan
- The Genome Institute, Washington University School of Medicine, St Louis, MO, USA
| | - R S Fulton
- The Genome Institute, Washington University School of Medicine, St Louis, MO, USA
| | - D M Moore
- Division of Hematology, Washington University School of Medicine, St Louis, MO, USA
| | - R K Wilson
- The Genome Institute, Washington University School of Medicine, St Louis, MO, USA
| | - T J Ley
- The Genome Institute, Division of Oncology, Washington University School of Medicine, St Louis, MO, USA
| | - S T Oh
- Division of Hematology, Washington University School of Medicine, St Louis, MO, USA
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Kettridge N, Turetsky MR, Sherwood JH, Thompson DK, Miller CA, Benscoter BW, Flannigan MD, Wotton BM, Waddington JM. Moderate drop in water table increases peatland vulnerability to post-fire regime shift. Sci Rep 2015; 5:8063. [PMID: 25623290 PMCID: PMC4306970 DOI: 10.1038/srep08063] [Citation(s) in RCA: 96] [Impact Index Per Article: 10.7] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Download PDF] [Figures] [Journal Information] [Subscribe] [Scholar Register] [Received: 10/12/2014] [Accepted: 12/31/2014] [Indexed: 11/23/2022] Open
Abstract
Northern and tropical peatlands represent a globally significant carbon reserve accumulated over thousands of years of waterlogged conditions. It is unclear whether moderate drying predicted for northern peatlands will stimulate burning and carbon losses as has occurred in their smaller tropical counterparts where the carbon legacy has been destabilized due to severe drainage and deep peat fires. Capitalizing on a unique long-term experiment, we quantify the post-wildfire recovery of a northern peatland subjected to decadal drainage. We show that the moderate drop in water table position predicted for most northern regions triggers a shift in vegetation composition previously observed within only severely disturbed tropical peatlands. The combined impact of moderate drainage followed by wildfire converted the low productivity, moss-dominated peatland to a non-carbon accumulating shrub-grass ecosystem. This new ecosystem is likely to experience a low intensity, high frequency wildfire regime, which will further deplete the legacy of stored peat carbon.
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Affiliation(s)
- N Kettridge
- School of Geography, Earth and Environmental Sciences, University of Birmingham, Edgbaston, Birmingham, B15 2TT, UK
| | - M R Turetsky
- Department of Integrative Biology, University of Guelph, Guelph, Ontario, N1G 2W1, Canada
| | - J H Sherwood
- School of Geography and Earth Sciences, McMaster University, Hamilton, Ontario, L8S 4K1, Canada
| | - D K Thompson
- 1] School of Geography and Earth Sciences, McMaster University, Hamilton, Ontario, L8S 4K1, Canada [2] Natural Resources Canada, Canadian Forest Service, Northern Forestry Centre, Edmonton, Alberta, T6H 3S5, Canada
| | - C A Miller
- Department of Integrative Biology, University of Guelph, Guelph, Ontario, N1G 2W1, Canada
| | - B W Benscoter
- Department of Biological Sciences, Florida Atlantic University, Davie, Florida 33314, USA
| | - M D Flannigan
- 1] Natural Resources Canada, Canadian Forest Service, Northern Forestry Centre, Edmonton, Alberta, T6H 3S5, Canada [2] Department of Renewable Resources, University of Alberta, Edmonton, Alberta, T6G 2H1, Canada
| | - B M Wotton
- 1] Faculty of Forestry, University of Toronto, Toronto, Ontario, M5S 3B3, Canada [2] Natural Resources Canada, Canadian Forest Service, Great Lakes Forestry Centre, Sault Ste Marie, Ontario, P6A ZES, Canada
| | - J M Waddington
- School of Geography and Earth Sciences, McMaster University, Hamilton, Ontario, L8S 4K1, Canada
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Spencer DH, Young MA, Lamprecht TL, Helton NM, Fulton R, O'Laughlin M, Fronick C, Magrini V, Demeter RT, Miller CA, Klco JM, Wilson RK, Ley TJ. Epigenomic analysis of the HOX gene loci reveals mechanisms that may control canonical expression patterns in AML and normal hematopoietic cells. Leukemia 2015; 29:1279-89. [PMID: 25600023 DOI: 10.1038/leu.2015.6] [Citation(s) in RCA: 85] [Impact Index Per Article: 9.4] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Received: 10/01/2014] [Revised: 11/19/2014] [Accepted: 12/16/2014] [Indexed: 01/05/2023]
Abstract
HOX genes are highly expressed in many acute myeloid leukemia (AML) samples, but the patterns of expression and associated regulatory mechanisms are not clearly understood. We analyzed RNA sequencing data from 179 primary AML samples and normal hematopoietic cells to understand the range of expression patterns in normal versus leukemic cells. HOX expression in AML was restricted to specific genes in the HOXA or HOXB loci, and was highly correlated with recurrent cytogenetic abnormalities. However, the majority of samples expressed a canonical set of HOXA and HOXB genes that was nearly identical to the expression signature of normal hematopoietic stem/progenitor cells. Transcriptional profiles at the HOX loci were similar between normal cells and AML samples, and involved bidirectional transcription at the center of each gene cluster. Epigenetic analysis of a subset of AML samples also identified common regions of chromatin accessibility in AML samples and normal CD34(+) cells that displayed differences in methylation depending on HOX expression patterns. These data provide an integrated epigenetic view of the HOX gene loci in primary AML samples, and suggest that HOX expression in most AML samples represents a normal stem cell program that is controlled by epigenetic mechanisms at specific regulatory elements.
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Affiliation(s)
- D H Spencer
- Department of Pathology and Immunology, Washington University School of Medicine, St Louis, MO, USA
| | - M A Young
- Department of Pediatrics, Washington University School of Medicine, St Louis, MO, USA
| | - T L Lamprecht
- Department of Internal Medicine, Division of Oncology, Section of Stem Cell Biology, Washington University School of Medicine, St Louis, MO, USA
| | - N M Helton
- Department of Internal Medicine, Division of Oncology, Section of Stem Cell Biology, Washington University School of Medicine, St Louis, MO, USA
| | - R Fulton
- The Genome Institute, Washington University, St Louis, MO, USA
| | - M O'Laughlin
- The Genome Institute, Washington University, St Louis, MO, USA
| | - C Fronick
- The Genome Institute, Washington University, St Louis, MO, USA
| | - V Magrini
- The Genome Institute, Washington University, St Louis, MO, USA
| | - R T Demeter
- The Genome Institute, Washington University, St Louis, MO, USA
| | - C A Miller
- The Genome Institute, Washington University, St Louis, MO, USA
| | - J M Klco
- Department of Pathology and Immunology, Washington University School of Medicine, St Louis, MO, USA
| | - R K Wilson
- The Genome Institute, Washington University, St Louis, MO, USA
| | - T J Ley
- 1] Department of Internal Medicine, Division of Oncology, Section of Stem Cell Biology, Washington University School of Medicine, St Louis, MO, USA [2] The Genome Institute, Washington University, St Louis, MO, USA
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15
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Abe K, Adam J, Aihara H, Akiri T, Andreopoulos C, Aoki S, Ariga A, Assylbekov S, Autiero D, Barbi M, Barker GJ, Barr G, Bass M, Batkiewicz M, Bay F, Berardi V, Berger BE, Berkman S, Bhadra S, Blaszczyk FDM, Blondel A, Bojechko C, Bordoni S, Boyd SB, Brailsford D, Bravar A, Bronner C, Buchanan N, Calland RG, Caravaca Rodríguez J, Cartwright SL, Castillo R, Catanesi MG, Cervera A, Cherdack D, Christodoulou G, Clifton A, Coleman J, Coleman SJ, Collazuol G, Connolly K, Cremonesi L, Dabrowska A, Danko I, Das R, Davis S, de Perio P, De Rosa G, Dealtry T, Dennis SR, Densham C, Dewhurst D, Di Lodovico F, Di Luise S, Drapier O, Duboyski T, Duffy K, Dumarchez J, Dytman S, Dziewiecki M, Emery-Schrenk S, Ereditato A, Escudero L, Finch AJ, Friend M, Fujii Y, Fukuda Y, Furmanski AP, Galymov V, Giffin S, Giganti C, Gilje K, Goeldi D, Golan T, Gonin M, Grant N, Gudin D, Hadley DR, Haesler A, Haigh MD, Hamilton P, Hansen D, Hara T, Hartz M, Hasegawa T, Hastings NC, Hayato Y, Hearty C, Helmer RL, Hierholzer M, Hignight J, Hillairet A, Himmel A, Hiraki T, Hirota S, Holeczek J, Horikawa S, Huang K, Ichikawa AK, Ieki K, Ieva M, Ikeda M, Imber J, Insler J, Irvine TJ, Ishida T, Ishii T, Iwai E, Iwamoto K, Iyogi K, Izmaylov A, Jacob A, Jamieson B, Johnson RA, Jo JH, Jonsson P, Jung CK, Kabirnezhad M, Kaboth AC, Kajita T, Kakuno H, Kameda J, Kanazawa Y, Karlen D, Karpikov I, Katori T, Kearns E, Khabibullin M, Khotjantsev A, Kielczewska D, Kikawa T, Kilinski A, Kim J, Kisiel J, Kitching P, Kobayashi T, Koch L, Kolaceke A, Konaka A, Kormos LL, Korzenev A, Koshio Y, Kropp W, Kubo H, Kudenko Y, Kurjata R, Kutter T, Lagoda J, Lamont I, Larkin E, Laveder M, Lawe M, Lazos M, Lindner T, Lister C, Litchfield RP, Longhin A, Ludovici L, Magaletti L, Mahn K, Malek M, Manly S, Marino AD, Marteau J, Martin JF, Martynenko S, Maruyama T, Matveev V, Mavrokoridis K, Mazzucato E, McCarthy M, McCauley N, McFarland KS, McGrew C, Metelko C, Mijakowski P, Miller CA, Minamino A, Mineev O, Missert A, Miura M, Moriyama S, Mueller TA, Murakami A, Murdoch M, Murphy S, Myslik J, Nakadaira T, Nakahata M, Nakamura K, Nakayama S, Nakaya T, Nakayoshi K, Nielsen C, Nirkko M, Nishikawa K, Nishimura Y, O'Keeffe HM, Ohta R, Okumura K, Okusawa T, Oryszczak W, Oser SM, Owen RA, Oyama Y, Palladino V, Palomino JL, Paolone V, Payne D, Perevozchikov O, Perkin JD, Petrov Y, Pickard L, Pinzon Guerra ES, Pistillo C, Plonski P, Poplawska E, Popov B, Posiadala M, Poutissou JM, Poutissou R, Przewlocki P, Quilain B, Radicioni E, Ratoff PN, Ravonel M, Rayner MAM, Redij A, Reeves M, Reinherz-Aronis E, Rodrigues PA, Rojas P, Rondio E, Roth S, Rubbia A, Ruterbories D, Sacco R, Sakashita K, Sánchez F, Sato F, Scantamburlo E, Scholberg K, Schoppmann S, Schwehr J, Scott M, Seiya Y, Sekiguchi T, Sekiya H, Sgalaberna D, Shiozawa M, Short S, Shustrov Y, Sinclair P, Smith B, Smy M, Sobczyk JT, Sobel H, Sorel M, Southwell L, Stamoulis P, Steinmann J, Still B, Suda Y, Suzuki A, Suzuki K, Suzuki SY, Suzuki Y, Tacik R, Tada M, Takahashi S, Takeda A, Takeuchi Y, Tanaka HK, Tanaka HA, Tanaka MM, Terhorst D, Terri R, Thompson LF, Thorley A, Tobayama S, Toki W, Tomura T, Totsuka Y, Touramanis C, Tsukamoto T, Tzanov M, Uchida Y, Vacheret A, Vagins M, Vasseur G, Wachala T, Waldron AV, Walter CW, Wark D, Wascko MO, Weber A, Wendell R, Wilkes RJ, Wilking MJ, Wilkinson C, Williamson Z, Wilson JR, Wilson RJ, Wongjirad T, Yamada Y, Yamamoto K, Yanagisawa C, Yano T, Yen S, Yershov N, Yokoyama M, Yuan T, Yu M, Zalewska A, Zalipska J, Zambelli L, Zaremba K, Ziembicki M, Zimmerman ED, Zito M, Żmuda J. Measurement of the inclusive electron neutrino charged current cross section on carbon with the T2K near detector. Phys Rev Lett 2014; 113:241803. [PMID: 25541766 DOI: 10.1103/physrevlett.113.241803] [Citation(s) in RCA: 4] [Impact Index Per Article: 0.4] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Received: 07/28/2014] [Indexed: 06/04/2023]
Abstract
The T2K off-axis near detector ND280 is used to make the first differential cross-section measurements of electron neutrino charged current interactions at energies ∼1 GeV as a function of electron momentum, electron scattering angle, and four-momentum transfer of the interaction. The total flux-averaged ν(e) charged current cross section on carbon is measured to be ⟨σ⟩(ϕ)=1.11±0.10(stat)±0.18(syst)×10⁻³⁸ cm²/nucleon. The differential and total cross-section measurements agree with the predictions of two leading neutrino interaction generators, NEUT and GENIE. The NEUT prediction is 1.23×10⁻³⁸ cm²/nucleon and the GENIE prediction is 1.08×10⁻³⁸ cm²/nucleon. The total ν(e) charged current cross-section result is also in agreement with data from the Gargamelle experiment.
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Affiliation(s)
- K Abe
- Institute for Cosmic Ray Research, University of Tokyo, Kamioka Observatory, Kamioka, Japan
| | - J Adam
- Department of Physics and Astronomy, State University of New York at Stony Brook, Stony Brook, New York, USA
| | - H Aihara
- Kavli Institute for the Physics and Mathematics of the Universe (WPI), Todai Institutes for Advanced Study, University of Tokyo, Kashiwa, Chiba, Japan and Department of Physics, University of Tokyo, Tokyo, Japan
| | - T Akiri
- Department of Physics, Duke University, Durham, North Carolina, USA
| | - C Andreopoulos
- STFC, Rutherford Appleton Laboratory, Harwell Oxford, and Daresbury Laboratory, Warrington, United Kingdom
| | - S Aoki
- Kobe University, Kobe, Japan
| | - A Ariga
- Albert Einstein Center for Fundamental Physics, Laboratory for High Energy Physics (LHEP), University of Bern, Bern, Switzerland
| | - S Assylbekov
- Department of Physics, Colorado State University, Fort Collins, Colorado, USA
| | - D Autiero
- Université de Lyon, Université Claude Bernard Lyon 1, IPN Lyon (IN2P3), Villeurbanne, France
| | - M Barbi
- Department of Physics, University of Regina, Regina, Saskatchewan, Canada
| | - G J Barker
- Department of Physics, University of Warwick, Coventry, United Kingdom
| | - G Barr
- Department of Physics, Oxford University, Oxford, United Kingdom
| | - M Bass
- Department of Physics, Colorado State University, Fort Collins, Colorado, USA
| | - M Batkiewicz
- H. Niewodniczanski Institute of Nuclear Physics PAN, Cracow, Poland
| | - F Bay
- Institute for Particle Physics, ETH Zurich, Zurich, Switzerland
| | - V Berardi
- Dipartimento Interuniversitario di Fisica, INFN Sezione di Bari and Università e Politecnico di Bari, Bari, Italy
| | - B E Berger
- Department of Physics, Colorado State University, Fort Collins, Colorado, USA and Kavli Institute for the Physics and Mathematics of the Universe (WPI), Todai Institutes for Advanced Study, University of Tokyo, Kashiwa, Chiba, Japan
| | - S Berkman
- Department of Physics and Astronomy, University of British Columbia, Vancouver, British Columbia, Canada
| | - S Bhadra
- Department of Physics and Astronomy, York University, Toronto, Ontario, Canada
| | - F d M Blaszczyk
- Department of Physics and Astronomy, Louisiana State University, Baton Rouge, Louisiana, USA
| | - A Blondel
- Section de Physique, University of Geneva, DPNC, Geneva, Switzerland
| | - C Bojechko
- Department of Physics and Astronomy, University of Victoria, Victoria, British Columbia, Canada
| | - S Bordoni
- Institut de Fisica d'Altes Energies (IFAE), Bellaterra (Barcelona), Spain
| | - S B Boyd
- Department of Physics, University of Warwick, Coventry, United Kingdom
| | - D Brailsford
- Department of Physics, Imperial College London, London, United Kingdom
| | - A Bravar
- Section de Physique, University of Geneva, DPNC, Geneva, Switzerland
| | - C Bronner
- Kavli Institute for the Physics and Mathematics of the Universe (WPI), Todai Institutes for Advanced Study, University of Tokyo, Kashiwa, Chiba, Japan
| | - N Buchanan
- Department of Physics, Colorado State University, Fort Collins, Colorado, USA
| | - R G Calland
- Department of Physics, University of Liverpool, Liverpool, United Kingdom
| | | | - S L Cartwright
- Department of Physics and Astronomy, University of Sheffield, Sheffield, United Kingdom
| | - R Castillo
- Institut de Fisica d'Altes Energies (IFAE), Bellaterra (Barcelona), Spain
| | - M G Catanesi
- Dipartimento Interuniversitario di Fisica, INFN Sezione di Bari and Università e Politecnico di Bari, Bari, Italy
| | - A Cervera
- IFIC (CSIC & University of Valencia), Valencia, Spain
| | - D Cherdack
- Department of Physics, Colorado State University, Fort Collins, Colorado, USA
| | - G Christodoulou
- Department of Physics, University of Liverpool, Liverpool, United Kingdom
| | - A Clifton
- Department of Physics, Colorado State University, Fort Collins, Colorado, USA
| | - J Coleman
- Department of Physics, University of Liverpool, Liverpool, United Kingdom
| | - S J Coleman
- Department of Physics, University of Colorado at Boulder, Boulder, Colorado, USA
| | - G Collazuol
- Dipartimento di Fisica, INFN Sezione di Padova and Università di Padova, Padova, Italy
| | - K Connolly
- Department of Physics, University of Washington, Seattle, Washington, USA
| | - L Cremonesi
- School of Physics and Astronomy, Queen Mary University of London, London, United Kingdom
| | - A Dabrowska
- H. Niewodniczanski Institute of Nuclear Physics PAN, Cracow, Poland
| | - I Danko
- Department of Physics and Astronomy, University of Pittsburgh, Pittsburgh, Pennsylvania, USA
| | - R Das
- Department of Physics, Colorado State University, Fort Collins, Colorado, USA
| | - S Davis
- Department of Physics, University of Washington, Seattle, Washington, USA
| | - P de Perio
- Department of Physics, University of Toronto, Toronto, Ontario, Canada
| | - G De Rosa
- Dipartimento di Fisica, INFN Sezione di Napoli and Università di Napoli, Napoli, Italy
| | - T Dealtry
- Department of Physics, Oxford University, Oxford, United Kingdom and STFC, Rutherford Appleton Laboratory, Harwell Oxford, and Daresbury Laboratory, Warrington, United Kingdom
| | - S R Dennis
- STFC, Rutherford Appleton Laboratory, Harwell Oxford, and Daresbury Laboratory, Warrington, United Kingdom and Department of Physics, University of Warwick, Coventry, United Kingdom
| | - C Densham
- STFC, Rutherford Appleton Laboratory, Harwell Oxford, and Daresbury Laboratory, Warrington, United Kingdom
| | - D Dewhurst
- Department of Physics, Oxford University, Oxford, United Kingdom
| | - F Di Lodovico
- School of Physics and Astronomy, Queen Mary University of London, London, United Kingdom
| | - S Di Luise
- Institute for Particle Physics, ETH Zurich, Zurich, Switzerland
| | - O Drapier
- Laboratoire Leprince-Ringuet, Ecole Polytechnique, IN2P3-CNRS, Palaiseau, France
| | - T Duboyski
- School of Physics and Astronomy, Queen Mary University of London, London, United Kingdom
| | - K Duffy
- Department of Physics, Oxford University, Oxford, United Kingdom
| | - J Dumarchez
- Laboratoire de Physique Nucléaire et de Hautes Energies (LPNHE), UPMC, Université Paris Diderot, CNRS/IN2P3, Paris, France
| | - S Dytman
- Department of Physics and Astronomy, University of Pittsburgh, Pittsburgh, Pennsylvania, USA
| | - M Dziewiecki
- Institute of Radioelectronics, Warsaw University of Technology, Warsaw, Poland
| | | | - A Ereditato
- Albert Einstein Center for Fundamental Physics, Laboratory for High Energy Physics (LHEP), University of Bern, Bern, Switzerland
| | - L Escudero
- IFIC (CSIC & University of Valencia), Valencia, Spain
| | - A J Finch
- Physics Department, Lancaster University, Lancaster, United Kingdom
| | - M Friend
- High Energy Accelerator Research Organization (KEK), Tsukuba, Ibaraki, Japan
| | - Y Fujii
- High Energy Accelerator Research Organization (KEK), Tsukuba, Ibaraki, Japan
| | - Y Fukuda
- Department of Physics, Miyagi University of Education, Sendai, Japan
| | - A P Furmanski
- Department of Physics, University of Warwick, Coventry, United Kingdom
| | - V Galymov
- Université de Lyon, Université Claude Bernard Lyon 1, IPN Lyon (IN2P3), Villeurbanne, France
| | - S Giffin
- Department of Physics, University of Regina, Regina, Saskatchewan, Canada
| | - C Giganti
- Laboratoire de Physique Nucléaire et de Hautes Energies (LPNHE), UPMC, Université Paris Diderot, CNRS/IN2P3, Paris, France
| | - K Gilje
- Department of Physics and Astronomy, State University of New York at Stony Brook, Stony Brook, New York, USA
| | - D Goeldi
- Albert Einstein Center for Fundamental Physics, Laboratory for High Energy Physics (LHEP), University of Bern, Bern, Switzerland
| | - T Golan
- Faculty of Physics and Astronomy, Wroclaw University, Wroclaw, Poland
| | - M Gonin
- Laboratoire Leprince-Ringuet, Ecole Polytechnique, IN2P3-CNRS, Palaiseau, France
| | - N Grant
- Physics Department, Lancaster University, Lancaster, United Kingdom
| | - D Gudin
- Institute for Nuclear Research of the Russian Academy of Sciences, Moscow, Russia
| | - D R Hadley
- Department of Physics, University of Warwick, Coventry, United Kingdom
| | - A Haesler
- Section de Physique, University of Geneva, DPNC, Geneva, Switzerland
| | - M D Haigh
- Department of Physics, University of Warwick, Coventry, United Kingdom
| | - P Hamilton
- Department of Physics, Imperial College London, London, United Kingdom
| | - D Hansen
- Department of Physics and Astronomy, University of Pittsburgh, Pittsburgh, Pennsylvania, USA
| | - T Hara
- Kobe University, Kobe, Japan
| | - M Hartz
- Kavli Institute for the Physics and Mathematics of the Universe (WPI), Todai Institutes for Advanced Study, University of Tokyo, Kashiwa, Chiba, Japan and TRIUMF, Vancouver, British Columbia, Canada
| | - T Hasegawa
- High Energy Accelerator Research Organization (KEK), Tsukuba, Ibaraki, Japan
| | - N C Hastings
- Department of Physics, University of Regina, Regina, Saskatchewan, Canada
| | - Y Hayato
- Kavli Institute for the Physics and Mathematics of the Universe (WPI), Todai Institutes for Advanced Study, University of Tokyo, Kashiwa, Chiba, Japan and Institute for Cosmic Ray Research, University of Tokyo, Kamioka Observatory, Kamioka, Japan
| | - C Hearty
- Department of Physics and Astronomy, University of British Columbia, Vancouver, British Columbia, Canada
| | - R L Helmer
- TRIUMF, Vancouver, British Columbia, Canada
| | - M Hierholzer
- Albert Einstein Center for Fundamental Physics, Laboratory for High Energy Physics (LHEP), University of Bern, Bern, Switzerland
| | - J Hignight
- Department of Physics and Astronomy, State University of New York at Stony Brook, Stony Brook, New York, USA
| | - A Hillairet
- Department of Physics and Astronomy, University of Victoria, Victoria, British Columbia, Canada
| | - A Himmel
- Department of Physics, Duke University, Durham, North Carolina, USA
| | - T Hiraki
- Department of Physics, Kyoto University, Kyoto, Japan
| | - S Hirota
- Department of Physics, Kyoto University, Kyoto, Japan
| | - J Holeczek
- Institute of Physics, University of Silesia, Katowice, Poland
| | - S Horikawa
- Institute for Particle Physics, ETH Zurich, Zurich, Switzerland
| | - K Huang
- Department of Physics, Kyoto University, Kyoto, Japan
| | - A K Ichikawa
- Department of Physics, Kyoto University, Kyoto, Japan
| | - K Ieki
- Department of Physics, Kyoto University, Kyoto, Japan
| | - M Ieva
- Institut de Fisica d'Altes Energies (IFAE), Bellaterra (Barcelona), Spain
| | - M Ikeda
- Institute for Cosmic Ray Research, University of Tokyo, Kamioka Observatory, Kamioka, Japan
| | - J Imber
- Department of Physics and Astronomy, State University of New York at Stony Brook, Stony Brook, New York, USA
| | - J Insler
- Department of Physics and Astronomy, Louisiana State University, Baton Rouge, Louisiana, USA
| | - T J Irvine
- Institute for Cosmic Ray Research, University of Tokyo, Research Center for Cosmic Neutrinos, Kashiwa, Japan
| | - T Ishida
- High Energy Accelerator Research Organization (KEK), Tsukuba, Ibaraki, Japan
| | - T Ishii
- High Energy Accelerator Research Organization (KEK), Tsukuba, Ibaraki, Japan
| | - E Iwai
- High Energy Accelerator Research Organization (KEK), Tsukuba, Ibaraki, Japan
| | - K Iwamoto
- Department of Physics and Astronomy, University of Rochester, Rochester, New York, USA
| | - K Iyogi
- Institute for Cosmic Ray Research, University of Tokyo, Kamioka Observatory, Kamioka, Japan
| | - A Izmaylov
- IFIC (CSIC & University of Valencia), Valencia, Spain and Institute for Nuclear Research of the Russian Academy of Sciences, Moscow, Russia
| | - A Jacob
- Department of Physics, Oxford University, Oxford, United Kingdom
| | - B Jamieson
- Department of Physics, University of Winnipeg, Winnipeg, Manitoba, Canada
| | - R A Johnson
- Department of Physics, University of Colorado at Boulder, Boulder, Colorado, USA
| | - J H Jo
- Department of Physics and Astronomy, State University of New York at Stony Brook, Stony Brook, New York, USA
| | - P Jonsson
- Department of Physics, Imperial College London, London, United Kingdom
| | - C K Jung
- Department of Physics and Astronomy, State University of New York at Stony Brook, Stony Brook, New York, USA
| | - M Kabirnezhad
- National Centre for Nuclear Research, Warsaw, Poland
| | - A C Kaboth
- Department of Physics, Imperial College London, London, United Kingdom
| | - T Kajita
- Institute for Cosmic Ray Research, University of Tokyo, Research Center for Cosmic Neutrinos, Kashiwa, Japan
| | - H Kakuno
- Department of Physics, Tokyo Metropolitan University, Tokyo, Japan
| | - J Kameda
- Institute for Cosmic Ray Research, University of Tokyo, Kamioka Observatory, Kamioka, Japan
| | - Y Kanazawa
- Department of Physics, University of Tokyo, Tokyo, Japan
| | - D Karlen
- TRIUMF, Vancouver, British Columbia, Canada and Department of Physics and Astronomy, University of Victoria, Victoria, British Columbia, Canada
| | - I Karpikov
- Institute for Nuclear Research of the Russian Academy of Sciences, Moscow, Russia
| | - T Katori
- School of Physics and Astronomy, Queen Mary University of London, London, United Kingdom
| | - E Kearns
- Department of Physics, Boston University, Boston, Massachusetts, USA and Kavli Institute for the Physics and Mathematics of the Universe (WPI), Todai Institutes for Advanced Study, University of Tokyo, Kashiwa, Chiba, Japan
| | - M Khabibullin
- Institute for Nuclear Research of the Russian Academy of Sciences, Moscow, Russia
| | - A Khotjantsev
- Institute for Nuclear Research of the Russian Academy of Sciences, Moscow, Russia
| | - D Kielczewska
- Faculty of Physics, University of Warsaw, Warsaw, Poland
| | - T Kikawa
- Department of Physics, Kyoto University, Kyoto, Japan
| | - A Kilinski
- National Centre for Nuclear Research, Warsaw, Poland
| | - J Kim
- Department of Physics and Astronomy, University of British Columbia, Vancouver, British Columbia, Canada
| | - J Kisiel
- Institute of Physics, University of Silesia, Katowice, Poland
| | - P Kitching
- Department of Physics, University of Alberta, Centre for Particle Physics, Edmonton, Alberta, Canada
| | - T Kobayashi
- High Energy Accelerator Research Organization (KEK), Tsukuba, Ibaraki, Japan
| | - L Koch
- RWTH Aachen University, III. Physikalisches Institut, Aachen, Germany
| | - A Kolaceke
- Department of Physics, University of Regina, Regina, Saskatchewan, Canada
| | - A Konaka
- TRIUMF, Vancouver, British Columbia, Canada
| | - L L Kormos
- Physics Department, Lancaster University, Lancaster, United Kingdom
| | - A Korzenev
- Section de Physique, University of Geneva, DPNC, Geneva, Switzerland
| | - Y Koshio
- Department of Physics, Okayama University, Okayama, Japan
| | - W Kropp
- Department of Physics and Astronomy, University of California, Irvine, Irvine, California, USA
| | - H Kubo
- Department of Physics, Kyoto University, Kyoto, Japan
| | - Y Kudenko
- Institute for Nuclear Research of the Russian Academy of Sciences, Moscow, Russia
| | - R Kurjata
- Institute of Radioelectronics, Warsaw University of Technology, Warsaw, Poland
| | - T Kutter
- Department of Physics and Astronomy, Louisiana State University, Baton Rouge, Louisiana, USA
| | - J Lagoda
- National Centre for Nuclear Research, Warsaw, Poland
| | - I Lamont
- Physics Department, Lancaster University, Lancaster, United Kingdom
| | - E Larkin
- Department of Physics, University of Warwick, Coventry, United Kingdom
| | - M Laveder
- Dipartimento di Fisica, INFN Sezione di Padova and Università di Padova, Padova, Italy
| | - M Lawe
- Department of Physics and Astronomy, University of Sheffield, Sheffield, United Kingdom
| | - M Lazos
- Department of Physics, University of Liverpool, Liverpool, United Kingdom
| | - T Lindner
- TRIUMF, Vancouver, British Columbia, Canada
| | - C Lister
- Department of Physics, University of Warwick, Coventry, United Kingdom
| | - R P Litchfield
- Department of Physics, University of Warwick, Coventry, United Kingdom
| | - A Longhin
- Dipartimento di Fisica, INFN Sezione di Padova and Università di Padova, Padova, Italy
| | - L Ludovici
- INFN Sezione di Roma and Università di Roma "La Sapienza", Roma, Italy
| | - L Magaletti
- Dipartimento Interuniversitario di Fisica, INFN Sezione di Bari and Università e Politecnico di Bari, Bari, Italy
| | - K Mahn
- TRIUMF, Vancouver, British Columbia, Canada
| | - M Malek
- Department of Physics, Imperial College London, London, United Kingdom
| | - S Manly
- Department of Physics and Astronomy, University of Rochester, Rochester, New York, USA
| | - A D Marino
- Department of Physics, University of Colorado at Boulder, Boulder, Colorado, USA
| | - J Marteau
- Université de Lyon, Université Claude Bernard Lyon 1, IPN Lyon (IN2P3), Villeurbanne, France
| | - J F Martin
- Department of Physics, University of Toronto, Toronto, Ontario, Canada
| | - S Martynenko
- Institute for Nuclear Research of the Russian Academy of Sciences, Moscow, Russia
| | - T Maruyama
- High Energy Accelerator Research Organization (KEK), Tsukuba, Ibaraki, Japan
| | - V Matveev
- Institute for Nuclear Research of the Russian Academy of Sciences, Moscow, Russia
| | - K Mavrokoridis
- Department of Physics, University of Liverpool, Liverpool, United Kingdom
| | | | - M McCarthy
- Department of Physics and Astronomy, University of British Columbia, Vancouver, British Columbia, Canada
| | - N McCauley
- Department of Physics, University of Liverpool, Liverpool, United Kingdom
| | - K S McFarland
- Department of Physics and Astronomy, University of Rochester, Rochester, New York, USA
| | - C McGrew
- Department of Physics and Astronomy, State University of New York at Stony Brook, Stony Brook, New York, USA
| | - C Metelko
- Department of Physics, University of Liverpool, Liverpool, United Kingdom
| | - P Mijakowski
- National Centre for Nuclear Research, Warsaw, Poland
| | - C A Miller
- TRIUMF, Vancouver, British Columbia, Canada
| | - A Minamino
- Department of Physics, Kyoto University, Kyoto, Japan
| | - O Mineev
- Institute for Nuclear Research of the Russian Academy of Sciences, Moscow, Russia
| | - A Missert
- Department of Physics, University of Colorado at Boulder, Boulder, Colorado, USA
| | - M Miura
- Institute for Cosmic Ray Research, University of Tokyo, Kamioka Observatory, Kamioka, Japan
| | - S Moriyama
- Institute for Cosmic Ray Research, University of Tokyo, Kamioka Observatory, Kamioka, Japan
| | - Th A Mueller
- Laboratoire Leprince-Ringuet, Ecole Polytechnique, IN2P3-CNRS, Palaiseau, France
| | - A Murakami
- Department of Physics, Kyoto University, Kyoto, Japan
| | - M Murdoch
- Department of Physics, University of Liverpool, Liverpool, United Kingdom
| | - S Murphy
- Institute for Particle Physics, ETH Zurich, Zurich, Switzerland
| | - J Myslik
- Department of Physics and Astronomy, University of Victoria, Victoria, British Columbia, Canada
| | - T Nakadaira
- High Energy Accelerator Research Organization (KEK), Tsukuba, Ibaraki, Japan
| | - M Nakahata
- Kavli Institute for the Physics and Mathematics of the Universe (WPI), Todai Institutes for Advanced Study, University of Tokyo, Kashiwa, Chiba, Japan and Institute for Cosmic Ray Research, University of Tokyo, Kamioka Observatory, Kamioka, Japan
| | - K Nakamura
- High Energy Accelerator Research Organization (KEK), Tsukuba, Ibaraki, Japan and Kavli Institute for the Physics and Mathematics of the Universe (WPI), Todai Institutes for Advanced Study, University of Tokyo, Kashiwa, Chiba, Japan
| | - S Nakayama
- Institute for Cosmic Ray Research, University of Tokyo, Kamioka Observatory, Kamioka, Japan
| | - T Nakaya
- Kavli Institute for the Physics and Mathematics of the Universe (WPI), Todai Institutes for Advanced Study, University of Tokyo, Kashiwa, Chiba, Japan and Department of Physics, Kyoto University, Kyoto, Japan
| | - K Nakayoshi
- High Energy Accelerator Research Organization (KEK), Tsukuba, Ibaraki, Japan
| | - C Nielsen
- Department of Physics and Astronomy, University of British Columbia, Vancouver, British Columbia, Canada
| | - M Nirkko
- Albert Einstein Center for Fundamental Physics, Laboratory for High Energy Physics (LHEP), University of Bern, Bern, Switzerland
| | - K Nishikawa
- High Energy Accelerator Research Organization (KEK), Tsukuba, Ibaraki, Japan
| | - Y Nishimura
- Institute for Cosmic Ray Research, University of Tokyo, Research Center for Cosmic Neutrinos, Kashiwa, Japan
| | - H M O'Keeffe
- Physics Department, Lancaster University, Lancaster, United Kingdom
| | - R Ohta
- High Energy Accelerator Research Organization (KEK), Tsukuba, Ibaraki, Japan
| | - K Okumura
- Kavli Institute for the Physics and Mathematics of the Universe (WPI), Todai Institutes for Advanced Study, University of Tokyo, Kashiwa, Chiba, Japan and Institute for Cosmic Ray Research, University of Tokyo, Research Center for Cosmic Neutrinos, Kashiwa, Japan
| | - T Okusawa
- Department of Physics, Osaka City University, Osaka, Japan
| | - W Oryszczak
- Faculty of Physics, University of Warsaw, Warsaw, Poland
| | - S M Oser
- Department of Physics and Astronomy, University of British Columbia, Vancouver, British Columbia, Canada
| | - R A Owen
- School of Physics and Astronomy, Queen Mary University of London, London, United Kingdom
| | - Y Oyama
- High Energy Accelerator Research Organization (KEK), Tsukuba, Ibaraki, Japan
| | - V Palladino
- Dipartimento di Fisica, INFN Sezione di Napoli and Università di Napoli, Napoli, Italy
| | - J L Palomino
- Department of Physics and Astronomy, State University of New York at Stony Brook, Stony Brook, New York, USA
| | - V Paolone
- Department of Physics and Astronomy, University of Pittsburgh, Pittsburgh, Pennsylvania, USA
| | - D Payne
- Department of Physics, University of Liverpool, Liverpool, United Kingdom
| | - O Perevozchikov
- Department of Physics and Astronomy, Louisiana State University, Baton Rouge, Louisiana, USA
| | - J D Perkin
- Department of Physics and Astronomy, University of Sheffield, Sheffield, United Kingdom
| | - Y Petrov
- Department of Physics and Astronomy, University of British Columbia, Vancouver, British Columbia, Canada
| | - L Pickard
- Department of Physics and Astronomy, University of Sheffield, Sheffield, United Kingdom
| | - E S Pinzon Guerra
- Department of Physics and Astronomy, York University, Toronto, Ontario, Canada
| | - C Pistillo
- Albert Einstein Center for Fundamental Physics, Laboratory for High Energy Physics (LHEP), University of Bern, Bern, Switzerland
| | - P Plonski
- Institute of Radioelectronics, Warsaw University of Technology, Warsaw, Poland
| | - E Poplawska
- School of Physics and Astronomy, Queen Mary University of London, London, United Kingdom
| | - B Popov
- Laboratoire de Physique Nucléaire et de Hautes Energies (LPNHE), UPMC, Université Paris Diderot, CNRS/IN2P3, Paris, France
| | - M Posiadala
- Faculty of Physics, University of Warsaw, Warsaw, Poland
| | | | | | - P Przewlocki
- National Centre for Nuclear Research, Warsaw, Poland
| | - B Quilain
- Laboratoire Leprince-Ringuet, Ecole Polytechnique, IN2P3-CNRS, Palaiseau, France
| | - E Radicioni
- Dipartimento Interuniversitario di Fisica, INFN Sezione di Bari and Università e Politecnico di Bari, Bari, Italy
| | - P N Ratoff
- Physics Department, Lancaster University, Lancaster, United Kingdom
| | - M Ravonel
- Section de Physique, University of Geneva, DPNC, Geneva, Switzerland
| | - M A M Rayner
- Section de Physique, University of Geneva, DPNC, Geneva, Switzerland
| | - A Redij
- Albert Einstein Center for Fundamental Physics, Laboratory for High Energy Physics (LHEP), University of Bern, Bern, Switzerland
| | - M Reeves
- Physics Department, Lancaster University, Lancaster, United Kingdom
| | - E Reinherz-Aronis
- Department of Physics, Colorado State University, Fort Collins, Colorado, USA
| | - P A Rodrigues
- Department of Physics and Astronomy, University of Rochester, Rochester, New York, USA
| | - P Rojas
- Department of Physics, Colorado State University, Fort Collins, Colorado, USA
| | - E Rondio
- National Centre for Nuclear Research, Warsaw, Poland
| | - S Roth
- RWTH Aachen University, III. Physikalisches Institut, Aachen, Germany
| | - A Rubbia
- Institute for Particle Physics, ETH Zurich, Zurich, Switzerland
| | - D Ruterbories
- Department of Physics and Astronomy, University of Rochester, Rochester, New York, USA
| | - R Sacco
- School of Physics and Astronomy, Queen Mary University of London, London, United Kingdom
| | - K Sakashita
- High Energy Accelerator Research Organization (KEK), Tsukuba, Ibaraki, Japan
| | - F Sánchez
- Institut de Fisica d'Altes Energies (IFAE), Bellaterra (Barcelona), Spain
| | - F Sato
- High Energy Accelerator Research Organization (KEK), Tsukuba, Ibaraki, Japan
| | - E Scantamburlo
- Section de Physique, University of Geneva, DPNC, Geneva, Switzerland
| | - K Scholberg
- Department of Physics, Duke University, Durham, North Carolina, USA
| | - S Schoppmann
- RWTH Aachen University, III. Physikalisches Institut, Aachen, Germany
| | - J Schwehr
- Department of Physics, Colorado State University, Fort Collins, Colorado, USA
| | - M Scott
- TRIUMF, Vancouver, British Columbia, Canada
| | - Y Seiya
- Department of Physics, Osaka City University, Osaka, Japan
| | - T Sekiguchi
- High Energy Accelerator Research Organization (KEK), Tsukuba, Ibaraki, Japan
| | - H Sekiya
- Institute for Cosmic Ray Research, University of Tokyo, Kamioka Observatory, Kamioka, Japan
| | - D Sgalaberna
- Institute for Particle Physics, ETH Zurich, Zurich, Switzerland
| | - M Shiozawa
- Kavli Institute for the Physics and Mathematics of the Universe (WPI), Todai Institutes for Advanced Study, University of Tokyo, Kashiwa, Chiba, Japan and Institute for Cosmic Ray Research, University of Tokyo, Kamioka Observatory, Kamioka, Japan
| | - S Short
- School of Physics and Astronomy, Queen Mary University of London, London, United Kingdom
| | - Y Shustrov
- Institute for Nuclear Research of the Russian Academy of Sciences, Moscow, Russia
| | - P Sinclair
- Department of Physics, Imperial College London, London, United Kingdom
| | - B Smith
- Department of Physics, Imperial College London, London, United Kingdom
| | - M Smy
- Department of Physics and Astronomy, University of California, Irvine, Irvine, California, USA
| | - J T Sobczyk
- Faculty of Physics and Astronomy, Wroclaw University, Wroclaw, Poland
| | - H Sobel
- Department of Physics and Astronomy, University of California, Irvine, Irvine, California, USA and Kavli Institute for the Physics and Mathematics of the Universe (WPI), Todai Institutes for Advanced Study, University of Tokyo, Kashiwa, Chiba, Japan
| | - M Sorel
- IFIC (CSIC & University of Valencia), Valencia, Spain
| | - L Southwell
- Physics Department, Lancaster University, Lancaster, United Kingdom
| | - P Stamoulis
- IFIC (CSIC & University of Valencia), Valencia, Spain
| | - J Steinmann
- RWTH Aachen University, III. Physikalisches Institut, Aachen, Germany
| | - B Still
- School of Physics and Astronomy, Queen Mary University of London, London, United Kingdom
| | - Y Suda
- Department of Physics, University of Tokyo, Tokyo, Japan
| | | | - K Suzuki
- Department of Physics, Kyoto University, Kyoto, Japan
| | - S Y Suzuki
- High Energy Accelerator Research Organization (KEK), Tsukuba, Ibaraki, Japan
| | - Y Suzuki
- Kavli Institute for the Physics and Mathematics of the Universe (WPI), Todai Institutes for Advanced Study, University of Tokyo, Kashiwa, Chiba, Japan
| | - R Tacik
- Department of Physics, University of Regina, Regina, Saskatchewan, Canada and TRIUMF, Vancouver, British Columbia, Canada
| | - M Tada
- High Energy Accelerator Research Organization (KEK), Tsukuba, Ibaraki, Japan
| | - S Takahashi
- Department of Physics, Kyoto University, Kyoto, Japan
| | - A Takeda
- Institute for Cosmic Ray Research, University of Tokyo, Kamioka Observatory, Kamioka, Japan
| | - Y Takeuchi
- Kavli Institute for the Physics and Mathematics of the Universe (WPI), Todai Institutes for Advanced Study, University of Tokyo, Kashiwa, Chiba, Japan and Kobe University, Kobe, Japan
| | - H K Tanaka
- Institute for Cosmic Ray Research, University of Tokyo, Kamioka Observatory, Kamioka, Japan
| | - H A Tanaka
- Department of Physics and Astronomy, University of British Columbia, Vancouver, British Columbia, Canada
| | - M M Tanaka
- High Energy Accelerator Research Organization (KEK), Tsukuba, Ibaraki, Japan
| | - D Terhorst
- RWTH Aachen University, III. Physikalisches Institut, Aachen, Germany
| | - R Terri
- School of Physics and Astronomy, Queen Mary University of London, London, United Kingdom
| | - L F Thompson
- Department of Physics and Astronomy, University of Sheffield, Sheffield, United Kingdom
| | - A Thorley
- Department of Physics, University of Liverpool, Liverpool, United Kingdom
| | - S Tobayama
- Department of Physics and Astronomy, University of British Columbia, Vancouver, British Columbia, Canada
| | - W Toki
- Department of Physics, Colorado State University, Fort Collins, Colorado, USA
| | - T Tomura
- Institute for Cosmic Ray Research, University of Tokyo, Kamioka Observatory, Kamioka, Japan
| | - Y Totsuka
- Department of Physics, University of Alberta, Centre for Particle Physics, Edmonton, Alberta, Canada
| | - C Touramanis
- Department of Physics, University of Liverpool, Liverpool, United Kingdom
| | - T Tsukamoto
- High Energy Accelerator Research Organization (KEK), Tsukuba, Ibaraki, Japan
| | - M Tzanov
- Department of Physics and Astronomy, Louisiana State University, Baton Rouge, Louisiana, USA
| | - Y Uchida
- Department of Physics, Imperial College London, London, United Kingdom
| | - A Vacheret
- Department of Physics, Oxford University, Oxford, United Kingdom
| | - M Vagins
- Department of Physics and Astronomy, University of California, Irvine, Irvine, California, USA and Kavli Institute for the Physics and Mathematics of the Universe (WPI), Todai Institutes for Advanced Study, University of Tokyo, Kashiwa, Chiba, Japan
| | - G Vasseur
- IRFU, CEA Saclay, Gif-sur-Yvette, France
| | - T Wachala
- H. Niewodniczanski Institute of Nuclear Physics PAN, Cracow, Poland
| | - A V Waldron
- Department of Physics, Oxford University, Oxford, United Kingdom
| | - C W Walter
- Department of Physics, Duke University, Durham, North Carolina, USA
| | - D Wark
- Department of Physics, Imperial College London, London, United Kingdom and STFC, Rutherford Appleton Laboratory, Harwell Oxford, and Daresbury Laboratory, Warrington, United Kingdom
| | - M O Wascko
- Department of Physics, Imperial College London, London, United Kingdom
| | - A Weber
- Department of Physics, Oxford University, Oxford, United Kingdom and STFC, Rutherford Appleton Laboratory, Harwell Oxford, and Daresbury Laboratory, Warrington, United Kingdom
| | - R Wendell
- Institute for Cosmic Ray Research, University of Tokyo, Kamioka Observatory, Kamioka, Japan
| | - R J Wilkes
- Department of Physics, University of Washington, Seattle, Washington, USA
| | | | - C Wilkinson
- Department of Physics and Astronomy, University of Sheffield, Sheffield, United Kingdom
| | - Z Williamson
- Department of Physics, Oxford University, Oxford, United Kingdom
| | - J R Wilson
- School of Physics and Astronomy, Queen Mary University of London, London, United Kingdom
| | - R J Wilson
- Department of Physics, Colorado State University, Fort Collins, Colorado, USA
| | - T Wongjirad
- Department of Physics, Duke University, Durham, North Carolina, USA
| | - Y Yamada
- High Energy Accelerator Research Organization (KEK), Tsukuba, Ibaraki, Japan
| | - K Yamamoto
- Department of Physics, Osaka City University, Osaka, Japan
| | - C Yanagisawa
- Department of Physics and Astronomy, State University of New York at Stony Brook, Stony Brook, New York, USA
| | - T Yano
- Kobe University, Kobe, Japan
| | - S Yen
- TRIUMF, Vancouver, British Columbia, Canada
| | - N Yershov
- Institute for Nuclear Research of the Russian Academy of Sciences, Moscow, Russia
| | - M Yokoyama
- Department of Physics, University of Tokyo, Tokyo, Japan
| | - T Yuan
- Department of Physics, University of Colorado at Boulder, Boulder, Colorado, USA
| | - M Yu
- Department of Physics and Astronomy, York University, Toronto, Ontario, Canada
| | - A Zalewska
- H. Niewodniczanski Institute of Nuclear Physics PAN, Cracow, Poland
| | - J Zalipska
- National Centre for Nuclear Research, Warsaw, Poland
| | - L Zambelli
- High Energy Accelerator Research Organization (KEK), Tsukuba, Ibaraki, Japan
| | - K Zaremba
- Institute of Radioelectronics, Warsaw University of Technology, Warsaw, Poland
| | - M Ziembicki
- Institute of Radioelectronics, Warsaw University of Technology, Warsaw, Poland
| | - E D Zimmerman
- Department of Physics, University of Colorado at Boulder, Boulder, Colorado, USA
| | - M Zito
- IRFU, CEA Saclay, Gif-sur-Yvette, France
| | - J Żmuda
- Faculty of Physics and Astronomy, Wroclaw University, Wroclaw, Poland
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16
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Abe K, Adam J, Aihara H, Akiri T, Andreopoulos C, Aoki S, Ariga A, Ariga T, Assylbekov S, Autiero D, Barbi M, Barker GJ, Barr G, Bass M, Batkiewicz M, Bay F, Bentham SW, Berardi V, Berger BE, Berkman S, Bertram I, Bhadra S, Blaszczyk FDM, Blondel A, Bojechko C, Bordoni S, Boyd SB, Brailsford D, Bravar A, Bronner C, Buchanan N, Calland RG, Caravaca Rodríguez J, Cartwright SL, Castillo R, Catanesi MG, Cervera A, Cherdack D, Christodoulou G, Clifton A, Coleman J, Coleman SJ, Collazuol G, Connolly K, Cremonesi L, Dabrowska A, Danko I, Das R, Davis S, de Perio P, De Rosa G, Dealtry T, Dennis SR, Densham C, Di Lodovico F, Di Luise S, Drapier O, Duboyski T, Duffy K, Dufour F, Dumarchez J, Dytman S, Dziewiecki M, Emery S, Ereditato A, Escudero L, Finch AJ, Floetotto L, Friend M, Fujii Y, Fukuda Y, Furmanski AP, Galymov V, Giffin S, Giganti C, Gilje K, Goeldi D, Golan T, Gonin M, Grant N, Gudin D, Hadley DR, Haesler A, Haigh MD, Hamilton P, Hansen D, Hara T, Hartz M, Hasegawa T, Hastings NC, Hayato Y, Hearty C, Helmer RL, Hierholzer M, Hignight J, Hillairet A, Himmel A, Hiraki T, Hirota S, Holeczek J, Horikawa S, Huang K, Ichikawa AK, Ieki K, Ieva M, Ikeda M, Imber J, Insler J, Irvine TJ, Ishida T, Ishii T, Ives SJ, Iwai E, Iyogi K, Izmaylov A, Jacob A, Jamieson B, Johnson RA, Jo JH, Jonsson P, Jung CK, Kabirnezhad M, Kaboth AC, Kajita T, Kakuno H, Kameda J, Kanazawa Y, Karlen D, Karpikov I, Kearns E, Khabibullin M, Khotjantsev A, Kielczewska D, Kikawa T, Kilinski A, Kim J, Kisiel J, Kitching P, Kobayashi T, Koch L, Kolaceke A, Konaka A, Kormos LL, Korzenev A, Koseki K, Koshio Y, Kreslo I, Kropp W, Kubo H, Kudenko Y, Kumaratunga S, Kurjata R, Kutter T, Lagoda J, Laihem K, Lamont I, Laveder M, Lawe M, Lazos M, Lee KP, Lindner T, Lister C, Litchfield RP, Longhin A, Ludovici L, Macaire M, Magaletti L, Mahn K, Malek M, Manly S, Marino AD, Marteau J, Martin JF, Maruyama T, Marzec J, Mathie EL, Matveev V, Mavrokoridis K, Mazzucato E, McCarthy M, McCauley N, McFarland KS, McGrew C, Metelko C, Mezzetto M, Mijakowski P, Miller CA, Minamino A, Mineev O, Mine S, Missert A, Miura M, Monfregola L, Moriyama S, Mueller TA, Murakami A, Murdoch M, Murphy S, Myslik J, Nagasaki T, Nakadaira T, Nakahata M, Nakai T, Nakamura K, Nakayama S, Nakaya T, Nakayoshi K, Naples D, Nielsen C, Nirkko M, Nishikawa K, Nishimura Y, O'Keeffe HM, Ohta R, Okumura K, Okusawa T, Oryszczak W, Oser SM, Owen RA, Oyama Y, Palladino V, Palomino J, Paolone V, Payne D, Perevozchikov O, Perkin JD, Petrov Y, Pickard L, Pinzon Guerra ES, Pistillo C, Plonski P, Poplawska E, Popov B, Posiadala M, Poutissou JM, Poutissou R, Przewlocki P, Quilain B, Radicioni E, Ratoff PN, Ravonel M, Rayner MAM, Redij A, Reeves M, Reinherz-Aronis E, Retiere F, Robert A, Rodrigues PA, Rojas P, Rondio E, Roth S, Rubbia A, Ruterbories D, Sacco R, Sakashita K, Sánchez F, Sato F, Scantamburlo E, Scholberg K, Schoppmann S, Schwehr J, Scott M, Seiya Y, Sekiguchi T, Sekiya H, Sgalaberna D, Shiozawa M, Short S, Shustrov Y, Sinclair P, Smith B, Smith RJ, Smy M, Sobczyk JT, Sobel H, Sorel M, Southwell L, Stamoulis P, Steinmann J, Still B, Suda Y, Suzuki A, Suzuki K, Suzuki SY, Suzuki Y, Szeglowski T, Tacik R, Tada M, Takahashi S, Takeda A, Takeuchi Y, Tanaka HK, Tanaka HA, Tanaka MM, Terhorst D, Terri R, Thompson LF, Thorley A, Tobayama S, Toki W, Tomura T, Totsuka Y, Touramanis C, Tsukamoto T, Tzanov M, Uchida Y, Ueno K, Vacheret A, Vagins M, Vasseur G, Wachala T, Waldron AV, Walter CW, Wark D, Wascko MO, Weber A, Wendell R, Wilkes RJ, Wilking MJ, Wilkinson C, Williamson Z, Wilson JR, Wilson RJ, Wongjirad T, Yamada Y, Yamamoto K, Yanagisawa C, Yen S, Yershov N, Yokoyama M, Yuan T, Yu M, Zalewska A, Zalipska J, Zambelli L, Zaremba K, Ziembicki M, Zimmerman ED, Zito M, Żmuda J. Precise measurement of the neutrino mixing parameter θ23 from muon neutrino disappearance in an off-axis beam. Phys Rev Lett 2014; 112:181801. [PMID: 24856687 DOI: 10.1103/physrevlett.112.181801] [Citation(s) in RCA: 10] [Impact Index Per Article: 1.0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Received: 03/06/2014] [Indexed: 06/03/2023]
Abstract
New data from the T2K neutrino oscillation experiment produce the most precise measurement of the neutrino mixing parameter θ23. Using an off-axis neutrino beam with a peak energy of 0.6 GeV and a data set corresponding to 6.57×10(20) protons on target, T2K has fit the energy-dependent νμ oscillation probability to determine oscillation parameters. The 68% confidence limit on sin(2)(θ23) is 0.514(-0.056)(+0.055) (0.511±0.055), assuming normal (inverted) mass hierarchy. The best-fit mass-squared splitting for normal hierarchy is Δm32(2)=(2.51±0.10)×10(-3) eV(2)/c(4) (inverted hierarchy: Δm13(2)=(2.48±0.10)×10(-3) eV(2)/c(4)). Adding a model of multinucleon interactions that affect neutrino energy reconstruction is found to produce only small biases in neutrino oscillation parameter extraction at current levels of statistical uncertainty.
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Affiliation(s)
- K Abe
- University of Tokyo, Institute for Cosmic Ray Research, Kamioka Observatory, Kamioka, Japan
| | - J Adam
- State University of New York at Stony Brook, Department of Physics and Astronomy, Stony Brook, New York, USA
| | - H Aihara
- Kavli Institute for the Physics and Mathematics of the Universe (WPI), Todai Institutes for Advanced Study, University of Tokyo, Kashiwa, Chiba, Japan and University of Tokyo, Department of Physics, Tokyo, Japan
| | - T Akiri
- Duke University, Department of Physics, Durham, North Carolina, USA
| | - C Andreopoulos
- STFC, Rutherford Appleton Laboratory, Harwell Oxford, and Daresbury Laboratory, Warrington, United Kingdom
| | - S Aoki
- Kobe University, Kobe, Japan
| | - A Ariga
- University of Bern, Albert Einstein Center for Fundamental Physics, Laboratory for High Energy Physics (LHEP), Bern, Switzerland
| | - T Ariga
- University of Bern, Albert Einstein Center for Fundamental Physics, Laboratory for High Energy Physics (LHEP), Bern, Switzerland
| | - S Assylbekov
- Colorado State University, Department of Physics, Fort Collins, Colorado, USA
| | - D Autiero
- Université de Lyon, Université Claude Bernard Lyon 1, IPN Lyon (IN2P3), Villeurbanne, France
| | - M Barbi
- University of Regina, Department of Physics, Regina, Saskatchewan, Canada
| | - G J Barker
- University of Warwick, Department of Physics, Coventry, United Kingdom
| | - G Barr
- Oxford University, Department of Physics, Oxford, United Kingdom
| | - M Bass
- Colorado State University, Department of Physics, Fort Collins, Colorado, USA
| | - M Batkiewicz
- H. Niewodniczanski Institute of Nuclear Physics PAN, Cracow, Poland
| | - F Bay
- ETH Zurich, Institute for Particle Physics, Zurich, Switzerland
| | - S W Bentham
- Lancaster University, Physics Department, Lancaster, United Kingdom
| | - V Berardi
- INFN Sezione di Bari and Università e Politecnico di Bari, Dipartimento Interuniversitario di Fisica, Bari, Italy
| | - B E Berger
- Colorado State University, Department of Physics, Fort Collins, Colorado, USA
| | - S Berkman
- University of British Columbia, Department of Physics and Astronomy, Vancouver, British Columbia, Canada
| | - I Bertram
- Lancaster University, Physics Department, Lancaster, United Kingdom
| | - S Bhadra
- York University, Department of Physics and Astronomy, Toronto, Ontario, Canada
| | - F d M Blaszczyk
- Louisiana State University, Department of Physics and Astronomy, Baton Rouge, Louisiana, USA
| | - A Blondel
- University of Geneva, Section de Physique, DPNC, Geneva, Switzerland
| | - C Bojechko
- University of Victoria, Department of Physics and Astronomy, Victoria, British Columbia, Canada
| | - S Bordoni
- Institut de Fisica d'Altes Energies (IFAE), Bellaterra (Barcelona), Spain
| | - S B Boyd
- University of Warwick, Department of Physics, Coventry, United Kingdom
| | - D Brailsford
- Imperial College London, Department of Physics, London, United Kingdom
| | - A Bravar
- University of Geneva, Section de Physique, DPNC, Geneva, Switzerland
| | - C Bronner
- Kyoto University, Department of Physics, Kyoto, Japan
| | - N Buchanan
- Colorado State University, Department of Physics, Fort Collins, Colorado, USA
| | - R G Calland
- University of Liverpool, Department of Physics, Liverpool, United Kingdom
| | | | - S L Cartwright
- University of Sheffield, Department of Physics and Astronomy, Sheffield, United Kingdom
| | - R Castillo
- Institut de Fisica d'Altes Energies (IFAE), Bellaterra (Barcelona), Spain
| | - M G Catanesi
- INFN Sezione di Bari and Università e Politecnico di Bari, Dipartimento Interuniversitario di Fisica, Bari, Italy
| | - A Cervera
- IFIC (CSIC and University of Valencia), Valencia, Spain
| | - D Cherdack
- Colorado State University, Department of Physics, Fort Collins, Colorado, USA
| | - G Christodoulou
- University of Liverpool, Department of Physics, Liverpool, United Kingdom
| | - A Clifton
- Colorado State University, Department of Physics, Fort Collins, Colorado, USA
| | - J Coleman
- University of Liverpool, Department of Physics, Liverpool, United Kingdom
| | - S J Coleman
- University of Colorado at Boulder, Department of Physics, Boulder, Colorado, USA
| | - G Collazuol
- INFN Sezione di Padova and Università di Padova, Dipartimento di Fisica, Padova, Italy
| | - K Connolly
- University of Washington, Department of Physics, Seattle, Washington, USA
| | - L Cremonesi
- Queen Mary University of London, School of Physics and Astronomy, London, United Kingdom
| | - A Dabrowska
- H. Niewodniczanski Institute of Nuclear Physics PAN, Cracow, Poland
| | - I Danko
- University of Pittsburgh, Department of Physics and Astronomy, Pittsburgh, Pennsylvania, USA
| | - R Das
- Colorado State University, Department of Physics, Fort Collins, Colorado, USA
| | - S Davis
- University of Washington, Department of Physics, Seattle, Washington, USA
| | - P de Perio
- University of Toronto, Department of Physics, Toronto, Ontario, Canada
| | - G De Rosa
- INFN Sezione di Napoli and Università di Napoli, Dipartimento di Fisica, Napoli, Italy
| | - T Dealtry
- Oxford University, Department of Physics, Oxford, United Kingdom and STFC, Rutherford Appleton Laboratory, Harwell Oxford, and Daresbury Laboratory, Warrington, United Kingdom
| | - S R Dennis
- STFC, Rutherford Appleton Laboratory, Harwell Oxford, and Daresbury Laboratory, Warrington, United Kingdom and University of Warwick, Department of Physics, Coventry, United Kingdom
| | - C Densham
- STFC, Rutherford Appleton Laboratory, Harwell Oxford, and Daresbury Laboratory, Warrington, United Kingdom
| | - F Di Lodovico
- Queen Mary University of London, School of Physics and Astronomy, London, United Kingdom
| | - S Di Luise
- ETH Zurich, Institute for Particle Physics, Zurich, Switzerland
| | - O Drapier
- Ecole Polytechnique, IN2P3-CNRS, Laboratoire Leprince-Ringuet, Palaiseau, France
| | - T Duboyski
- Queen Mary University of London, School of Physics and Astronomy, London, United Kingdom
| | - K Duffy
- Oxford University, Department of Physics, Oxford, United Kingdom
| | - F Dufour
- University of Geneva, Section de Physique, DPNC, Geneva, Switzerland
| | - J Dumarchez
- UPMC, Université Paris Diderot, CNRS/IN2P3, Laboratoire de Physique Nucléaire et de Hautes Energies (LPNHE), Paris, France
| | - S Dytman
- University of Pittsburgh, Department of Physics and Astronomy, Pittsburgh, Pennsylvania, USA
| | - M Dziewiecki
- Warsaw University of Technology, Institute of Radioelectronics, Warsaw, Poland
| | - S Emery
- IRFU, CEA Saclay, Gif-sur-Yvette, France
| | - A Ereditato
- University of Bern, Albert Einstein Center for Fundamental Physics, Laboratory for High Energy Physics (LHEP), Bern, Switzerland
| | - L Escudero
- IFIC (CSIC and University of Valencia), Valencia, Spain
| | - A J Finch
- Lancaster University, Physics Department, Lancaster, United Kingdom
| | - L Floetotto
- RWTH Aachen University, III. Physikalisches Institut, Aachen, Germany
| | - M Friend
- High Energy Accelerator Research Organization (KEK), Tsukuba, Ibaraki, Japan
| | - Y Fujii
- High Energy Accelerator Research Organization (KEK), Tsukuba, Ibaraki, Japan
| | - Y Fukuda
- Miyagi University of Education, Department of Physics, Sendai, Japan
| | - A P Furmanski
- University of Warwick, Department of Physics, Coventry, United Kingdom
| | - V Galymov
- IRFU, CEA Saclay, Gif-sur-Yvette, France
| | - S Giffin
- University of Regina, Department of Physics, Regina, Saskatchewan, Canada
| | - C Giganti
- UPMC, Université Paris Diderot, CNRS/IN2P3, Laboratoire de Physique Nucléaire et de Hautes Energies (LPNHE), Paris, France
| | - K Gilje
- State University of New York at Stony Brook, Department of Physics and Astronomy, Stony Brook, New York, USA
| | - D Goeldi
- University of Bern, Albert Einstein Center for Fundamental Physics, Laboratory for High Energy Physics (LHEP), Bern, Switzerland
| | - T Golan
- Wroclaw University, Faculty of Physics and Astronomy, Wroclaw, Poland
| | - M Gonin
- Ecole Polytechnique, IN2P3-CNRS, Laboratoire Leprince-Ringuet, Palaiseau, France
| | - N Grant
- Lancaster University, Physics Department, Lancaster, United Kingdom
| | - D Gudin
- Institute for Nuclear Research of the Russian Academy of Sciences, Moscow, Russia
| | - D R Hadley
- University of Warwick, Department of Physics, Coventry, United Kingdom
| | - A Haesler
- University of Geneva, Section de Physique, DPNC, Geneva, Switzerland
| | - M D Haigh
- University of Warwick, Department of Physics, Coventry, United Kingdom
| | - P Hamilton
- Imperial College London, Department of Physics, London, United Kingdom
| | - D Hansen
- University of Pittsburgh, Department of Physics and Astronomy, Pittsburgh, Pennsylvania, USA
| | - T Hara
- Kobe University, Kobe, Japan
| | - M Hartz
- Kavli Institute for the Physics and Mathematics of the Universe (WPI), Todai Institutes for Advanced Study, University of Tokyo, Kashiwa, Chiba, Japan and TRIUMF, Vancouver, British Columbia, Canada
| | - T Hasegawa
- High Energy Accelerator Research Organization (KEK), Tsukuba, Ibaraki, Japan
| | - N C Hastings
- University of Regina, Department of Physics, Regina, Saskatchewan, Canada
| | - Y Hayato
- University of Tokyo, Institute for Cosmic Ray Research, Kamioka Observatory, Kamioka, Japan
| | - C Hearty
- University of British Columbia, Department of Physics and Astronomy, Vancouver, British Columbia, Canada
| | - R L Helmer
- TRIUMF, Vancouver, British Columbia, Canada
| | - M Hierholzer
- University of Bern, Albert Einstein Center for Fundamental Physics, Laboratory for High Energy Physics (LHEP), Bern, Switzerland
| | - J Hignight
- State University of New York at Stony Brook, Department of Physics and Astronomy, Stony Brook, New York, USA
| | - A Hillairet
- University of Victoria, Department of Physics and Astronomy, Victoria, British Columbia, Canada
| | - A Himmel
- Duke University, Department of Physics, Durham, North Carolina, USA
| | - T Hiraki
- Kyoto University, Department of Physics, Kyoto, Japan
| | - S Hirota
- Kyoto University, Department of Physics, Kyoto, Japan
| | - J Holeczek
- University of Silesia, Institute of Physics, Katowice, Poland
| | - S Horikawa
- ETH Zurich, Institute for Particle Physics, Zurich, Switzerland
| | - K Huang
- Kyoto University, Department of Physics, Kyoto, Japan
| | - A K Ichikawa
- Kyoto University, Department of Physics, Kyoto, Japan
| | - K Ieki
- Kyoto University, Department of Physics, Kyoto, Japan
| | - M Ieva
- Institut de Fisica d'Altes Energies (IFAE), Bellaterra (Barcelona), Spain
| | - M Ikeda
- University of Tokyo, Institute for Cosmic Ray Research, Kamioka Observatory, Kamioka, Japan
| | - J Imber
- State University of New York at Stony Brook, Department of Physics and Astronomy, Stony Brook, New York, USA
| | - J Insler
- Louisiana State University, Department of Physics and Astronomy, Baton Rouge, Louisiana, USA
| | - T J Irvine
- University of Tokyo, Institute for Cosmic Ray Research, Research Center for Cosmic Neutrinos, Kashiwa, Japan
| | - T Ishida
- High Energy Accelerator Research Organization (KEK), Tsukuba, Ibaraki, Japan
| | - T Ishii
- High Energy Accelerator Research Organization (KEK), Tsukuba, Ibaraki, Japan
| | - S J Ives
- Imperial College London, Department of Physics, London, United Kingdom
| | - E Iwai
- High Energy Accelerator Research Organization (KEK), Tsukuba, Ibaraki, Japan
| | - K Iyogi
- University of Tokyo, Institute for Cosmic Ray Research, Kamioka Observatory, Kamioka, Japan
| | - A Izmaylov
- IFIC (CSIC and University of Valencia), Valencia, Spain and Institute for Nuclear Research of the Russian Academy of Sciences, Moscow, Russia
| | - A Jacob
- Oxford University, Department of Physics, Oxford, United Kingdom
| | - B Jamieson
- University of Winnipeg, Department of Physics, Winnipeg, Manitoba, Canada
| | - R A Johnson
- University of Colorado at Boulder, Department of Physics, Boulder, Colorado, USA
| | - J H Jo
- State University of New York at Stony Brook, Department of Physics and Astronomy, Stony Brook, New York, USA
| | - P Jonsson
- Imperial College London, Department of Physics, London, United Kingdom
| | - C K Jung
- State University of New York at Stony Brook, Department of Physics and Astronomy, Stony Brook, New York, USA
| | - M Kabirnezhad
- National Centre for Nuclear Research, Warsaw, Poland
| | - A C Kaboth
- Imperial College London, Department of Physics, London, United Kingdom
| | - T Kajita
- University of Tokyo, Institute for Cosmic Ray Research, Research Center for Cosmic Neutrinos, Kashiwa, Japan
| | - H Kakuno
- Tokyo Metropolitan University, Department of Physics, Tokyo, Japan
| | - J Kameda
- University of Tokyo, Institute for Cosmic Ray Research, Kamioka Observatory, Kamioka, Japan
| | - Y Kanazawa
- University of Tokyo, Department of Physics, Tokyo, Japan
| | - D Karlen
- TRIUMF, Vancouver, British Columbia, Canada and University of Victoria, Department of Physics and Astronomy, Victoria, British Columbia, Canada
| | - I Karpikov
- Institute for Nuclear Research of the Russian Academy of Sciences, Moscow, Russia
| | - E Kearns
- Boston University, Department of Physics, Boston, Massachusetts, USA and Kavli Institute for the Physics and Mathematics of the Universe (WPI), Todai Institutes for Advanced Study, University of Tokyo, Kashiwa, Chiba, Japan
| | - M Khabibullin
- Institute for Nuclear Research of the Russian Academy of Sciences, Moscow, Russia
| | - A Khotjantsev
- Institute for Nuclear Research of the Russian Academy of Sciences, Moscow, Russia
| | - D Kielczewska
- University of Warsaw, Faculty of Physics, Warsaw, Poland
| | - T Kikawa
- Kyoto University, Department of Physics, Kyoto, Japan
| | - A Kilinski
- National Centre for Nuclear Research, Warsaw, Poland
| | - J Kim
- University of British Columbia, Department of Physics and Astronomy, Vancouver, British Columbia, Canada
| | - J Kisiel
- University of Silesia, Institute of Physics, Katowice, Poland
| | - P Kitching
- University of Alberta, Centre for Particle Physics, Department of Physics, Edmonton, Alberta, Canada
| | - T Kobayashi
- High Energy Accelerator Research Organization (KEK), Tsukuba, Ibaraki, Japan
| | - L Koch
- RWTH Aachen University, III. Physikalisches Institut, Aachen, Germany
| | - A Kolaceke
- University of Regina, Department of Physics, Regina, Saskatchewan, Canada
| | - A Konaka
- TRIUMF, Vancouver, British Columbia, Canada
| | - L L Kormos
- Lancaster University, Physics Department, Lancaster, United Kingdom
| | - A Korzenev
- University of Geneva, Section de Physique, DPNC, Geneva, Switzerland
| | - K Koseki
- High Energy Accelerator Research Organization (KEK), Tsukuba, Ibaraki, Japan
| | - Y Koshio
- Okayama University, Department of Physics, Okayama, Japan
| | - I Kreslo
- University of Bern, Albert Einstein Center for Fundamental Physics, Laboratory for High Energy Physics (LHEP), Bern, Switzerland
| | - W Kropp
- University of California, Irvine, Department of Physics and Astronomy, Irvine, California, USA
| | - H Kubo
- Kyoto University, Department of Physics, Kyoto, Japan
| | - Y Kudenko
- Institute for Nuclear Research of the Russian Academy of Sciences, Moscow, Russia
| | | | - R Kurjata
- Warsaw University of Technology, Institute of Radioelectronics, Warsaw, Poland
| | - T Kutter
- Louisiana State University, Department of Physics and Astronomy, Baton Rouge, Louisiana, USA
| | - J Lagoda
- National Centre for Nuclear Research, Warsaw, Poland
| | - K Laihem
- RWTH Aachen University, III. Physikalisches Institut, Aachen, Germany
| | - I Lamont
- Lancaster University, Physics Department, Lancaster, United Kingdom
| | - M Laveder
- INFN Sezione di Padova and Università di Padova, Dipartimento di Fisica, Padova, Italy
| | - M Lawe
- University of Sheffield, Department of Physics and Astronomy, Sheffield, United Kingdom
| | - M Lazos
- University of Liverpool, Department of Physics, Liverpool, United Kingdom
| | - K P Lee
- University of Tokyo, Institute for Cosmic Ray Research, Research Center for Cosmic Neutrinos, Kashiwa, Japan
| | - T Lindner
- TRIUMF, Vancouver, British Columbia, Canada
| | - C Lister
- University of Warwick, Department of Physics, Coventry, United Kingdom
| | - R P Litchfield
- University of Warwick, Department of Physics, Coventry, United Kingdom
| | - A Longhin
- INFN Sezione di Padova and Università di Padova, Dipartimento di Fisica, Padova, Italy
| | - L Ludovici
- INFN Sezione di Roma and Università di Roma "La Sapienza," Roma, Italy
| | - M Macaire
- IRFU, CEA Saclay, Gif-sur-Yvette, France
| | - L Magaletti
- INFN Sezione di Bari and Università e Politecnico di Bari, Dipartimento Interuniversitario di Fisica, Bari, Italy
| | - K Mahn
- TRIUMF, Vancouver, British Columbia, Canada
| | - M Malek
- Imperial College London, Department of Physics, London, United Kingdom
| | - S Manly
- University of Rochester, Department of Physics and Astronomy, Rochester, New York, USA
| | - A D Marino
- University of Colorado at Boulder, Department of Physics, Boulder, Colorado, USA
| | - J Marteau
- Université de Lyon, Université Claude Bernard Lyon 1, IPN Lyon (IN2P3), Villeurbanne, France
| | - J F Martin
- University of Toronto, Department of Physics, Toronto, Ontario, Canada
| | - T Maruyama
- High Energy Accelerator Research Organization (KEK), Tsukuba, Ibaraki, Japan
| | - J Marzec
- Warsaw University of Technology, Institute of Radioelectronics, Warsaw, Poland
| | - E L Mathie
- University of Regina, Department of Physics, Regina, Saskatchewan, Canada
| | - V Matveev
- Institute for Nuclear Research of the Russian Academy of Sciences, Moscow, Russia
| | - K Mavrokoridis
- University of Liverpool, Department of Physics, Liverpool, United Kingdom
| | | | - M McCarthy
- University of British Columbia, Department of Physics and Astronomy, Vancouver, British Columbia, Canada
| | - N McCauley
- University of Liverpool, Department of Physics, Liverpool, United Kingdom
| | - K S McFarland
- University of Rochester, Department of Physics and Astronomy, Rochester, New York, USA
| | - C McGrew
- State University of New York at Stony Brook, Department of Physics and Astronomy, Stony Brook, New York, USA
| | - C Metelko
- University of Liverpool, Department of Physics, Liverpool, United Kingdom
| | - M Mezzetto
- INFN Sezione di Padova and Università di Padova, Dipartimento di Fisica, Padova, Italy
| | - P Mijakowski
- National Centre for Nuclear Research, Warsaw, Poland
| | - C A Miller
- TRIUMF, Vancouver, British Columbia, Canada
| | - A Minamino
- Kyoto University, Department of Physics, Kyoto, Japan
| | - O Mineev
- Institute for Nuclear Research of the Russian Academy of Sciences, Moscow, Russia
| | - S Mine
- University of California, Irvine, Department of Physics and Astronomy, Irvine, California, USA
| | - A Missert
- University of Colorado at Boulder, Department of Physics, Boulder, Colorado, USA
| | - M Miura
- University of Tokyo, Institute for Cosmic Ray Research, Kamioka Observatory, Kamioka, Japan
| | - L Monfregola
- IFIC (CSIC and University of Valencia), Valencia, Spain
| | - S Moriyama
- University of Tokyo, Institute for Cosmic Ray Research, Kamioka Observatory, Kamioka, Japan
| | - Th A Mueller
- Ecole Polytechnique, IN2P3-CNRS, Laboratoire Leprince-Ringuet, Palaiseau, France
| | - A Murakami
- Kyoto University, Department of Physics, Kyoto, Japan
| | - M Murdoch
- University of Liverpool, Department of Physics, Liverpool, United Kingdom
| | - S Murphy
- ETH Zurich, Institute for Particle Physics, Zurich, Switzerland
| | - J Myslik
- University of Victoria, Department of Physics and Astronomy, Victoria, British Columbia, Canada
| | - T Nagasaki
- Kyoto University, Department of Physics, Kyoto, Japan
| | - T Nakadaira
- High Energy Accelerator Research Organization (KEK), Tsukuba, Ibaraki, Japan
| | - M Nakahata
- Kavli Institute for the Physics and Mathematics of the Universe (WPI), Todai Institutes for Advanced Study, University of Tokyo, Kashiwa, Chiba, Japan and University of Tokyo, Institute for Cosmic Ray Research, Kamioka Observatory, Kamioka, Japan
| | - T Nakai
- Osaka City University, Department of Physics, Osaka, Japan
| | - K Nakamura
- High Energy Accelerator Research Organization (KEK), Tsukuba, Ibaraki, Japan and Kavli Institute for the Physics and Mathematics of the Universe (WPI), Todai Institutes for Advanced Study, University of Tokyo, Kashiwa, Chiba, Japan
| | - S Nakayama
- University of Tokyo, Institute for Cosmic Ray Research, Kamioka Observatory, Kamioka, Japan
| | - T Nakaya
- Kavli Institute for the Physics and Mathematics of the Universe (WPI), Todai Institutes for Advanced Study, University of Tokyo, Kashiwa, Chiba, Japan and Kyoto University, Department of Physics, Kyoto, Japan
| | - K Nakayoshi
- High Energy Accelerator Research Organization (KEK), Tsukuba, Ibaraki, Japan
| | - D Naples
- University of Pittsburgh, Department of Physics and Astronomy, Pittsburgh, Pennsylvania, USA
| | - C Nielsen
- University of British Columbia, Department of Physics and Astronomy, Vancouver, British Columbia, Canada
| | - M Nirkko
- University of Bern, Albert Einstein Center for Fundamental Physics, Laboratory for High Energy Physics (LHEP), Bern, Switzerland
| | - K Nishikawa
- High Energy Accelerator Research Organization (KEK), Tsukuba, Ibaraki, Japan
| | - Y Nishimura
- University of Tokyo, Institute for Cosmic Ray Research, Research Center for Cosmic Neutrinos, Kashiwa, Japan
| | - H M O'Keeffe
- Lancaster University, Physics Department, Lancaster, United Kingdom
| | - R Ohta
- High Energy Accelerator Research Organization (KEK), Tsukuba, Ibaraki, Japan
| | - K Okumura
- Kavli Institute for the Physics and Mathematics of the Universe (WPI), Todai Institutes for Advanced Study, University of Tokyo, Kashiwa, Chiba, Japan and University of Tokyo, Institute for Cosmic Ray Research, Research Center for Cosmic Neutrinos, Kashiwa, Japan
| | - T Okusawa
- Osaka City University, Department of Physics, Osaka, Japan
| | - W Oryszczak
- University of Warsaw, Faculty of Physics, Warsaw, Poland
| | - S M Oser
- University of British Columbia, Department of Physics and Astronomy, Vancouver, British Columbia, Canada
| | - R A Owen
- Queen Mary University of London, School of Physics and Astronomy, London, United Kingdom
| | - Y Oyama
- High Energy Accelerator Research Organization (KEK), Tsukuba, Ibaraki, Japan
| | - V Palladino
- INFN Sezione di Napoli and Università di Napoli, Dipartimento di Fisica, Napoli, Italy
| | - J Palomino
- State University of New York at Stony Brook, Department of Physics and Astronomy, Stony Brook, New York, USA
| | - V Paolone
- University of Pittsburgh, Department of Physics and Astronomy, Pittsburgh, Pennsylvania, USA
| | - D Payne
- University of Liverpool, Department of Physics, Liverpool, United Kingdom
| | - O Perevozchikov
- Louisiana State University, Department of Physics and Astronomy, Baton Rouge, Louisiana, USA
| | - J D Perkin
- University of Sheffield, Department of Physics and Astronomy, Sheffield, United Kingdom
| | - Y Petrov
- University of British Columbia, Department of Physics and Astronomy, Vancouver, British Columbia, Canada
| | - L Pickard
- University of Sheffield, Department of Physics and Astronomy, Sheffield, United Kingdom
| | - E S Pinzon Guerra
- York University, Department of Physics and Astronomy, Toronto, Ontario, Canada
| | - C Pistillo
- University of Bern, Albert Einstein Center for Fundamental Physics, Laboratory for High Energy Physics (LHEP), Bern, Switzerland
| | - P Plonski
- Warsaw University of Technology, Institute of Radioelectronics, Warsaw, Poland
| | - E Poplawska
- Queen Mary University of London, School of Physics and Astronomy, London, United Kingdom
| | - B Popov
- UPMC, Université Paris Diderot, CNRS/IN2P3, Laboratoire de Physique Nucléaire et de Hautes Energies (LPNHE), Paris, France
| | - M Posiadala
- University of Warsaw, Faculty of Physics, Warsaw, Poland
| | | | | | - P Przewlocki
- National Centre for Nuclear Research, Warsaw, Poland
| | - B Quilain
- Ecole Polytechnique, IN2P3-CNRS, Laboratoire Leprince-Ringuet, Palaiseau, France
| | - E Radicioni
- INFN Sezione di Bari and Università e Politecnico di Bari, Dipartimento Interuniversitario di Fisica, Bari, Italy
| | - P N Ratoff
- Lancaster University, Physics Department, Lancaster, United Kingdom
| | - M Ravonel
- University of Geneva, Section de Physique, DPNC, Geneva, Switzerland
| | - M A M Rayner
- University of Geneva, Section de Physique, DPNC, Geneva, Switzerland
| | - A Redij
- University of Bern, Albert Einstein Center for Fundamental Physics, Laboratory for High Energy Physics (LHEP), Bern, Switzerland
| | - M Reeves
- Lancaster University, Physics Department, Lancaster, United Kingdom
| | - E Reinherz-Aronis
- Colorado State University, Department of Physics, Fort Collins, Colorado, USA
| | - F Retiere
- TRIUMF, Vancouver, British Columbia, Canada
| | - A Robert
- UPMC, Université Paris Diderot, CNRS/IN2P3, Laboratoire de Physique Nucléaire et de Hautes Energies (LPNHE), Paris, France
| | - P A Rodrigues
- University of Rochester, Department of Physics and Astronomy, Rochester, New York, USA
| | - P Rojas
- Colorado State University, Department of Physics, Fort Collins, Colorado, USA
| | - E Rondio
- National Centre for Nuclear Research, Warsaw, Poland
| | - S Roth
- RWTH Aachen University, III. Physikalisches Institut, Aachen, Germany
| | - A Rubbia
- ETH Zurich, Institute for Particle Physics, Zurich, Switzerland
| | - D Ruterbories
- Colorado State University, Department of Physics, Fort Collins, Colorado, USA
| | - R Sacco
- Queen Mary University of London, School of Physics and Astronomy, London, United Kingdom
| | - K Sakashita
- High Energy Accelerator Research Organization (KEK), Tsukuba, Ibaraki, Japan
| | - F Sánchez
- Institut de Fisica d'Altes Energies (IFAE), Bellaterra (Barcelona), Spain
| | - F Sato
- High Energy Accelerator Research Organization (KEK), Tsukuba, Ibaraki, Japan
| | - E Scantamburlo
- University of Geneva, Section de Physique, DPNC, Geneva, Switzerland
| | - K Scholberg
- Duke University, Department of Physics, Durham, North Carolina, USA
| | - S Schoppmann
- RWTH Aachen University, III. Physikalisches Institut, Aachen, Germany
| | - J Schwehr
- Colorado State University, Department of Physics, Fort Collins, Colorado, USA
| | - M Scott
- TRIUMF, Vancouver, British Columbia, Canada
| | - Y Seiya
- Osaka City University, Department of Physics, Osaka, Japan
| | - T Sekiguchi
- High Energy Accelerator Research Organization (KEK), Tsukuba, Ibaraki, Japan
| | - H Sekiya
- University of Tokyo, Institute for Cosmic Ray Research, Kamioka Observatory, Kamioka, Japan
| | - D Sgalaberna
- ETH Zurich, Institute for Particle Physics, Zurich, Switzerland
| | - M Shiozawa
- Kavli Institute for the Physics and Mathematics of the Universe (WPI), Todai Institutes for Advanced Study, University of Tokyo, Kashiwa, Chiba, Japan and University of Tokyo, Institute for Cosmic Ray Research, Kamioka Observatory, Kamioka, Japan
| | - S Short
- Imperial College London, Department of Physics, London, United Kingdom
| | - Y Shustrov
- Institute for Nuclear Research of the Russian Academy of Sciences, Moscow, Russia
| | - P Sinclair
- Imperial College London, Department of Physics, London, United Kingdom
| | - B Smith
- Imperial College London, Department of Physics, London, United Kingdom
| | - R J Smith
- Oxford University, Department of Physics, Oxford, United Kingdom
| | - M Smy
- University of California, Irvine, Department of Physics and Astronomy, Irvine, California, USA
| | - J T Sobczyk
- Wroclaw University, Faculty of Physics and Astronomy, Wroclaw, Poland
| | - H Sobel
- University of California, Irvine, Department of Physics and Astronomy, Irvine, California, USA and Kavli Institute for the Physics and Mathematics of the Universe (WPI), Todai Institutes for Advanced Study, University of Tokyo, Kashiwa, Chiba, Japan
| | - M Sorel
- IFIC (CSIC and University of Valencia), Valencia, Spain
| | - L Southwell
- Lancaster University, Physics Department, Lancaster, United Kingdom
| | - P Stamoulis
- IFIC (CSIC and University of Valencia), Valencia, Spain
| | - J Steinmann
- RWTH Aachen University, III. Physikalisches Institut, Aachen, Germany
| | - B Still
- Queen Mary University of London, School of Physics and Astronomy, London, United Kingdom
| | - Y Suda
- University of Tokyo, Department of Physics, Tokyo, Japan
| | | | - K Suzuki
- Kyoto University, Department of Physics, Kyoto, Japan
| | - S Y Suzuki
- High Energy Accelerator Research Organization (KEK), Tsukuba, Ibaraki, Japan
| | - Y Suzuki
- Kavli Institute for the Physics and Mathematics of the Universe (WPI), Todai Institutes for Advanced Study, University of Tokyo, Kashiwa, Chiba, Japan and University of Tokyo, Institute for Cosmic Ray Research, Kamioka Observatory, Kamioka, Japan
| | - T Szeglowski
- University of Silesia, Institute of Physics, Katowice, Poland
| | - R Tacik
- University of Regina, Department of Physics, Regina, Saskatchewan, Canada and TRIUMF, Vancouver, British Columbia, Canada
| | - M Tada
- High Energy Accelerator Research Organization (KEK), Tsukuba, Ibaraki, Japan
| | - S Takahashi
- Kyoto University, Department of Physics, Kyoto, Japan
| | - A Takeda
- University of Tokyo, Institute for Cosmic Ray Research, Kamioka Observatory, Kamioka, Japan
| | - Y Takeuchi
- Kavli Institute for the Physics and Mathematics of the Universe (WPI), Todai Institutes for Advanced Study, University of Tokyo, Kashiwa, Chiba, Japan and Kobe University, Kobe, Japan
| | - H K Tanaka
- University of Tokyo, Institute for Cosmic Ray Research, Kamioka Observatory, Kamioka, Japan
| | - H A Tanaka
- University of British Columbia, Department of Physics and Astronomy, Vancouver, British Columbia, Canada
| | - M M Tanaka
- High Energy Accelerator Research Organization (KEK), Tsukuba, Ibaraki, Japan
| | - D Terhorst
- RWTH Aachen University, III. Physikalisches Institut, Aachen, Germany
| | - R Terri
- Queen Mary University of London, School of Physics and Astronomy, London, United Kingdom
| | - L F Thompson
- University of Sheffield, Department of Physics and Astronomy, Sheffield, United Kingdom
| | - A Thorley
- University of Liverpool, Department of Physics, Liverpool, United Kingdom
| | - S Tobayama
- University of British Columbia, Department of Physics and Astronomy, Vancouver, British Columbia, Canada
| | - W Toki
- Colorado State University, Department of Physics, Fort Collins, Colorado, USA
| | - T Tomura
- University of Tokyo, Institute for Cosmic Ray Research, Kamioka Observatory, Kamioka, Japan
| | - Y Totsuka
- University of Alberta, Centre for Particle Physics, Department of Physics, Edmonton, Alberta, Canada and University of Bern, Albert Einstein Center for Fundamental Physics, Laboratory for High Energy Physics (LHEP), Bern, Switzerland and Boston University, Department of Physics, Boston, Massachusetts, USA and University of British Columbia, Department of Physics and Astronomy, Vancouver, British Columbia, Canada and University of California, Irvine, Department of Physics and Astronomy, Irvine, California, USA and IRFU, CEA Saclay, Gif-sur-Yvette, France and University of Colorado at Boulder, Department of Physics, Boulder, Colorado, USA and Colorado State University, Department of Physics, Fort Collins, Colorado, USA and Duke University, Department of Physics, Durham, North Carolina, USA and Ecole Polytechnique, IN2P3-CNRS, Laboratoire Leprince-Ringuet, Palaiseau, France and ETH Zurich, Institute for Particle Physics, Zurich, Switzerland and University of Geneva, Section de Physique, DPNC, Geneva, Switzerland and H. Niewodniczanski Institute of Nuclear Physics PAN, Cracow, Poland and High Energy Accelerator Research Organization (KEK), Tsukuba, Ibaraki, Japan and Institut de Fisica d'Altes Energies (IFAE), Bellaterra (Barcelona), Spain and IFIC (CSIC and University of Valencia), Valencia, Spain and Imperial College London, Department of Physics, London, United Kingdom and INFN Sezione di Bari and Università e Politecnico di Bari, Dipartimento Interuniversitario di Fisica, Bari, Italy and INFN Sezione di Napoli and Università di Napoli, Dipartimento di Fisica, Napoli, Italy and INFN Sezione di Padova and Università di Padova, Dipartimento di Fisica, Padova, Italy and INFN Sezione di Roma and Università di Roma "La Sapienza," Roma, Italy and Institute for Nuclear Research of the Russian Academy of Sciences, Moscow, Russia and Kavli Institute for the Physics and Mathematics of the Universe (WPI), Todai Institutes for Advanced Study, University of Tokyo, Kashiwa, Ch
| | - C Touramanis
- University of Liverpool, Department of Physics, Liverpool, United Kingdom
| | - T Tsukamoto
- High Energy Accelerator Research Organization (KEK), Tsukuba, Ibaraki, Japan
| | - M Tzanov
- Louisiana State University, Department of Physics and Astronomy, Baton Rouge, Louisiana, USA
| | - Y Uchida
- Imperial College London, Department of Physics, London, United Kingdom
| | - K Ueno
- University of Tokyo, Institute for Cosmic Ray Research, Kamioka Observatory, Kamioka, Japan
| | - A Vacheret
- Oxford University, Department of Physics, Oxford, United Kingdom
| | - M Vagins
- University of California, Irvine, Department of Physics and Astronomy, Irvine, California, USA and Kavli Institute for the Physics and Mathematics of the Universe (WPI), Todai Institutes for Advanced Study, University of Tokyo, Kashiwa, Chiba, Japan
| | - G Vasseur
- IRFU, CEA Saclay, Gif-sur-Yvette, France
| | - T Wachala
- H. Niewodniczanski Institute of Nuclear Physics PAN, Cracow, Poland
| | - A V Waldron
- Oxford University, Department of Physics, Oxford, United Kingdom
| | - C W Walter
- Duke University, Department of Physics, Durham, North Carolina, USA
| | - D Wark
- Imperial College London, Department of Physics, London, United Kingdom and STFC, Rutherford Appleton Laboratory, Harwell Oxford, and Daresbury Laboratory, Warrington, United Kingdom
| | - M O Wascko
- Imperial College London, Department of Physics, London, United Kingdom
| | - A Weber
- Oxford University, Department of Physics, Oxford, United Kingdom and STFC, Rutherford Appleton Laboratory, Harwell Oxford, and Daresbury Laboratory, Warrington, United Kingdom
| | - R Wendell
- University of Tokyo, Institute for Cosmic Ray Research, Kamioka Observatory, Kamioka, Japan
| | - R J Wilkes
- University of Washington, Department of Physics, Seattle, Washington, USA
| | | | - C Wilkinson
- University of Sheffield, Department of Physics and Astronomy, Sheffield, United Kingdom
| | - Z Williamson
- Oxford University, Department of Physics, Oxford, United Kingdom
| | - J R Wilson
- Queen Mary University of London, School of Physics and Astronomy, London, United Kingdom
| | - R J Wilson
- Colorado State University, Department of Physics, Fort Collins, Colorado, USA
| | - T Wongjirad
- Duke University, Department of Physics, Durham, North Carolina, USA
| | - Y Yamada
- High Energy Accelerator Research Organization (KEK), Tsukuba, Ibaraki, Japan
| | - K Yamamoto
- Osaka City University, Department of Physics, Osaka, Japan
| | - C Yanagisawa
- State University of New York at Stony Brook, Department of Physics and Astronomy, Stony Brook, New York, USA
| | - S Yen
- TRIUMF, Vancouver, British Columbia, Canada
| | - N Yershov
- Institute for Nuclear Research of the Russian Academy of Sciences, Moscow, Russia
| | - M Yokoyama
- University of Tokyo, Department of Physics, Tokyo, Japan
| | - T Yuan
- University of Colorado at Boulder, Department of Physics, Boulder, Colorado, USA
| | - M Yu
- York University, Department of Physics and Astronomy, Toronto, Ontario, Canada
| | - A Zalewska
- H. Niewodniczanski Institute of Nuclear Physics PAN, Cracow, Poland
| | - J Zalipska
- National Centre for Nuclear Research, Warsaw, Poland
| | - L Zambelli
- UPMC, Université Paris Diderot, CNRS/IN2P3, Laboratoire de Physique Nucléaire et de Hautes Energies (LPNHE), Paris, France
| | - K Zaremba
- Warsaw University of Technology, Institute of Radioelectronics, Warsaw, Poland
| | - M Ziembicki
- Warsaw University of Technology, Institute of Radioelectronics, Warsaw, Poland
| | - E D Zimmerman
- University of Colorado at Boulder, Department of Physics, Boulder, Colorado, USA
| | - M Zito
- IRFU, CEA Saclay, Gif-sur-Yvette, France
| | - J Żmuda
- Wroclaw University, Faculty of Physics and Astronomy, Wroclaw, Poland
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Crabb MG, Davidson JL, Little R, Wright P, Morgan AR, Miller CA, Naish JH, Parker GJM, Kikinis R, McCann H, Lionheart WRB. Mutual information as a measure of image quality for 3D dynamic lung imaging with EIT. Physiol Meas 2014; 35:863-79. [PMID: 24710978 PMCID: PMC4059506 DOI: 10.1088/0967-3334/35/5/863] [Citation(s) in RCA: 12] [Impact Index Per Article: 1.2] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Key Words] [MESH Headings] [Grants] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/12/2022]
Abstract
We report on a pilot study of dynamic lung electrical impedance tomography (EIT) at the University of Manchester. Low-noise EIT data at 100 frames per second were obtained from healthy male subjects during controlled breathing, followed by magnetic resonance imaging (MRI) subsequently used for spatial validation of the EIT reconstruction. The torso surface in the MR image and electrode positions obtained using MRI fiducial markers informed the construction of a 3D finite element model extruded along the caudal-distal axis of the subject. Small changes in the boundary that occur during respiration were accounted for by incorporating the sensitivity with respect to boundary shape into a robust temporal difference reconstruction algorithm. EIT and MRI images were co-registered using the open source medical imaging software, 3D Slicer. A quantitative comparison of quality of different EIT reconstructions was achieved through calculation of the mutual information with a lung-segmented MR image. EIT reconstructions using a linear shape correction algorithm reduced boundary image artefacts, yielding better contrast of the lungs, and had 10% greater mutual information compared with a standard linear EIT reconstruction.
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Affiliation(s)
- M G Crabb
- School of Mathematics, University of Manchester, UK
| | - J L Davidson
- School of Electrical and Electronic Engineering, University of Manchester, UK
| | - R Little
- Centre for Imaging Sciences, Biomedical Imaging Institute, University of Manchester, UK
| | - P Wright
- School of Electrical and Electronic Engineering, University of Manchester, UK
| | - A R Morgan
- Centre for Imaging Sciences, Biomedical Imaging Institute, University of Manchester, UK
| | - C A Miller
- Centre for Imaging Sciences, Biomedical Imaging Institute, University of Manchester, UK
| | - J H Naish
- Centre for Imaging Sciences, Biomedical Imaging Institute, University of Manchester, UK
| | - G J M Parker
- Centre for Imaging Sciences, Biomedical Imaging Institute, University of Manchester, UK
| | - R Kikinis
- Surgical Planning Laboratory, Brigham and Women’s Hospital, Harvard Medical School, Boston, USA
| | - H McCann
- School of Electrical and Electronic Engineering, University of Manchester, UK
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Affiliation(s)
- Hadi ShamsiJazeyi
- Chemical and Biomolecular Engineering Department; Rice University; 6100 Main Street, Houston Texas 77005
| | - Clarence A. Miller
- Chemical and Biomolecular Engineering Department; Rice University; 6100 Main Street, Houston Texas 77005
| | - Michael S. Wong
- Chemical and Biomolecular Engineering Department; Rice University; 6100 Main Street, Houston Texas 77005
| | - James M. Tour
- Department of Chemistry; Rice University; 6100 Main Street, Houston Texas 77005
| | - Rafael Verduzco
- Chemical and Biomolecular Engineering Department; Rice University; 6100 Main Street, Houston Texas 77005
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19
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Abe K, Adam J, Aihara H, Akiri T, Andreopoulos C, Aoki S, Ariga A, Ariga T, Assylbekov S, Autiero D, Barbi M, Barker GJ, Barr G, Bass M, Batkiewicz M, Bay F, Bentham SW, Berardi V, Berger BE, Berkman S, Bertram I, Bhadra S, Blaszczyk FDM, Blondel A, Bojechko C, Bordoni S, Boyd SB, Brailsford D, Bravar A, Bronner C, Buchanan N, Calland RG, Caravaca Rodríguez J, Cartwright SL, Castillo R, Catanesi MG, Cervera A, Cherdack D, Christodoulou G, Clifton A, Coleman J, Coleman SJ, Collazuol G, Connolly K, Cremonesi L, Dabrowska A, Danko I, Das R, Davis S, de Perio P, De Rosa G, Dealtry T, Dennis SR, Densham C, Di Lodovico F, Di Luise S, Drapier O, Duboyski T, Duffy K, Dufour F, Dumarchez J, Dytman S, Dziewiecki M, Emery S, Ereditato A, Escudero L, Finch AJ, Floetotto L, Friend M, Fujii Y, Fukuda Y, Furmanski AP, Galymov V, Gaudin A, Giffin S, Giganti C, Gilje K, Goeldi D, Golan T, Gomez-Cadenas JJ, Gonin M, Grant N, Gudin D, Hadley DR, Haesler A, Haigh MD, Hamilton P, Hansen D, Hara T, Hartz M, Hasegawa T, Hastings NC, Hayato Y, Hearty C, Helmer RL, Hierholzer M, Hignight J, Hillairet A, Himmel A, Hiraki T, Hirota S, Holeczek J, Horikawa S, Huang K, Ichikawa AK, Ieki K, Ieva M, Ikeda M, Imber J, Insler J, Irvine TJ, Ishida T, Ishii T, Ives SJ, Iyogi K, Izmaylov A, Jacob A, Jamieson B, Johnson RA, Jo JH, Jonsson P, Jung CK, Kaboth AC, Kajita T, Kakuno H, Kameda J, Kanazawa Y, Karlen D, Karpikov I, Kearns E, Khabibullin M, Khotjantsev A, Kielczewska D, Kikawa T, Kilinski A, Kim J, Kisiel J, Kitching P, Kobayashi T, Koch L, Kolaceke A, Konaka A, Kormos LL, Korzenev A, Koseki K, Koshio Y, Kreslo I, Kropp W, Kubo H, Kudenko Y, Kumaratunga S, Kurjata R, Kutter T, Lagoda J, Laihem K, Lamont I, Laveder M, Lawe M, Lazos M, Lee KP, Licciardi C, Lindner T, Lister C, Litchfield RP, Longhin A, Ludovici L, Macaire M, Magaletti L, Mahn K, Malek M, Manly S, Marino AD, Marteau J, Martin JF, Maruyama T, Marzec J, Mathie EL, Matveev V, Mavrokoridis K, Mazzucato E, McCarthy M, McCauley N, McFarland KS, McGrew C, Metelko C, Mezzetto M, Mijakowski P, Miller CA, Minamino A, Mineev O, Mine S, Missert A, Miura M, Monfregola L, Moriyama S, Mueller TA, Murakami A, Murdoch M, Murphy S, Myslik J, Nagasaki T, Nakadaira T, Nakahata M, Nakai T, Nakamura K, Nakayama S, Nakaya T, Nakayoshi K, Naples D, Nielsen C, Nirkko M, Nishikawa K, Nishimura Y, O'Keeffe HM, Ohta R, Okumura K, Okusawa T, Oryszczak W, Oser SM, Owen RA, Oyama Y, Palladino V, Paolone V, Payne D, Pearce GF, Perevozchikov O, Perkin JD, Petrov Y, Pickard LJ, Pinzon Guerra ES, Pistillo C, Plonski P, Poplawska E, Popov B, Posiadala M, Poutissou JM, Poutissou R, Przewlocki P, Quilain B, Radicioni E, Ratoff PN, Ravonel M, Rayner MAM, Redij A, Reeves M, Reinherz-Aronis E, Retiere F, Robert A, Rodrigues PA, Rojas P, Rondio E, Roth S, Rubbia A, Ruterbories D, Sacco R, Sakashita K, Sánchez F, Sato F, Scantamburlo E, Scholberg K, Schwehr J, Scott M, Seiya Y, Sekiguchi T, Sekiya H, Sgalaberna D, Shiozawa M, Short S, Shustrov Y, Sinclair P, Smith B, Smith RJ, Smy M, Sobczyk JT, Sobel H, Sorel M, Southwell L, Stamoulis P, Steinmann J, Still B, Suda Y, Suzuki A, Suzuki K, Suzuki SY, Suzuki Y, Szeglowski T, Tacik R, Tada M, Takahashi S, Takeda A, Takeuchi Y, Tanaka HK, Tanaka HA, Tanaka MM, Terhorst D, Terri R, Thompson LF, Thorley A, Tobayama S, Toki W, Tomura T, Totsuka Y, Touramanis C, Tsukamoto T, Tzanov M, Uchida Y, Ueno K, Vacheret A, Vagins M, Vasseur G, Wachala T, Waldron AV, Walter CW, Wark D, Wascko MO, Weber A, Wendell R, Wilkes RJ, Wilking MJ, Wilkinson C, Williamson Z, Wilson JR, Wilson RJ, Wongjirad T, Yamada Y, Yamamoto K, Yanagisawa C, Yen S, Yershov N, Yokoyama M, Yuan T, Zalewska A, Zalipska J, Zambelli L, Zaremba K, Ziembicki M, Zimmerman ED, Zito M, Zmuda J. Observation of electron neutrino appearance in a muon neutrino beam. Phys Rev Lett 2014; 112:061802. [PMID: 24580687 DOI: 10.1103/physrevlett.112.061802] [Citation(s) in RCA: 29] [Impact Index Per Article: 2.9] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Received: 11/19/2013] [Indexed: 06/03/2023]
Abstract
The T2K experiment has observed electron neutrino appearance in a muon neutrino beam produced 295 km from the Super-Kamiokande detector with a peak energy of 0.6 GeV. A total of 28 electron neutrino events were detected with an energy distribution consistent with an appearance signal, corresponding to a significance of 7.3σ when compared to 4.92±0.55 expected background events. In the Pontecorvo-Maki-Nakagawa-Sakata mixing model, the electron neutrino appearance signal depends on several parameters including three mixing angles θ12, θ23, θ13, a mass difference Δm(32)(2) and a CP violating phase δ(CP). In this neutrino oscillation scenario, assuming |Δm(32)(2)|=2.4×10(-3) eV(2), sin(2)θ(23)=0.5, and Δm322>0 (Δm(32)(2)<0), a best-fit value of sin(2)2θ(13)=0.140(-0.032)(+0.038) (0.170(-0.037)(+0.045)) is obtained at δ(CP)=0. When combining the result with the current best knowledge of oscillation parameters including the world average value of θ(13) from reactor experiments, some values of δ(CP) are disfavored at the 90% C.L.
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Affiliation(s)
- K Abe
- University of Tokyo, Institute for Cosmic Ray Research, Kamioka Observatory, Kamioka, Japan
| | - J Adam
- State University of New York at Stony Brook, Department of Physics and Astronomy, Stony Brook, New York, USA
| | - H Aihara
- Kavli Institute for the Physics and Mathematics of the Universe (WPI), Todai Institutes for Advanced Study, University of Tokyo, Kashiwa, Chiba, Japan and University of Tokyo, Department of Physics, Tokyo, Japan
| | - T Akiri
- Duke University, Department of Physics, Durham, North Carolina, USA
| | - C Andreopoulos
- STFC, Rutherford Appleton Laboratory, Harwell Oxford, and Daresbury Laboratory, Warrington, United Kingdom
| | - S Aoki
- Kobe University, Kobe, Japan
| | - A Ariga
- University of Bern, Albert Einstein Center for Fundamental Physics, Laboratory for High Energy Physics (LHEP), Bern, Switzerland
| | - T Ariga
- University of Bern, Albert Einstein Center for Fundamental Physics, Laboratory for High Energy Physics (LHEP), Bern, Switzerland
| | - S Assylbekov
- Colorado State University, Department of Physics, Fort Collins, Colorado, USA
| | - D Autiero
- Université de Lyon, Université Claude Bernard Lyon 1, IPN Lyon (IN2P3), Villeurbanne, France
| | - M Barbi
- University of Regina, Department of Physics, Regina, Saskatchewan, Canada
| | - G J Barker
- University of Warwick, Department of Physics, Coventry, United Kingdom
| | - G Barr
- Oxford University, Department of Physics, Oxford, United Kingdom
| | - M Bass
- Colorado State University, Department of Physics, Fort Collins, Colorado, USA
| | - M Batkiewicz
- H. Niewodniczanski Institute of Nuclear Physics PAN, Cracow, Poland
| | - F Bay
- ETH Zurich, Institute for Particle Physics, Zurich, Switzerland
| | - S W Bentham
- Lancaster University, Physics Department, Lancaster, United Kingdom
| | - V Berardi
- INFN Sezione di Bari and Università e Politecnico di Bari, Dipartimento Interuniversitario di Fisica, Bari, Italy
| | - B E Berger
- Colorado State University, Department of Physics, Fort Collins, Colorado, USA
| | - S Berkman
- University of British Columbia, Department of Physics and Astronomy, Vancouver, British Columbia, Canada
| | - I Bertram
- Lancaster University, Physics Department, Lancaster, United Kingdom
| | - S Bhadra
- York University, Department of Physics and Astronomy, Toronto, Ontario, Canada
| | - F D M Blaszczyk
- Louisiana State University, Department of Physics and Astronomy, Baton Rouge, Louisiana, USA
| | - A Blondel
- University of Geneva, Section de Physique, DPNC, Geneva, Switzerland
| | - C Bojechko
- University of Victoria, Department of Physics and Astronomy, Victoria, British Columbia, Canada
| | - S Bordoni
- Institut de Fisica d'Altes Energies (IFAE), Bellaterra (Barcelona), Spain
| | - S B Boyd
- University of Warwick, Department of Physics, Coventry, United Kingdom
| | - D Brailsford
- Imperial College London, Department of Physics, London, United Kingdom
| | - A Bravar
- University of Geneva, Section de Physique, DPNC, Geneva, Switzerland
| | - C Bronner
- Kyoto University, Department of Physics, Kyoto, Japan
| | - N Buchanan
- Colorado State University, Department of Physics, Fort Collins, Colorado, USA
| | - R G Calland
- University of Liverpool, Department of Physics, Liverpool, United Kingdom
| | | | - S L Cartwright
- University of Sheffield, Department of Physics and Astronomy, Sheffield, United Kingdom
| | - R Castillo
- Institut de Fisica d'Altes Energies (IFAE), Bellaterra (Barcelona), Spain
| | - M G Catanesi
- INFN Sezione di Bari and Università e Politecnico di Bari, Dipartimento Interuniversitario di Fisica, Bari, Italy
| | - A Cervera
- IFIC (CSIC and University of Valencia), Valencia, Spain
| | - D Cherdack
- Colorado State University, Department of Physics, Fort Collins, Colorado, USA
| | - G Christodoulou
- University of Liverpool, Department of Physics, Liverpool, United Kingdom
| | - A Clifton
- Colorado State University, Department of Physics, Fort Collins, Colorado, USA
| | - J Coleman
- University of Liverpool, Department of Physics, Liverpool, United Kingdom
| | - S J Coleman
- University of Colorado at Boulder, Department of Physics, Boulder, Colorado, USA
| | - G Collazuol
- INFN Sezione di Padova and Università di Padova, Dipartimento di Fisica, Padova, Italy
| | - K Connolly
- University of Washington, Department of Physics, Seattle, Washington, USA
| | - L Cremonesi
- Queen Mary University of London, School of Physics and Astronomy, London, United Kingdom
| | - A Dabrowska
- H. Niewodniczanski Institute of Nuclear Physics PAN, Cracow, Poland
| | - I Danko
- University of Pittsburgh, Department of Physics and Astronomy, Pittsburgh, Pennsylvania, USA
| | - R Das
- Colorado State University, Department of Physics, Fort Collins, Colorado, USA
| | - S Davis
- University of Washington, Department of Physics, Seattle, Washington, USA
| | - P de Perio
- University of Toronto, Department of Physics, Toronto, Ontario, Canada
| | - G De Rosa
- INFN Sezione di Napoli and Università di Napoli, Dipartimento di Fisica, Napoli, Italy
| | - T Dealtry
- Oxford University, Department of Physics, Oxford, United Kingdom and STFC, Rutherford Appleton Laboratory, Harwell Oxford, and Daresbury Laboratory, Warrington, United Kingdom
| | - S R Dennis
- STFC, Rutherford Appleton Laboratory, Harwell Oxford, and Daresbury Laboratory, Warrington, United Kingdom and University of Warwick, Department of Physics, Coventry, United Kingdom
| | - C Densham
- STFC, Rutherford Appleton Laboratory, Harwell Oxford, and Daresbury Laboratory, Warrington, United Kingdom
| | - F Di Lodovico
- Queen Mary University of London, School of Physics and Astronomy, London, United Kingdom
| | - S Di Luise
- ETH Zurich, Institute for Particle Physics, Zurich, Switzerland
| | - O Drapier
- Ecole Polytechnique, IN2P3-CNRS, Laboratoire Leprince-Ringuet, Palaiseau, France
| | - T Duboyski
- Queen Mary University of London, School of Physics and Astronomy, London, United Kingdom
| | - K Duffy
- Oxford University, Department of Physics, Oxford, United Kingdom
| | - F Dufour
- University of Geneva, Section de Physique, DPNC, Geneva, Switzerland
| | - J Dumarchez
- UPMC, Université Paris Diderot, CNRS/IN2P3, Laboratoire de Physique Nucléaire et de Hautes Energies (LPNHE), Paris, France
| | - S Dytman
- University of Pittsburgh, Department of Physics and Astronomy, Pittsburgh, Pennsylvania, USA
| | - M Dziewiecki
- Warsaw University of Technology, Institute of Radioelectronics, Warsaw, Poland
| | - S Emery
- IRFU, CEA Saclay, Gif-sur-Yvette, France
| | - A Ereditato
- University of Bern, Albert Einstein Center for Fundamental Physics, Laboratory for High Energy Physics (LHEP), Bern, Switzerland
| | - L Escudero
- IFIC (CSIC and University of Valencia), Valencia, Spain
| | - A J Finch
- Lancaster University, Physics Department, Lancaster, United Kingdom
| | - L Floetotto
- RWTH Aachen University, III. Physikalisches Institut, Aachen, Germany
| | - M Friend
- High Energy Accelerator Research Organization (KEK), Tsukuba, Ibaraki, Japan
| | - Y Fujii
- High Energy Accelerator Research Organization (KEK), Tsukuba, Ibaraki, Japan
| | - Y Fukuda
- Miyagi University of Education, Department of Physics, Sendai, Japan
| | - A P Furmanski
- University of Warwick, Department of Physics, Coventry, United Kingdom
| | - V Galymov
- IRFU, CEA Saclay, Gif-sur-Yvette, France
| | - A Gaudin
- University of Victoria, Department of Physics and Astronomy, Victoria, British Columbia, Canada
| | - S Giffin
- University of Regina, Department of Physics, Regina, Saskatchewan, Canada
| | - C Giganti
- UPMC, Université Paris Diderot, CNRS/IN2P3, Laboratoire de Physique Nucléaire et de Hautes Energies (LPNHE), Paris, France
| | - K Gilje
- State University of New York at Stony Brook, Department of Physics and Astronomy, Stony Brook, New York, USA
| | - D Goeldi
- University of Bern, Albert Einstein Center for Fundamental Physics, Laboratory for High Energy Physics (LHEP), Bern, Switzerland
| | - T Golan
- Wroclaw University, Faculty of Physics and Astronomy, Wroclaw, Poland
| | | | - M Gonin
- Ecole Polytechnique, IN2P3-CNRS, Laboratoire Leprince-Ringuet, Palaiseau, France
| | - N Grant
- Lancaster University, Physics Department, Lancaster, United Kingdom
| | - D Gudin
- Institute for Nuclear Research of the Russian Academy of Sciences, Moscow, Russia
| | - D R Hadley
- University of Warwick, Department of Physics, Coventry, United Kingdom
| | - A Haesler
- University of Geneva, Section de Physique, DPNC, Geneva, Switzerland
| | - M D Haigh
- University of Warwick, Department of Physics, Coventry, United Kingdom
| | - P Hamilton
- Imperial College London, Department of Physics, London, United Kingdom
| | - D Hansen
- University of Pittsburgh, Department of Physics and Astronomy, Pittsburgh, Pennsylvania, USA
| | - T Hara
- Kobe University, Kobe, Japan
| | - M Hartz
- Kavli Institute for the Physics and Mathematics of the Universe (WPI), Todai Institutes for Advanced Study, University of Tokyo, Kashiwa, Chiba, Japan and TRIUMF, Vancouver, British Columbia, Canada
| | - T Hasegawa
- High Energy Accelerator Research Organization (KEK), Tsukuba, Ibaraki, Japan
| | - N C Hastings
- University of Regina, Department of Physics, Regina, Saskatchewan, Canada
| | - Y Hayato
- University of Tokyo, Institute for Cosmic Ray Research, Kamioka Observatory, Kamioka, Japan
| | - C Hearty
- University of British Columbia, Department of Physics and Astronomy, Vancouver, British Columbia, Canada
| | - R L Helmer
- TRIUMF, Vancouver, British Columbia, Canada
| | - M Hierholzer
- University of Bern, Albert Einstein Center for Fundamental Physics, Laboratory for High Energy Physics (LHEP), Bern, Switzerland
| | - J Hignight
- State University of New York at Stony Brook, Department of Physics and Astronomy, Stony Brook, New York, USA
| | - A Hillairet
- University of Victoria, Department of Physics and Astronomy, Victoria, British Columbia, Canada
| | - A Himmel
- Duke University, Department of Physics, Durham, North Carolina, USA
| | - T Hiraki
- Kyoto University, Department of Physics, Kyoto, Japan
| | - S Hirota
- Kyoto University, Department of Physics, Kyoto, Japan
| | - J Holeczek
- University of Silesia, Institute of Physics, Katowice, Poland
| | - S Horikawa
- ETH Zurich, Institute for Particle Physics, Zurich, Switzerland
| | - K Huang
- Kyoto University, Department of Physics, Kyoto, Japan
| | - A K Ichikawa
- Kyoto University, Department of Physics, Kyoto, Japan
| | - K Ieki
- Kyoto University, Department of Physics, Kyoto, Japan
| | - M Ieva
- Institut de Fisica d'Altes Energies (IFAE), Bellaterra (Barcelona), Spain
| | - M Ikeda
- University of Tokyo, Institute for Cosmic Ray Research, Kamioka Observatory, Kamioka, Japan
| | - J Imber
- State University of New York at Stony Brook, Department of Physics and Astronomy, Stony Brook, New York, USA
| | - J Insler
- Louisiana State University, Department of Physics and Astronomy, Baton Rouge, Louisiana, USA
| | - T J Irvine
- University of Tokyo, Institute for Cosmic Ray Research, Research Center for Cosmic Neutrinos, Kashiwa, Japan
| | - T Ishida
- High Energy Accelerator Research Organization (KEK), Tsukuba, Ibaraki, Japan
| | - T Ishii
- High Energy Accelerator Research Organization (KEK), Tsukuba, Ibaraki, Japan
| | - S J Ives
- Imperial College London, Department of Physics, London, United Kingdom
| | - K Iyogi
- University of Tokyo, Institute for Cosmic Ray Research, Kamioka Observatory, Kamioka, Japan
| | - A Izmaylov
- IFIC (CSIC and University of Valencia), Valencia, Spain and Institute for Nuclear Research of the Russian Academy of Sciences, Moscow, Russia
| | - A Jacob
- Oxford University, Department of Physics, Oxford, United Kingdom
| | - B Jamieson
- University of Winnipeg, Department of Physics, Winnipeg, Manitoba, Canada
| | - R A Johnson
- University of Colorado at Boulder, Department of Physics, Boulder, Colorado, USA
| | - J H Jo
- State University of New York at Stony Brook, Department of Physics and Astronomy, Stony Brook, New York, USA
| | - P Jonsson
- Imperial College London, Department of Physics, London, United Kingdom
| | - C K Jung
- State University of New York at Stony Brook, Department of Physics and Astronomy, Stony Brook, New York, USA
| | - A C Kaboth
- Imperial College London, Department of Physics, London, United Kingdom
| | - T Kajita
- University of Tokyo, Institute for Cosmic Ray Research, Research Center for Cosmic Neutrinos, Kashiwa, Japan
| | - H Kakuno
- Tokyo Metropolitan University, Department of Physics, Tokyo, Japan
| | - J Kameda
- University of Tokyo, Institute for Cosmic Ray Research, Kamioka Observatory, Kamioka, Japan
| | - Y Kanazawa
- University of Tokyo, Department of Physics, Tokyo, Japan
| | - D Karlen
- TRIUMF, Vancouver, British Columbia, Canada and University of Victoria, Department of Physics and Astronomy, Victoria, British Columbia, Canada
| | - I Karpikov
- Institute for Nuclear Research of the Russian Academy of Sciences, Moscow, Russia
| | - E Kearns
- Boston University, Department of Physics, Boston, Massachusetts, USA and Kavli Institute for the Physics and Mathematics of the Universe (WPI), Todai Institutes for Advanced Study, University of Tokyo, Kashiwa, Chiba, Japan
| | - M Khabibullin
- Institute for Nuclear Research of the Russian Academy of Sciences, Moscow, Russia
| | - A Khotjantsev
- Institute for Nuclear Research of the Russian Academy of Sciences, Moscow, Russia
| | - D Kielczewska
- University of Warsaw, Faculty of Physics, Warsaw, Poland
| | - T Kikawa
- Kyoto University, Department of Physics, Kyoto, Japan
| | - A Kilinski
- National Centre for Nuclear Research, Warsaw, Poland
| | - J Kim
- University of British Columbia, Department of Physics and Astronomy, Vancouver, British Columbia, Canada
| | - J Kisiel
- University of Silesia, Institute of Physics, Katowice, Poland
| | - P Kitching
- University of Alberta, Centre for Particle Physics, Department of Physics, Edmonton, Alberta, Canada
| | - T Kobayashi
- High Energy Accelerator Research Organization (KEK), Tsukuba, Ibaraki, Japan
| | - L Koch
- RWTH Aachen University, III. Physikalisches Institut, Aachen, Germany
| | - A Kolaceke
- University of Regina, Department of Physics, Regina, Saskatchewan, Canada
| | - A Konaka
- TRIUMF, Vancouver, British Columbia, Canada
| | - L L Kormos
- Lancaster University, Physics Department, Lancaster, United Kingdom
| | - A Korzenev
- University of Geneva, Section de Physique, DPNC, Geneva, Switzerland
| | - K Koseki
- High Energy Accelerator Research Organization (KEK), Tsukuba, Ibaraki, Japan
| | - Y Koshio
- Okayama University, Department of Physics, Okayama, Japan
| | - I Kreslo
- University of Bern, Albert Einstein Center for Fundamental Physics, Laboratory for High Energy Physics (LHEP), Bern, Switzerland
| | - W Kropp
- University of California, Irvine, Department of Physics and Astronomy, Irvine, California, USA
| | - H Kubo
- Kyoto University, Department of Physics, Kyoto, Japan
| | - Y Kudenko
- Institute for Nuclear Research of the Russian Academy of Sciences, Moscow, Russia
| | | | - R Kurjata
- Warsaw University of Technology, Institute of Radioelectronics, Warsaw, Poland
| | - T Kutter
- Louisiana State University, Department of Physics and Astronomy, Baton Rouge, Louisiana, USA
| | - J Lagoda
- National Centre for Nuclear Research, Warsaw, Poland
| | - K Laihem
- RWTH Aachen University, III. Physikalisches Institut, Aachen, Germany
| | - I Lamont
- Lancaster University, Physics Department, Lancaster, United Kingdom
| | - M Laveder
- INFN Sezione di Padova and Università di Padova, Dipartimento di Fisica, Padova, Italy
| | - M Lawe
- University of Sheffield, Department of Physics and Astronomy, Sheffield, United Kingdom
| | - M Lazos
- University of Liverpool, Department of Physics, Liverpool, United Kingdom
| | - K P Lee
- University of Tokyo, Institute for Cosmic Ray Research, Research Center for Cosmic Neutrinos, Kashiwa, Japan
| | - C Licciardi
- University of Regina, Department of Physics, Regina, Saskatchewan, Canada
| | - T Lindner
- TRIUMF, Vancouver, British Columbia, Canada
| | - C Lister
- University of Warwick, Department of Physics, Coventry, United Kingdom
| | - R P Litchfield
- University of Warwick, Department of Physics, Coventry, United Kingdom
| | - A Longhin
- INFN Sezione di Padova and Università di Padova, Dipartimento di Fisica, Padova, Italy
| | - L Ludovici
- INFN Sezione di Roma and Università di Roma "La Sapienza", Roma, Italy
| | - M Macaire
- IRFU, CEA Saclay, Gif-sur-Yvette, France
| | - L Magaletti
- INFN Sezione di Bari and Università e Politecnico di Bari, Dipartimento Interuniversitario di Fisica, Bari, Italy
| | - K Mahn
- TRIUMF, Vancouver, British Columbia, Canada
| | - M Malek
- Imperial College London, Department of Physics, London, United Kingdom
| | - S Manly
- University of Rochester, Department of Physics and Astronomy, Rochester, New York, USA
| | - A D Marino
- University of Colorado at Boulder, Department of Physics, Boulder, Colorado, USA
| | - J Marteau
- Université de Lyon, Université Claude Bernard Lyon 1, IPN Lyon (IN2P3), Villeurbanne, France
| | - J F Martin
- University of Toronto, Department of Physics, Toronto, Ontario, Canada
| | - T Maruyama
- High Energy Accelerator Research Organization (KEK), Tsukuba, Ibaraki, Japan
| | - J Marzec
- Warsaw University of Technology, Institute of Radioelectronics, Warsaw, Poland
| | - E L Mathie
- University of Regina, Department of Physics, Regina, Saskatchewan, Canada
| | - V Matveev
- Institute for Nuclear Research of the Russian Academy of Sciences, Moscow, Russia
| | - K Mavrokoridis
- University of Liverpool, Department of Physics, Liverpool, United Kingdom
| | | | - M McCarthy
- University of British Columbia, Department of Physics and Astronomy, Vancouver, British Columbia, Canada
| | - N McCauley
- University of Liverpool, Department of Physics, Liverpool, United Kingdom
| | - K S McFarland
- University of Rochester, Department of Physics and Astronomy, Rochester, New York, USA
| | - C McGrew
- State University of New York at Stony Brook, Department of Physics and Astronomy, Stony Brook, New York, USA
| | - C Metelko
- University of Liverpool, Department of Physics, Liverpool, United Kingdom
| | - M Mezzetto
- INFN Sezione di Padova and Università di Padova, Dipartimento di Fisica, Padova, Italy
| | - P Mijakowski
- National Centre for Nuclear Research, Warsaw, Poland
| | - C A Miller
- TRIUMF, Vancouver, British Columbia, Canada
| | - A Minamino
- Kyoto University, Department of Physics, Kyoto, Japan
| | - O Mineev
- Institute for Nuclear Research of the Russian Academy of Sciences, Moscow, Russia
| | - S Mine
- University of California, Irvine, Department of Physics and Astronomy, Irvine, California, USA
| | - A Missert
- University of Colorado at Boulder, Department of Physics, Boulder, Colorado, USA
| | - M Miura
- University of Tokyo, Institute for Cosmic Ray Research, Kamioka Observatory, Kamioka, Japan
| | - L Monfregola
- IFIC (CSIC and University of Valencia), Valencia, Spain
| | - S Moriyama
- University of Tokyo, Institute for Cosmic Ray Research, Kamioka Observatory, Kamioka, Japan
| | - Th A Mueller
- Ecole Polytechnique, IN2P3-CNRS, Laboratoire Leprince-Ringuet, Palaiseau, France
| | - A Murakami
- Kyoto University, Department of Physics, Kyoto, Japan
| | - M Murdoch
- University of Liverpool, Department of Physics, Liverpool, United Kingdom
| | - S Murphy
- ETH Zurich, Institute for Particle Physics, Zurich, Switzerland
| | - J Myslik
- University of Victoria, Department of Physics and Astronomy, Victoria, British Columbia, Canada
| | - T Nagasaki
- Kyoto University, Department of Physics, Kyoto, Japan
| | - T Nakadaira
- High Energy Accelerator Research Organization (KEK), Tsukuba, Ibaraki, Japan
| | - M Nakahata
- Kavli Institute for the Physics and Mathematics of the Universe (WPI), Todai Institutes for Advanced Study, University of Tokyo, Kashiwa, Chiba, Japan and University of Tokyo, Institute for Cosmic Ray Research, Kamioka Observatory, Kamioka, Japan
| | - T Nakai
- Osaka City University, Department of Physics, Osaka, Japan
| | - K Nakamura
- High Energy Accelerator Research Organization (KEK), Tsukuba, Ibaraki, Japan and Kavli Institute for the Physics and Mathematics of the Universe (WPI), Todai Institutes for Advanced Study, University of Tokyo, Kashiwa, Chiba, Japan
| | - S Nakayama
- University of Tokyo, Institute for Cosmic Ray Research, Kamioka Observatory, Kamioka, Japan
| | - T Nakaya
- Kavli Institute for the Physics and Mathematics of the Universe (WPI), Todai Institutes for Advanced Study, University of Tokyo, Kashiwa, Chiba, Japan and Kyoto University, Department of Physics, Kyoto, Japan
| | - K Nakayoshi
- High Energy Accelerator Research Organization (KEK), Tsukuba, Ibaraki, Japan
| | - D Naples
- University of Pittsburgh, Department of Physics and Astronomy, Pittsburgh, Pennsylvania, USA
| | - C Nielsen
- University of British Columbia, Department of Physics and Astronomy, Vancouver, British Columbia, Canada
| | - M Nirkko
- University of Bern, Albert Einstein Center for Fundamental Physics, Laboratory for High Energy Physics (LHEP), Bern, Switzerland
| | - K Nishikawa
- High Energy Accelerator Research Organization (KEK), Tsukuba, Ibaraki, Japan
| | - Y Nishimura
- University of Tokyo, Institute for Cosmic Ray Research, Research Center for Cosmic Neutrinos, Kashiwa, Japan
| | - H M O'Keeffe
- Lancaster University, Physics Department, Lancaster, United Kingdom
| | - R Ohta
- High Energy Accelerator Research Organization (KEK), Tsukuba, Ibaraki, Japan
| | - K Okumura
- Kavli Institute for the Physics and Mathematics of the Universe (WPI), Todai Institutes for Advanced Study, University of Tokyo, Kashiwa, Chiba, Japan and University of Tokyo, Institute for Cosmic Ray Research, Research Center for Cosmic Neutrinos, Kashiwa, Japan
| | - T Okusawa
- Osaka City University, Department of Physics, Osaka, Japan
| | - W Oryszczak
- University of Warsaw, Faculty of Physics, Warsaw, Poland
| | - S M Oser
- University of British Columbia, Department of Physics and Astronomy, Vancouver, British Columbia, Canada
| | - R A Owen
- Queen Mary University of London, School of Physics and Astronomy, London, United Kingdom
| | - Y Oyama
- High Energy Accelerator Research Organization (KEK), Tsukuba, Ibaraki, Japan
| | - V Palladino
- INFN Sezione di Napoli and Università di Napoli, Dipartimento di Fisica, Napoli, Italy
| | - V Paolone
- University of Pittsburgh, Department of Physics and Astronomy, Pittsburgh, Pennsylvania, USA
| | - D Payne
- University of Liverpool, Department of Physics, Liverpool, United Kingdom
| | - G F Pearce
- STFC, Rutherford Appleton Laboratory, Harwell Oxford, and Daresbury Laboratory, Warrington, United Kingdom
| | - O Perevozchikov
- Louisiana State University, Department of Physics and Astronomy, Baton Rouge, Louisiana, USA
| | - J D Perkin
- University of Sheffield, Department of Physics and Astronomy, Sheffield, United Kingdom
| | - Y Petrov
- University of British Columbia, Department of Physics and Astronomy, Vancouver, British Columbia, Canada
| | - L J Pickard
- University of Sheffield, Department of Physics and Astronomy, Sheffield, United Kingdom
| | - E S Pinzon Guerra
- York University, Department of Physics and Astronomy, Toronto, Ontario, Canada
| | - C Pistillo
- University of Bern, Albert Einstein Center for Fundamental Physics, Laboratory for High Energy Physics (LHEP), Bern, Switzerland
| | - P Plonski
- Warsaw University of Technology, Institute of Radioelectronics, Warsaw, Poland
| | - E Poplawska
- Queen Mary University of London, School of Physics and Astronomy, London, United Kingdom
| | - B Popov
- UPMC, Université Paris Diderot, CNRS/IN2P3, Laboratoire de Physique Nucléaire et de Hautes Energies (LPNHE), Paris, France
| | - M Posiadala
- University of Warsaw, Faculty of Physics, Warsaw, Poland
| | | | | | - P Przewlocki
- National Centre for Nuclear Research, Warsaw, Poland
| | - B Quilain
- Ecole Polytechnique, IN2P3-CNRS, Laboratoire Leprince-Ringuet, Palaiseau, France
| | - E Radicioni
- INFN Sezione di Bari and Università e Politecnico di Bari, Dipartimento Interuniversitario di Fisica, Bari, Italy
| | - P N Ratoff
- Lancaster University, Physics Department, Lancaster, United Kingdom
| | - M Ravonel
- University of Geneva, Section de Physique, DPNC, Geneva, Switzerland
| | - M A M Rayner
- University of Geneva, Section de Physique, DPNC, Geneva, Switzerland
| | - A Redij
- University of Bern, Albert Einstein Center for Fundamental Physics, Laboratory for High Energy Physics (LHEP), Bern, Switzerland
| | - M Reeves
- Lancaster University, Physics Department, Lancaster, United Kingdom
| | - E Reinherz-Aronis
- Colorado State University, Department of Physics, Fort Collins, Colorado, USA
| | - F Retiere
- TRIUMF, Vancouver, British Columbia, Canada
| | - A Robert
- UPMC, Université Paris Diderot, CNRS/IN2P3, Laboratoire de Physique Nucléaire et de Hautes Energies (LPNHE), Paris, France
| | - P A Rodrigues
- University of Rochester, Department of Physics and Astronomy, Rochester, New York, USA
| | - P Rojas
- Colorado State University, Department of Physics, Fort Collins, Colorado, USA
| | - E Rondio
- National Centre for Nuclear Research, Warsaw, Poland
| | - S Roth
- RWTH Aachen University, III. Physikalisches Institut, Aachen, Germany
| | - A Rubbia
- ETH Zurich, Institute for Particle Physics, Zurich, Switzerland
| | - D Ruterbories
- Colorado State University, Department of Physics, Fort Collins, Colorado, USA
| | - R Sacco
- Queen Mary University of London, School of Physics and Astronomy, London, United Kingdom
| | - K Sakashita
- High Energy Accelerator Research Organization (KEK), Tsukuba, Ibaraki, Japan
| | - F Sánchez
- Institut de Fisica d'Altes Energies (IFAE), Bellaterra (Barcelona), Spain
| | - F Sato
- High Energy Accelerator Research Organization (KEK), Tsukuba, Ibaraki, Japan
| | - E Scantamburlo
- University of Geneva, Section de Physique, DPNC, Geneva, Switzerland
| | - K Scholberg
- Duke University, Department of Physics, Durham, North Carolina, USA
| | - J Schwehr
- Colorado State University, Department of Physics, Fort Collins, Colorado, USA
| | - M Scott
- TRIUMF, Vancouver, British Columbia, Canada
| | - Y Seiya
- Osaka City University, Department of Physics, Osaka, Japan
| | - T Sekiguchi
- High Energy Accelerator Research Organization (KEK), Tsukuba, Ibaraki, Japan
| | - H Sekiya
- University of Tokyo, Institute for Cosmic Ray Research, Kamioka Observatory, Kamioka, Japan
| | - D Sgalaberna
- ETH Zurich, Institute for Particle Physics, Zurich, Switzerland
| | - M Shiozawa
- Kavli Institute for the Physics and Mathematics of the Universe (WPI), Todai Institutes for Advanced Study, University of Tokyo, Kashiwa, Chiba, Japan and University of Tokyo, Institute for Cosmic Ray Research, Kamioka Observatory, Kamioka, Japan
| | - S Short
- Imperial College London, Department of Physics, London, United Kingdom
| | - Y Shustrov
- Institute for Nuclear Research of the Russian Academy of Sciences, Moscow, Russia
| | - P Sinclair
- Imperial College London, Department of Physics, London, United Kingdom
| | - B Smith
- Imperial College London, Department of Physics, London, United Kingdom
| | - R J Smith
- Oxford University, Department of Physics, Oxford, United Kingdom
| | - M Smy
- University of California, Irvine, Department of Physics and Astronomy, Irvine, California, USA
| | - J T Sobczyk
- Wroclaw University, Faculty of Physics and Astronomy, Wroclaw, Poland
| | - H Sobel
- University of California, Irvine, Department of Physics and Astronomy, Irvine, California, USA and Kavli Institute for the Physics and Mathematics of the Universe (WPI), Todai Institutes for Advanced Study, University of Tokyo, Kashiwa, Chiba, Japan
| | - M Sorel
- IFIC (CSIC and University of Valencia), Valencia, Spain
| | - L Southwell
- Lancaster University, Physics Department, Lancaster, United Kingdom
| | - P Stamoulis
- IFIC (CSIC and University of Valencia), Valencia, Spain
| | - J Steinmann
- RWTH Aachen University, III. Physikalisches Institut, Aachen, Germany
| | - B Still
- Queen Mary University of London, School of Physics and Astronomy, London, United Kingdom
| | - Y Suda
- University of Tokyo, Department of Physics, Tokyo, Japan
| | | | - K Suzuki
- Kyoto University, Department of Physics, Kyoto, Japan
| | - S Y Suzuki
- High Energy Accelerator Research Organization (KEK), Tsukuba, Ibaraki, Japan
| | - Y Suzuki
- Kavli Institute for the Physics and Mathematics of the Universe (WPI), Todai Institutes for Advanced Study, University of Tokyo, Kashiwa, Chiba, Japan and University of Tokyo, Institute for Cosmic Ray Research, Kamioka Observatory, Kamioka, Japan
| | - T Szeglowski
- University of Silesia, Institute of Physics, Katowice, Poland
| | - R Tacik
- University of Regina, Department of Physics, Regina, Saskatchewan, Canada and TRIUMF, Vancouver, British Columbia, Canada
| | - M Tada
- High Energy Accelerator Research Organization (KEK), Tsukuba, Ibaraki, Japan
| | - S Takahashi
- Kyoto University, Department of Physics, Kyoto, Japan
| | - A Takeda
- University of Tokyo, Institute for Cosmic Ray Research, Kamioka Observatory, Kamioka, Japan
| | - Y Takeuchi
- Kavli Institute for the Physics and Mathematics of the Universe (WPI), Todai Institutes for Advanced Study, University of Tokyo, Kashiwa, Chiba, Japan and Kobe University, Kobe, Japan
| | - H K Tanaka
- University of Tokyo, Institute for Cosmic Ray Research, Kamioka Observatory, Kamioka, Japan
| | - H A Tanaka
- University of British Columbia, Department of Physics and Astronomy, Vancouver, British Columbia, Canada
| | - M M Tanaka
- High Energy Accelerator Research Organization (KEK), Tsukuba, Ibaraki, Japan
| | - D Terhorst
- RWTH Aachen University, III. Physikalisches Institut, Aachen, Germany
| | - R Terri
- Queen Mary University of London, School of Physics and Astronomy, London, United Kingdom
| | - L F Thompson
- University of Sheffield, Department of Physics and Astronomy, Sheffield, United Kingdom
| | - A Thorley
- University of Liverpool, Department of Physics, Liverpool, United Kingdom
| | - S Tobayama
- University of British Columbia, Department of Physics and Astronomy, Vancouver, British Columbia, Canada
| | - W Toki
- Colorado State University, Department of Physics, Fort Collins, Colorado, USA
| | - T Tomura
- University of Tokyo, Institute for Cosmic Ray Research, Kamioka Observatory, Kamioka, Japan
| | - Y Totsuka
- University of Alberta, Centre for Particle Physics, Department of Physics, Edmonton, Alberta, Canada and University of Bern, Albert Einstein Center for Fundamental Physics, Laboratory for High Energy Physics (LHEP), Bern, Switzerland and Boston University, Department of Physics, Boston, Massachusetts, USA and University of British Columbia, Department of Physics and Astronomy, Vancouver, British Columbia, Canada and University of California, Irvine, Department of Physics and Astronomy, Irvine, California, USA and IRFU, CEA Saclay, Gif-sur-Yvette, France and University of Colorado at Boulder, Department of Physics, Boulder, Colorado, USA and Colorado State University, Department of Physics, Fort Collins, Colorado, USA and Duke University, Department of Physics, Durham, North Carolina, USA and Ecole Polytechnique, IN2P3-CNRS, Laboratoire Leprince-Ringuet, Palaiseau, France and ETH Zurich, Institute for Particle Physics, Zurich, Switzerland and University of Geneva, Section de Physique, DPNC, Geneva, Switzerland and H. Niewodniczanski Institute of Nuclear Physics PAN, Cracow, Poland and High Energy Accelerator Research Organization (KEK), Tsukuba, Ibaraki, Japan and Institut de Fisica d'Altes Energies (IFAE), Bellaterra (Barcelona), Spain and IFIC (CSIC and University of Valencia), Valencia, Spain and Imperial College London, Department of Physics, London, United Kingdom and INFN Sezione di Bari and Università e Politecnico di Bari, Dipartimento Interuniversitario di Fisica, Bari, Italy and INFN Sezione di Napoli and Università di Napoli, Dipartimento di Fisica, Napoli, Italy and INFN Sezione di Padova and Università di Padova, Dipartimento di Fisica, Padova, Italy and INFN Sezione di Roma and Università di Roma "La Sapienza", Roma, Italy and Institute for Nuclear Research of the Russian Academy of Sciences, Moscow, Russia and Kavli Institute for the Physics and Mathematics of the Universe (WPI), Todai Institutes for Advanced Study, University of Tokyo, Kashiwa, Ch
| | - C Touramanis
- University of Liverpool, Department of Physics, Liverpool, United Kingdom
| | - T Tsukamoto
- High Energy Accelerator Research Organization (KEK), Tsukuba, Ibaraki, Japan
| | - M Tzanov
- Louisiana State University, Department of Physics and Astronomy, Baton Rouge, Louisiana, USA
| | - Y Uchida
- Imperial College London, Department of Physics, London, United Kingdom
| | - K Ueno
- University of Tokyo, Institute for Cosmic Ray Research, Kamioka Observatory, Kamioka, Japan
| | - A Vacheret
- Oxford University, Department of Physics, Oxford, United Kingdom
| | - M Vagins
- University of California, Irvine, Department of Physics and Astronomy, Irvine, California, USA and Kavli Institute for the Physics and Mathematics of the Universe (WPI), Todai Institutes for Advanced Study, University of Tokyo, Kashiwa, Chiba, Japan
| | - G Vasseur
- IRFU, CEA Saclay, Gif-sur-Yvette, France
| | - T Wachala
- H. Niewodniczanski Institute of Nuclear Physics PAN, Cracow, Poland
| | - A V Waldron
- Oxford University, Department of Physics, Oxford, United Kingdom
| | - C W Walter
- Duke University, Department of Physics, Durham, North Carolina, USA
| | - D Wark
- Imperial College London, Department of Physics, London, United Kingdom and STFC, Rutherford Appleton Laboratory, Harwell Oxford, and Daresbury Laboratory, Warrington, United Kingdom
| | - M O Wascko
- Imperial College London, Department of Physics, London, United Kingdom
| | - A Weber
- Oxford University, Department of Physics, Oxford, United Kingdom and STFC, Rutherford Appleton Laboratory, Harwell Oxford, and Daresbury Laboratory, Warrington, United Kingdom
| | - R Wendell
- University of Tokyo, Institute for Cosmic Ray Research, Kamioka Observatory, Kamioka, Japan
| | - R J Wilkes
- University of Washington, Department of Physics, Seattle, Washington, USA
| | | | - C Wilkinson
- University of Sheffield, Department of Physics and Astronomy, Sheffield, United Kingdom
| | - Z Williamson
- Oxford University, Department of Physics, Oxford, United Kingdom
| | - J R Wilson
- Queen Mary University of London, School of Physics and Astronomy, London, United Kingdom
| | - R J Wilson
- Colorado State University, Department of Physics, Fort Collins, Colorado, USA
| | - T Wongjirad
- Duke University, Department of Physics, Durham, North Carolina, USA
| | - Y Yamada
- High Energy Accelerator Research Organization (KEK), Tsukuba, Ibaraki, Japan
| | - K Yamamoto
- Osaka City University, Department of Physics, Osaka, Japan
| | - C Yanagisawa
- State University of New York at Stony Brook, Department of Physics and Astronomy, Stony Brook, New York, USA
| | - S Yen
- TRIUMF, Vancouver, British Columbia, Canada
| | - N Yershov
- Institute for Nuclear Research of the Russian Academy of Sciences, Moscow, Russia
| | - M Yokoyama
- University of Tokyo, Department of Physics, Tokyo, Japan
| | - T Yuan
- University of Colorado at Boulder, Department of Physics, Boulder, Colorado, USA
| | - A Zalewska
- H. Niewodniczanski Institute of Nuclear Physics PAN, Cracow, Poland
| | - J Zalipska
- National Centre for Nuclear Research, Warsaw, Poland
| | - L Zambelli
- UPMC, Université Paris Diderot, CNRS/IN2P3, Laboratoire de Physique Nucléaire et de Hautes Energies (LPNHE), Paris, France
| | - K Zaremba
- Warsaw University of Technology, Institute of Radioelectronics, Warsaw, Poland
| | - M Ziembicki
- Warsaw University of Technology, Institute of Radioelectronics, Warsaw, Poland
| | - E D Zimmerman
- University of Colorado at Boulder, Department of Physics, Boulder, Colorado, USA
| | - M Zito
- IRFU, CEA Saclay, Gif-sur-Yvette, France
| | - J Zmuda
- Wroclaw University, Faculty of Physics and Astronomy, Wroclaw, Poland
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Ma K, Farajzadeh R, Lopez-Salinas JL, Miller CA, Biswal SL, Hirasaki GJ. Non-uniqueness, Numerical Artifacts, and Parameter Sensitivity in Simulating Steady-State and Transient Foam Flow Through Porous Media. Transp Porous Media 2014. [DOI: 10.1007/s11242-014-0276-9] [Citation(s) in RCA: 46] [Impact Index Per Article: 4.6] [Reference Citation Analysis] [What about the content of this article? (0)] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/30/2022]
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Abe K, Adam J, Aihara H, Akiri T, Andreopoulos C, Aoki S, Ariga A, Ariga T, Assylbekov S, Autiero D, Barbi M, Barker GJ, Barr G, Bass M, Batkiewicz M, Bay F, Bentham SW, Berardi V, Berger BE, Berkman S, Bertram I, Bhadra S, Blaszczyk FDM, Blondel A, Bojechko C, Bordoni S, Boyd SB, Brailsford D, Bravar A, Bronner C, Buchanan N, Calland RG, Caravaca Rodríguez J, Cartwright SL, Castillo R, Catanesi MG, Cervera A, Cherdack D, Christodoulou G, Clifton A, Coleman J, Coleman SJ, Collazuol G, Connolly K, Cremonesi L, Curioni A, Dabrowska A, Danko I, Das R, Davis S, de Perio P, De Rosa G, Dealtry T, Dennis SR, Densham C, Di Lodovico F, Di Luise S, Drapier O, Duboyski T, Duffy K, Dufour F, Dumarchez J, Dytman S, Dziewiecki M, Emery S, Ereditato A, Escudero L, Finch AJ, Frank E, Friend M, Fujii Y, Fukuda Y, Furmanski AP, Galymov V, Gaudin A, Giffin S, Giganti C, Gilje K, Golan T, Gomez-Cadenas JJ, Gonin M, Grant N, Gudin D, Hadley DR, Haesler A, Haigh MD, Hamilton P, Hansen D, Hara T, Hartz M, Hasegawa T, Hastings NC, Hayato Y, Hearty C, Helmer RL, Hierholzer M, Hignight J, Hillairet A, Himmel A, Hiraki T, Hirota S, Holeczek J, Horikawa S, Huang K, Ichikawa AK, Ieki K, Ieva M, Ikeda M, Imber J, Insler J, Irvine TJ, Ishida T, Ishii T, Ives SJ, Iyogi K, Izmaylov A, Jacob A, Jamieson B, Johnson RA, Jo JH, Jonsson P, Joo KK, Jung CK, Kaboth AC, Kajita T, Kakuno H, Kameda J, Kanazawa Y, Karlen D, Karpikov I, Kearns E, Khabibullin M, Khotjantsev A, Kielczewska D, Kikawa T, Kilinski A, Kim J, Kim SB, Kisiel J, Kitching P, Kobayashi T, Kogan G, Kolaceke A, Konaka A, Kormos LL, Korzenev A, Koseki K, Koshio Y, Kreslo I, Kropp W, Kubo H, Kudenko Y, Kumaratunga S, Kurjata R, Kutter T, Lagoda J, Laihem K, Laveder M, Lawe M, Lazos M, Lee KP, Licciardi C, Lim IT, Lindner T, Lister C, Litchfield RP, Longhin A, Lopez GD, Ludovici L, Macaire M, Magaletti L, Mahn K, Malek M, Manly S, Marino AD, Marteau J, Martin JF, Maruyama T, Marzec J, Masliah P, Mathie EL, Matveev V, Mavrokoridis K, Mazzucato E, McCarthy M, McCauley N, McFarland KS, McGrew C, Metelko C, Mijakowski P, Miller CA, Minamino A, Mineev O, Mine S, Missert A, Miura M, Monfregola L, Moriyama S, Mueller TA, Murakami A, Murdoch M, Murphy S, Myslik J, Nagasaki T, Nakadaira T, Nakahata M, Nakai T, Nakamura K, Nakayama S, Nakaya T, Nakayoshi K, Naples D, Nielsen C, Nirkko M, Nishikawa K, Nishimura Y, O'Keeffe HM, Ohta R, Okumura K, Okusawa T, Oryszczak W, Oser SM, Otani M, Owen RA, Oyama Y, Pac MY, Palladino V, Paolone V, Payne D, Pearce GF, Perevozchikov O, Perkin JD, Petrov Y, Pinzon Guerra ES, Pistillo C, Plonski P, Poplawska E, Popov B, Posiadala M, Poutissou JM, Poutissou R, Przewlocki P, Quilain B, Radicioni E, Ratoff PN, Ravonel M, Rayner MAM, Redij A, Reeves M, Reinherz-Aronis E, Retiere F, Robert A, Rodrigues PA, Rondio E, Roth S, Rubbia A, Ruterbories D, Sacco R, Sakashita K, Sánchez F, Sato F, Scantamburlo E, Scholberg K, Schwehr J, Scott M, Seiya Y, Sekiguchi T, Sekiya H, Sgalaberna D, Shiozawa M, Short S, Shustrov Y, Sinclair P, Smith B, Smith RJ, Smy M, Sobczyk JT, Sobel H, Sorel M, Southwell L, Stamoulis P, Steinmann J, Still B, Suda Y, Suzuki A, Suzuki K, Suzuki SY, Suzuki Y, Szeglowski T, Tacik R, Tada M, Takahashi S, Takeda A, Takeuchi Y, Tanaka HK, Tanaka HA, Tanaka MM, Taylor IJ, Terhorst D, Terri R, Thompson LF, Thorley A, Tobayama S, Toki W, Tomura T, Totsuka Y, Touramanis C, Tsukamoto T, Tzanov M, Uchida Y, Ueno K, Vacheret A, Vagins M, Vasseur G, Wachala T, Waldron AV, Walter CW, Wark D, Wascko MO, Weber A, Wendell R, Wilkes RJ, Wilking MJ, Wilkinson C, Williamson Z, Wilson JR, Wilson RJ, Wongjirad T, Yamada Y, Yamamoto K, Yanagisawa C, Yen S, Yershov N, Yokoyama M, Yuan T, Zalewska A, Zalipska J, Zambelli L, Zaremba K, Ziembicki M, Zimmerman ED, Zito M, Zmuda J. Measurement of neutrino oscillation parameters from muon neutrino disappearance with an off-axis beam. Phys Rev Lett 2013; 111:211803. [PMID: 24313479 DOI: 10.1103/physrevlett.111.211803] [Citation(s) in RCA: 6] [Impact Index Per Article: 0.5] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Received: 07/31/2013] [Revised: 10/09/2013] [Indexed: 06/02/2023]
Abstract
The T2K Collaboration reports a precision measurement of muon neutrino disappearance with an off-axis neutrino beam with a peak energy of 0.6 GeV. Near detector measurements are used to constrain the neutrino flux and cross section parameters. The Super-Kamiokande far detector, which is 295 km downstream of the neutrino production target, collected data corresponding to 3.01×10(20) protons on target. In the absence of neutrino oscillations, 205±17 (syst) events are expected to be detected while only 58 muon neutrino event candidates are observed. A fit to the neutrino rate and energy spectrum, assuming three neutrino flavors and normal mass hierarchy yields a best-fit mixing angle sin2(θ23)=0.514±0.082 and mass splitting |Δm(32)(2)|=2.44(-0.15)(+0.17)×10(-3) eV2/c4. Our result corresponds to the maximal oscillation disappearance probability.
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Affiliation(s)
- K Abe
- University of Tokyo, Institute for Cosmic Ray Research, Kamioka Observatory, Kamioka, Japan
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Bozeya A, Al-Bawab A, Friberg SE, Miller CA. Spontaneous Emulsification and Phase Equilibria in the System Water, Ethanol, and Benzene. J DISPER SCI TECHNOL 2013. [DOI: 10.1080/01932691.2012.743363] [Citation(s) in RCA: 4] [Impact Index Per Article: 0.4] [Reference Citation Analysis] [What about the content of this article? (0)] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 10/27/2022]
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Johnson A, Al-Kaisy N, Miller CA, Martin N. The effect of denture design and fixatives on the retention of mandibular complete dentures tested on a novel in-vitro edentulous model. Eur J Prosthodont Restor Dent 2013; 21:64-74. [PMID: 23888529] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [MESH Headings] [Subscribe] [Scholar Register] [Indexed: 06/02/2023]
Abstract
The aim of this study was to evaluate the effect of the design (extension and adaptation) of a mandibular complete acrylic denture and the use of denture adhesives using a novel in-vitro edentulous model. The model is a highly anatomically accurate replica based on a moderately resorbed human mandibular edentulous arch. The model has been designed and fabricated by means of an elaborate clinical and technical process that employs synthetic elastomeric materials with properties that attempts to reproduce in-vitro characteristics of the soft tissues overlying the ridges and immediate reflected tissues. This model was used to measure and compare the retention of mandibular dentures ofvarying designs (well-fitting, over- and under-extended) with and without the aid of denture fixatives. Retention tests were conducted with different volumes of artificial saliva at a cross head speed of 50 mm/min with 4 equidistant holding points on the denture occlusal surface, using a universal tensile testing machine in an axial pull direction. The effect of three denture adhesives on denture retention was also tested on the same denture types at different times over a period of 5 hours and beyond. The in-vitro model presented can be effectively used to test the retention of mandibular complete dentures. The speed of dislodgement force and amount of saliva are important variables in mandibular denture retention. The retention of well-fitting dentures was statistically higher than that of ill-fitting dentures. A significantly higher retention force was needed to dislodge mandibular dentures (well and ill-fitting dentures) when using a denture adhesive.
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Affiliation(s)
- A Johnson
- School of Clinical Dentistry, University of Sheffield, Claremont Cresent, Sheffield.
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Miller CA, Naish J, Bishop P, Coutts G, Clark D, Zhou S, Ray SG, Yonan N, Williams SG, Flett AS, Moon JC, Parker GJM, Schmitt M. 083 HISTOLOGICAL VALIDATION OF DYNAMIC-EQUILIBRIUM CARDIOVASCULAR MAGNETIC RESONANCE FOR THE ASSESSMENT OF MYOCARDIAL EXTRACELLULAR VOLUME. Heart 2013. [DOI: 10.1136/heartjnl-2013-304019.83] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Track Full Text] [Subscribe] [Scholar Register] [Indexed: 11/03/2022]
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Miller CA, Naish J, Coutts G, Clark D, Zhou S, Ray SG, Parker GJM, Schmitt M. 084 EFFECT OF CONTRAST DOSE, POST-CONTRAST ACQUISITION TIME, MYOCARDIAL REGIONALITY, CARDIAC CYCLE AND GENDER ON DYNAMIC-EQUILIBRIUM CONTRAST CMR MEASUREMENT OF MYOCARDIAL EXTRACELLULAR VOLUME. Heart 2013. [DOI: 10.1136/heartjnl-2013-304019.84] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Track Full Text] [Subscribe] [Scholar Register] [Indexed: 11/03/2022]
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Walter MJ, Shen D, Shao J, Ding L, White BS, Kandoth C, Miller CA, Niu B, McLellan MD, Dees ND, Fulton R, Elliot K, Heath S, Grillot M, Westervelt P, Link DC, DiPersio JF, Mardis E, Ley TJ, Wilson RK, Graubert TA. Clonal diversity of recurrently mutated genes in myelodysplastic syndromes. Leukemia 2013; 27:1275-82. [PMID: 23443460 DOI: 10.1038/leu.2013.58] [Citation(s) in RCA: 235] [Impact Index Per Article: 21.4] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 12/16/2022]
Abstract
Recent studies suggest that most cases of myelodysplastic syndrome (MDS) are clonally heterogeneous, with a founding clone and multiple subclones. It is not known whether specific gene mutations typically occur in founding clones or subclones. We screened a panel of 94 candidate genes in a cohort of 157 patients with MDS or secondary acute myeloid leukemia (sAML). This included 150 cases with samples obtained at MDS diagnosis and 15 cases with samples obtained at sAML transformation (8 were also analyzed at the MDS stage). We performed whole-genome sequencing (WGS) to define the clonal architecture in eight sAML genomes and identified the range of variant allele frequencies (VAFs) for founding clone mutations. At least one mutation or cytogenetic abnormality was detected in 83% of the 150 MDS patients and 17 genes were significantly mutated (false discovery rate ≤0.05). Individual genes and patient samples displayed a wide range of VAFs for recurrently mutated genes, indicating that no single gene is exclusively mutated in the founding clone. The VAFs of recurrently mutated genes did not fully recapitulate the clonal architecture defined by WGS, suggesting that comprehensive sequencing may be required to accurately assess the clonal status of recurrently mutated genes in MDS.
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Affiliation(s)
- M J Walter
- Division of Oncology, Department of Internal Medicine, Washington University School of Medicine, St Louis, MO, USA
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Hynes AM, Miller CA, Eley L, Simms RJ, White K, Miles C, Sayer JA. Characterising a novel mouse model with a mutated ciliopathy gene (Cep290) leading to Joubert Syndrome. Cilia 2012. [PMCID: PMC3555904 DOI: 10.1186/2046-2530-1-s1-p89] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Track Full Text] [Download PDF] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/29/2022] Open
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Rajan E, Gostout CJ, Bonin EA, Moran EA, Locke GR, Szarka LA, Talley NJ, Deters JL, Miller CA, Knipschield MA, Lurken MS, Stoltz GJ, Bernard CE, Grover M, Farrugia G. Endoscopic full-thickness biopsy of the gastric wall with defect closure by using an endoscopic suturing device: survival porcine study. Gastrointest Endosc 2012; 76:1014-9. [PMID: 23078926 PMCID: PMC3666864 DOI: 10.1016/j.gie.2012.07.010] [Citation(s) in RCA: 33] [Impact Index Per Article: 2.8] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Journal Information] [Submit a Manuscript] [Subscribe] [Scholar Register] [Received: 04/19/2012] [Accepted: 07/06/2012] [Indexed: 02/08/2023]
Abstract
BACKGROUND The pathogenesis of several common gastric motility diseases and functional GI disorders remains essentially unexplained. Gastric wall biopsies that include the muscularis propria to evaluate the enteric nervous system, interstitial cells of Cajal, and immune cells can provide important insights for our understanding of the etiology of these disorders. OBJECTIVES To determine the technical feasibility, reproducibility, and safety of performing a full-thickness gastric biopsy (FTGB) by using a submucosal endoscopy with mucosal flap (SEMF) technique; the technical feasibility, reproducibility, and safety of tissue closure by using an endoscopic suturing device; the ability to identify myenteric ganglia in resected specimens; and the long-term safety. DESIGN Single center, preclinical survival study. SETTING Animal research laboratory, developmental endoscopy unit. SUBJECTS Twelve domestic pigs. INTERVENTIONS Animals underwent an SEMF procedure with gastric muscularis propria resection. The resultant offset mucosal entry site was closed by using an endoscopic suturing device. Animals were kept alive for 2 weeks. MAIN OUTCOME MEASUREMENTS The technical feasibility, reproducibility, and safety of the procedure; the clinical course of the animals; the histological and immunochemical evaluation of the resected specimen to determine whether myenteric ganglia were present in the sample. RESULTS FTGB was performed by using the SEMF technique in all 12 animals. The offset mucosal entry site was successfully closed by using the suturing device in all animals. The mean resected tissue specimen size was 11 mm. Mean total procedure time was 61 minutes with 2 to 4 interrupted sutures placed per animal. Histology showed muscularis propria and serosa, confirming full-thickness resections in all animals. Myenteric ganglia were visualized in 11 of 12 animals. The clinical course was uneventful. Repeat endoscopy and necropsy at 2 weeks showed absence of ulceration at both the mucosal entry sites and overlying the more distal muscularis propria resection sites. There was complete healing of the serosa in all animals with minimal single-band adhesions in 5 of 12 animals. Retained sutures were present in 10 of 12 animals. LIMITATIONS Animal experiment. CONCLUSIONS FTGB by using the SEMF technique and an endoscopic suturing device is technically feasible, reproducible, and safe. Larger tissue specimens will allow improved analysis of multiple cell types.
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Affiliation(s)
| | | | | | | | - GR Locke
- Developmental Endoscopy Unit and Enteric NeuroScience Program, Division of Gastroenterology and Hepatology, Mayo Clinic College of Medicine, 200 First St. SW, Rochester, MN 55905
| | - LA Szarka
- Developmental Endoscopy Unit and Enteric NeuroScience Program, Division of Gastroenterology and Hepatology, Mayo Clinic College of Medicine, 200 First St. SW, Rochester, MN 55905
| | | | | | | | | | | | - GJ Stoltz
- Developmental Endoscopy Unit and Enteric NeuroScience Program, Division of Gastroenterology and Hepatology, Mayo Clinic College of Medicine, 200 First St. SW, Rochester, MN 55905
| | - CE Bernard
- Developmental Endoscopy Unit and Enteric NeuroScience Program, Division of Gastroenterology and Hepatology, Mayo Clinic College of Medicine, 200 First St. SW, Rochester, MN 55905
| | - M Grover
- Developmental Endoscopy Unit and Enteric NeuroScience Program, Division of Gastroenterology and Hepatology, Mayo Clinic College of Medicine, 200 First St. SW, Rochester, MN 55905
| | - G Farrugia
- Developmental Endoscopy Unit and Enteric NeuroScience Program, Division of Gastroenterology and Hepatology, Mayo Clinic College of Medicine, 200 First St. SW, Rochester, MN 55905
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Kini GC, Biswal SL, Wong MS, Miller CA. Characteristics of spontaneously formed nanoemulsions in octane/AOT/brine systems. J Colloid Interface Sci 2012; 385:111-21. [DOI: 10.1016/j.jcis.2012.07.041] [Citation(s) in RCA: 13] [Impact Index Per Article: 1.1] [Reference Citation Analysis] [What about the content of this article? (0)] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Received: 05/15/2012] [Revised: 07/12/2012] [Accepted: 07/13/2012] [Indexed: 11/15/2022]
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Kovacs JM, Nkolola JP, Peng H, Cheung A, Perry J, Miller CA, Seaman MS, Barouch D, Chen B. HIV-1 envelope trimer elicits higher neutralizing antibody responses than monomeric gp120. Retrovirology 2012. [PMCID: PMC3441467 DOI: 10.1186/1742-4690-9-s2-o62] [Citation(s) in RCA: 2] [Impact Index Per Article: 0.2] [Reference Citation Analysis] [What about the content of this article? (0)] [Track Full Text] [Download PDF] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 12/03/2022] Open
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Abe K, Abgrall N, Ajima Y, Aihara H, Albert JB, Andreopoulos C, Andrieu B, Aoki S, Araoka O, Argyriades J, Ariga A, Ariga T, Assylbekov S, Autiero D, Badertscher A, Barbi M, Barker GJ, Barr G, Bass M, Bay F, Bentham S, Berardi V, Berger BE, Bertram I, Besnier M, Beucher J, Beznosko D, Bhadra S, Blaszczyk FDMM, Blondel A, Bojechko C, Bouchez J, Boyd SB, Bravar A, Bronner C, Brook-Roberge DG, Buchanan N, Budd H, Calvet D, Cartwright SL, Carver A, Castillo R, Catanesi MG, Cazes A, Cervera A, Chavez C, Choi S, Christodoulou G, Coleman J, Coleman W, Collazuol G, Connolly K, Curioni A, Dabrowska A, Danko I, Das R, Davies GS, Davis S, Day M, De Rosa G, de André JPAM, de Perio P, Delbart A, Densham C, Di Lodovico F, Di Luise S, Dinh Tran P, Dobson J, Dore U, Drapier O, Dufour F, Dumarchez J, Dytman S, Dziewiecki M, Dziomba M, Emery S, Ereditato A, Escudero L, Esposito LS, Fechner M, Ferrero A, Finch AJ, Frank E, Fujii Y, Fukuda Y, Galymov V, Gannaway FC, Gaudin A, Gendotti A, George MA, Giffin S, Giganti C, Gilje K, Golan T, Goldhaber M, Gomez-Cadenas JJ, Gonin M, Grant N, Grant A, Gumplinger P, Guzowski P, Haesler A, Haigh MD, Hamano K, Hansen C, Hansen D, Hara T, Harrison PF, Hartfiel B, Hartz M, Haruyama T, Hasegawa T, Hastings NC, Hastings S, Hatzikoutelis A, Hayashi K, Hayato Y, Hearty C, Helmer RL, Henderson R, Higashi N, Hignight J, Hirose E, Holeczek J, Horikawa S, Hyndman A, Ichikawa AK, Ieki K, Ieva M, Iida M, Ikeda M, Ilic J, Imber J, Ishida T, Ishihara C, Ishii T, Ives SJ, Iwasaki M, Iyogi K, Izmaylov A, Jamieson B, Johnson RA, Joo KK, Jover-Manas GV, Jung CK, Kaji H, Kajita T, Kakuno H, Kameda J, Kaneyuki K, Karlen D, Kasami K, Kato I, Kearns E, Khabibullin M, Khanam F, Khotjantsev A, Kielczewska D, Kikawa T, Kim J, Kim JY, Kim SB, Kimura N, Kirby B, Kisiel J, Kitching P, Kobayashi T, Kogan G, Koike S, Konaka A, Kormos LL, Korzenev A, Koseki K, Koshio Y, Kouzuma Y, Kowalik K, Kravtsov V, Kreslo I, Kropp W, Kubo H, Kudenko Y, Kulkarni N, Kurjata R, Kutter T, Lagoda J, Laihem K, Laveder M, Lee KP, Le PT, Levy JM, Licciardi C, Lim IT, Lindner T, Litchfield RP, Litos M, Longhin A, Lopez GD, Loverre PF, Ludovici L, Lux T, Macaire M, Mahn K, Makida Y, Malek M, Manly S, Marchionni A, Marino AD, Marteau J, Martin JF, Maruyama T, Maryon T, Marzec J, Masliah P, Mathie EL, Matsumura C, Matsuoka K, Matveev V, Mavrokoridis K, Mazzucato E, McCauley N, McFarland KS, McGrew C, McLachlan T, Messina M, Metcalf W, Metelko C, Mezzetto M, Mijakowski P, Miller CA, Minamino A, Mineev O, Mine S, Missert AD, Mituka G, Miura M, Mizouchi K, Monfregola L, Moreau F, Morgan B, Moriyama S, Muir A, Murakami A, Murdoch M, Murphy S, Myslik J, Nakadaira T, Nakahata M, Nakai T, Nakajima K, Nakamoto T, Nakamura K, Nakayama S, Nakaya T, Naples D, Navin ML, Nelson B, Nicholls TC, Nishikawa K, Nishino H, Nowak JA, Noy M, Obayashi Y, Ogitsu T, Ohhata H, Okamura T, Okumura K, Okusawa T, Oser SM, Otani M, Owen RA, Oyama Y, Ozaki T, Pac MY, Palladino V, Paolone V, Paul P, Payne D, Pearce GF, Perkin JD, Pettinacci V, Pierre F, Poplawska E, Popov B, Posiadala M, Poutissou JM, Poutissou R, Przewlocki P, Qian W, Raaf JL, Radicioni E, Ratoff PN, Raufer TM, Ravonel M, Raymond M, Retiere F, Robert A, Rodrigues PA, Rondio E, Roney JM, Rossi B, Roth S, Rubbia A, Ruterbories D, Sabouri S, Sacco R, Sakashita K, Sánchez F, Sarrat A, Sasaki K, Scholberg K, Schwehr J, Scott M, Scully DI, Seiya Y, Sekiguchi T, Sekiya H, Shibata M, Shimizu Y, Shiozawa M, Short S, Siyad M, Smith RJ, Smy M, Sobczyk JT, Sobel H, Sorel M, Stahl A, Stamoulis P, Steinmann J, Still B, Stone J, Strabel C, Sulak LR, Sulej R, Sutcliffe P, Suzuki A, Suzuki K, Suzuki S, Suzuki SY, Suzuki Y, Suzuki Y, Szeglowski T, Szeptycka M, Tacik R, Tada M, Takahashi S, Takeda A, Takenaga Y, Takeuchi Y, Tanaka K, Tanaka HA, Tanaka M, Tanaka MM, Tanimoto N, Tashiro K, Taylor I, Terashima A, Terhorst D, Terri R, Thompson LF, Thorley A, Toki W, Tomaru T, Totsuka Y, Touramanis C, Tsukamoto T, Tzanov M, Uchida Y, Ueno K, Vacheret A, Vagins M, Vasseur G, Wachala T, Walding JJ, Waldron AV, Walter CW, Wanderer PJ, Wang J, Ward MA, Ward GP, Wark D, Wascko MO, Weber A, Wendell R, West N, Whitehead LH, Wikström G, Wilkes RJ, Wilking MJ, Wilson JR, Wilson RJ, Wongjirad T, Yamada S, Yamada Y, Yamamoto A, Yamamoto K, Yamanoi Y, Yamaoka H, Yanagisawa C, Yano T, Yen S, Yershov N, Yokoyama M, Zalewska A, Zalipska J, Zambelli L, Zaremba K, Ziembicki M, Zimmerman ED, Zito M, Żmuda J. Indication of electron neutrino appearance from an accelerator-produced off-axis muon neutrino beam. Phys Rev Lett 2011; 107:041801. [PMID: 21866992 DOI: 10.1103/physrevlett.107.041801] [Citation(s) in RCA: 65] [Impact Index Per Article: 5.0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Received: 06/13/2011] [Indexed: 05/31/2023]
Abstract
The T2K experiment observes indications of ν(μ) → ν(e) appearance in data accumulated with 1.43×10(20) protons on target. Six events pass all selection criteria at the far detector. In a three-flavor neutrino oscillation scenario with |Δm(23)(2)| = 2.4×10(-3) eV(2), sin(2)2θ(23) = 1 and sin(2)2θ(13) = 0, the expected number of such events is 1.5±0.3(syst). Under this hypothesis, the probability to observe six or more candidate events is 7×10(-3), equivalent to 2.5σ significance. At 90% C.L., the data are consistent with 0.03(0.04) < sin(2)2θ(13) < 0.28(0.34) for δ(CP) = 0 and a normal (inverted) hierarchy.
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Affiliation(s)
- K Abe
- University of Tokyo, Institute for Cosmic Ray Research, Kamioka Observatory, Kamioka, Japan
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Kayali IH, Liu S, Miller CA. Microemulsions containing mixtures of propoxylated sulfates with slightly branched hydrocarbon chains and cationic surfactants with short hydrophobes or PO chains. Colloids Surf A Physicochem Eng Asp 2010. [DOI: 10.1016/j.colsurfa.2009.07.058] [Citation(s) in RCA: 17] [Impact Index Per Article: 1.2] [Reference Citation Analysis] [What about the content of this article? (0)] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 10/20/2022]
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Airapetian A, Akopov N, Akopov Z, Aschenauer EC, Augustyniak W, Avetissian A, Avetisyan E, Bacchetta A, Ball B, Bianchi N, Blok HP, Böttcher H, Bonomo C, Borissov A, Bryzgalov V, Burns J, Capiluppi M, Capitani GP, Cisbani E, Ciullo G, Contalbrigo M, Dalpiaz PF, Deconinck W, De Leo R, De Nardo L, De Sanctis E, Diefenthaler M, Di Nezza P, Dreschler J, Düren M, Ehrenfried M, Elbakian G, Ellinghaus F, Elschenbroich U, Fabbri R, Fantoni A, Felawka L, Frullani S, Gabbert D, Gapienko G, Gapienko V, Garibaldi F, Gharibyan V, Giordano F, Gliske S, Hadjidakis C, Hartig M, Hasch D, Hill G, Hillenbrand A, Hoek M, Holler Y, Hristova I, Imazu Y, Ivanilov A, Jackson HE, Jo HS, Joosten S, Kaiser R, Keri T, Kinney E, Kisselev A, Korotkov V, Kozlov V, Kravchenko P, Lagamba L, Lamb R, Lapikás L, Lehmann I, Lenisa P, Linden-Levy LA, López Ruiz A, Lorenzon W, Lu XG, Lu XR, Ma BQ, Mahon D, Makins NCR, Manaenkov SI, Manfré L, Mao Y, Marianski B, Martinez de la Ossa A, Marukyan H, Miller CA, Miyachi Y, Movsisyan A, Murray M, Mussgiller A, Nappi E, Naryshkin Y, Nass A, Negodaev M, Nowak WD, Pappalardo LL, Perez-Benito R, Reimer PE, Reolon AR, Riedl C, Rith K, Rosner G, Rostomyan A, Rubin J, Ryckbosch D, Salomatin Y, Sanftl F, Schäfer A, Schnell G, Schüler KP, Seitz B, Shibata TA, Shutov V, Stancari M, Statera M, Steijger JJM, Stenzel H, Stewart J, Stinzing F, Taroian S, Terkulov A, Trzcinski A, Tytgat M, Vandenbroucke A, van der Nat PB, Van Haarlem Y, Van Hulse C, Varanda M, Veretennikov D, Vikhrov V, Vilardi I, Vogel C, Wang S, Yaschenko S, Ye H, Ye Z, Yen S, Yu W, Zeiler D, Zihlmann B, Zupranski P. Observation of the naive-T-odd Sivers effect in deep-inelastic scattering. Phys Rev Lett 2009; 103:152002. [PMID: 19905623 DOI: 10.1103/physrevlett.103.152002] [Citation(s) in RCA: 43] [Impact Index Per Article: 2.9] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Received: 06/23/2009] [Indexed: 05/28/2023]
Abstract
Azimuthal single-spin asymmetries of leptoproduced pions and charged kaons were measured on a transversely polarized hydrogen target. Evidence for a naive-T-odd, transverse-momentum-dependent parton distribution function is deduced from nonvanishing Sivers effects for pi(+), pi(0), and K(+/-), as well as in the difference of the pi(+) and pi(-) cross sections.
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Affiliation(s)
- A Airapetian
- Physikalisches Institut, Universität Giessen, 35392 Giessen, Germany
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Garrett PR, Carr D, Giles D, Pierre-Louis G, Staples E, Miller CA, Chen BH. Solubilisation of triolein by microemulsions containing C12E4/hexadecane/water: Equilibrium and dynamics. J Colloid Interface Sci 2008; 325:508-15. [DOI: 10.1016/j.jcis.2008.06.014] [Citation(s) in RCA: 6] [Impact Index Per Article: 0.4] [Reference Citation Analysis] [What about the content of this article? (0)] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Received: 03/20/2008] [Revised: 06/05/2008] [Accepted: 06/07/2008] [Indexed: 10/21/2022]
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Peña AA, Miller CA. Solubilization rates of oils in surfactant solutions and their relationship to mass transport in emulsions. Adv Colloid Interface Sci 2006; 123-126:241-57. [PMID: 16860285 DOI: 10.1016/j.cis.2006.05.005] [Citation(s) in RCA: 46] [Impact Index Per Article: 2.6] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 10/24/2022]
Abstract
Information on solubilization rates of oils in aqueous micellar solutions is reviewed. For ionic surfactants electrostatic repulsion prevents close approach of micelles to the oil-water interface, so that solubilization results from oil molecules dissolving individually in the solution and being taken up by micelles during and/or after transport across a diffusion boundary layer to the bulk solution. Experiments with SDS solutions and single oil drops having low (but not negligible) solubility indicate that mass transfer is often not rate-controlling. Instead phenomena near the oil-water interface including, but not limited to, the rates of micellar uptake of oil from the aqueous solution seem to control the solubilization rate. In contrast, Ostwald ripening experiments involving multiple oil drops in SDS solutions are often interpreted in terms of molecular dissolution and diffusion alone since ripening rates are typically only slightly different from those observed in the absence of surfactant micelles, where this mechanism is considered to hold. For many nonionic surfactant systems and oils of low or negligible solubility the principal mechanism of solubilization is incorporation of surfactant at the oil-water interface from micelles, which coalesce or "adsorb" at the interface or else dissociate nearby, permitting individual surfactant molecules to be adsorbed. Subsequently the excess surfactant is emitted as oil-containing micelles. Most experiments have indicated that this process, which appears in the analyses as an interfacial resistance, is rate controlling. New results are presented here supporting this model and showing that resistance to mass transfer is often quite low because natural convection can arise near an oil drop owing to the density change produced by solubilized oil in micelles near the drop surface. Provided that polydispersity of drop sizes is properly accounted for, experiments on solubilization and compositional ripening in emulsions stabilized with nonionic surfactants can be interpreted using the interfacial resistance model with values of resistance obtained from single-drop experiments. However, it is unclear whether mass transfer, interfacial resistance or perhaps some combined mechanism controls the rate of Ostwald ripening. One uncertainty limiting predictions of the interfacial resistance model is the lack of information on the oil-to-surfactant ratio in micelles when the concentration of individually dissolved oil molecules slightly exceeds the equilibrium value for a plane oil-water interface, the situation during Ostwald ripening.
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Affiliation(s)
- Alejandro A Peña
- Department of Chemical and Biomolecular Engineering, Rice University, Houston, TX 77005, USA
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Airapetian A, Akopov N, Akopov Z, Amarian M, Andrus A, Aschenauer EC, Augustyniak W, Avakian R, Avetissian A, Avetissian E, Bailey P, Belostotski S, Bianchi N, Blok HP, Böttcher H, Borissov A, Borysenko A, Brüll A, Bryzgalov V, Capiluppi M, Capitani GP, Ciullo G, Contalbrigo M, Dalpiaz PF, Deconinck W, De Leo R, Demey M, De Nardo L, De Sanctis E, Devitsin E, Diefenthaler M, Di Nezza P, Dreschler J, Düren M, Ehrenfried M, Elalaoui-Moulay A, Elbakian G, Ellinghaus F, Elschenbroich U, Fabbri R, Fantoni A, Felawka L, Frullani S, Funel A, Gapienko G, Gapienko V, Garibaldi F, Garrow K, Gavrilov G, Gharibyan V, Giordano F, Grebeniouk O, Gregor IM, Griffioen K, Guler H, Hadjidakis C, Hartig M, Hasch D, Hasegawa T, Hesselink WH, Hillenbrand A, Hoek M, Holler Y, Hommez B, Hristova I, Iarygin G, Ivanilov A, Izotov A, Jackson HE, Jgoun A, Kaiser R, Keri T, Kinney E, Kisselev A, Kobayashi T, Kopytin M, Korotkov V, Kozlov V, Krauss B, Kravchenko P, Krivokhijine VG, Lagamba L, Lapikás L, Lenisa P, Liebing P, Linden-Levy LA, Lorenzon W, Lu J, Lu S, Ma BQ, Maiheu B, Makins NCR, Mao Y, Marianski B, Marukyan H, Masoli F, Mexner V, Meyners N, Michler T, Mikloukho O, Miller CA, Miyachi Y, Muccifora V, Murray M, Nagaitsev A, Nappi E, Naryshkin Y, Negodaev M, Nowak WD, Ohsuga H, Osborne A, Perez-Benito R, Pickert N, Raithel M, Reggiani D, Reimer PE, Reischl A, Roelon AR, Riedl C, Rith K, Rosner G, Rostomyan A, Rubacek L, Rubin J, Ryckbosch D, Salomatin Y, Sanjiev I, Savin I, Schäfer A, Schnell G, Schüler KP, Seele J, Seidl R, Seitz B, Shearer C, Shibata TA, Shutov V, Sinram K, Stancari M, Statera M, Steffens E, Steijger JJM, Stenzel H, Stewart J, Stinzing F, Streit J, Tait P, Tanaka H, Taroian S, Tchuiko B, Terkulov A, Trzcinski A, Tytgat M, Vandenbroucke A, van der Nat PB, van der Steenhoven G, van Haarlem Y, Veretennikov D, Vikhrov V, Vogel C, Wang S, Ye Y, Ye Z, Yen S, Zihlmann B, Zupranski P. Double-hadron leptoproduction in the nuclear medium. Phys Rev Lett 2006; 96:162301. [PMID: 16712217 DOI: 10.1103/physrevlett.96.162301] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Received: 10/11/2005] [Indexed: 05/09/2023]
Abstract
The first measurements of double-hadron production in deep-inelastic scattering within the nuclear medium were made with the HERMES spectrometer at DESY HERA using a 27.6 GeV positron beam. By comparing data for deuterium, nitrogen, krypton, and xenon nuclei, the influence of the nuclear medium on the ratio of double-hadron to single-hadron yields was investigated. Nuclear effects on the additional hadron are clearly observed, but with little or no difference among nitrogen, krypton, or xenon, and with smaller magnitude than effects seen on previously measured single-hadron multiplicities. The data are compared with models based on partonic energy loss or prehadronic scattering and with a model based on a purely absorptive treatment of the final-state interactions. Thus, the double-hadron ratio provides an additional tool for studying modifications of hadronization in nuclear matter.
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Affiliation(s)
- A Airapetian
- Randall Laboratory of Physics, University of Michigan, Ann Arbor, Michigan 48109-1040, USA
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Airapetian A, Akopov N, Akopov Z, Amarian M, Ammosov VV, Andrus A, Aschenauer EC, Augustyniak W, Avakian R, Avetissian A, Avetissian E, Bailey P, Balin D, Baturin V, Beckmann M, Belostotski S, Bernreuther S, Bianchi N, Blok HP, Böttcher H, Borissov A, Borysenko A, Bouwhuis M, Brack J, Brüll A, Bryzgalov V, Capitani GP, Chen T, Chiang HC, Ciullo G, Contalbrigo M, Dalpiaz PF, De Leo R, Demey M, De Nardo L, De Sanctis E, Devitsin E, Di Nezza P, Dreschler J, Düren M, Ehrenfried M, Elalaoui-Moulay A, Elbakian G, Ellinghaus F, Elschenbroich U, Fabbri R, Fantoni A, Fechtchenko A, Felawka L, Fox B, Frullani S, Gapienko G, Gapienko V, Garibaldi F, Garrow K, Garutti E, Gaskell D, Gavrilov G, Gharibyan V, Graw G, Grebeniouk O, Greeniaus LG, Gregor IM, Hafidi K, Hartig M, Hasch D, Heesbeen D, Henoch M, Hertenberger R, Hesselink WHA, Hillenbrand A, Hoek M, Holler Y, Hommez B, Iarygin G, Ivanilov A, Izotov A, Jackson HE, Jgoun A, Kaiser R, Kinney E, Kisselev A, Kopytin M, Korotkov V, Kozlov V, Krauss B, Krivokhijine VG, Lagamba L, Lapikás L, Laziev A, Lenisa P, Liebing P, Linden-Levy LA, Lipka K, Lorenzon W, Lu H, Lu J, Lu S, Ma BQ, Maiheu B, Makins NCR, Mao Y, Marianski B, Marukyan H, Masoli F, Mexner V, Meyners N, Mikloukho O, Miller CA, Miyachi Y, Muccifora V, Nagaitsev A, Nappi E, Naryshkin Y, Nass A, Negodaev M, Nowak WD, Oganessyan K, Ohsuga H, Pickert N, Potashov S, Potterveld DH, Raithel M, Reggiani D, Reimer PE, Reischl A, Reolon AR, Riedl C, Rith K, Rosner G, Rostomyan A, Rubacek L, Rubin J, Ryckbosch D, Salomatin Y, Sanjiev I, Savin I, Schäfer A, Schill C, Schnell G, Schüler KP, Seele J, Seidl R, Seitz B, Shanidze R, Shearer C, Shibata TA, Shutov V, Simani MC, Sinram K, Stancari M, Statera M, Steffens E, Steijger JJM, Stenzel H, Stewart J, Stinzing F, Stösslein U, Tait P, Tanaka H, Taroian S, Tchuiko B, Terkulov A, Tkabladze A, Trzcinski A, Tytgat M, Vandenbroucke A, van der Nat PB, van der Steenhoven G, Vetterli MC, Vikhrov V, Vincter MG, Vogel C, Vogt M, Volmer J, Weiskopf C, Wendland J, Wilbert J, Ye Y, Ye Z, Yen S, Zihlmann B, Zupranski P. Measurement of the tensor structure function b1 of the deuteron. Phys Rev Lett 2005; 95:242001. [PMID: 16384369 DOI: 10.1103/physrevlett.95.242001] [Citation(s) in RCA: 1] [Impact Index Per Article: 0.1] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Received: 06/08/2005] [Indexed: 05/05/2023]
Abstract
The Hermes experiment has investigated the tensor spin structure of the deuteron using the 27.6 GeV/c positron beam of DESY HERA. The use of a tensor-polarized deuteron gas target with only a negligible residual vector polarization enabled the first measurement of the tensor asymmetry A(d)zz and the tensor structure function b(d)1 for average values of the Bjorken variable 0.01< <x> <0.45 and of the negative of the squared four-momentum transfer 0.5 GeV2 < <Q2> <5 GeV2. The quantities A(d)zz and b(d)1 are found to be nonzero. The rise of b(d)1 for decreasing values of x can be interpreted to originate from the same mechanism that leads to nuclear shadowing in unpolarized scattering.
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Affiliation(s)
- A Airapetian
- Yerevan Physics Institute, 375036 Yerevan, Armenia
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Roberson ED, Hesse JH, Rose KD, Slama H, Johnson JK, Yaffe K, Forman MS, Miller CA, Trojanowski JQ, Kramer JH, Miller BL. Frontotemporal dementia progresses to death faster than Alzheimer disease. Neurology 2005; 65:719-25. [PMID: 16157905 DOI: 10.1212/01.wnl.0000173837.82820.9f] [Citation(s) in RCA: 157] [Impact Index Per Article: 8.3] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [MESH Headings] [Grants] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/15/2022] Open
Abstract
BACKGROUND Frontotemporal lobar degeneration (FTLD) is a common cause of non-Alzheimer dementia, but its natural history and the factors related to mortality in affected patients are not well understood. METHODS This retrospective, longitudinal study compared survival in FTLD (n = 177) with Alzheimer disease (AD; n = 395). Hazards analysis investigated the contribution of various demographic, neuropsychiatric, and neuropsychological variables and associated neurologic and neuropathologic findings. RESULTS The frontotemporal dementia (FTD) subtype of FTLD progressed faster than AD (median survival from retrospectively determined symptom onset, 8.7 +/- 1.2 vs 11.8 +/- 0.6 years, p < 0.0001; median survival from initial clinic presentation, 3.0 +/- 0.5 vs 5.7 +/- 0.1 years, p < 0.0001). Survival was similarly reduced in the related conditions corticobasal degeneration and progressive supranuclear palsy. Survival in the semantic dementia subtype of FTLD (11.9 +/- 0.2 years from onset and 5.3 +/- 0.4 years from presentation), however, was significantly longer than in FTD and did not differ from AD. Hazards analysis to determine factors affecting survival in FTLD showed no effect of age at onset, sex, education, family history, or neuropsychiatric profile. Among neuropsychological measures examined, impaired letter fluency had a significant association with reduced survival. Associated ALS significantly reduced survival in FTLD. The presence of tau-positive inclusions was associated with the slowest progression. CONCLUSIONS Frontotemporal lobar degeneration progresses more rapidly than Alzheimer disease, and the fastest-progressing cases are those with the frontotemporal dementia clinical subtype, coexisting motor neuron disease, or tau-negative neuropathology.
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Affiliation(s)
- E D Roberson
- Memory and Aging Center, Department of Neurology, University of California, San Francisco, CA, USA.
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Airapetian A, Akopov N, Akopov Z, Amarian M, Andrus A, Aschenauer EC, Augustyniak W, Avakian R, Avetissian A, Avetissian E, Bacchetta A, Bailey P, Balin D, Beckmann M, Belostotski S, Bianchi N, Blok HP, Böttcher H, Borissov A, Borysenko A, Bouwhuis M, Brüll A, Bryzgalov V, Capitani GP, Cappiluppi M, Chen T, Ciullo G, Contalbrigo M, Dalpiaz PF, Leo RD, Demey M, Nardo LD, Sanctis ED, Devitsin E, Nezza PD, Düren M, Ehrenfried M, Elalaoui-Moulay A, Elbakian G, Ellinghaus F, Elschenbroich U, Fabbri R, Fantoni A, Fechtchenko A, Felawka L, Frullani S, Gapienko G, Gapienko V, Garibaldi F, Garrow K, Gavrilov G, Gharibyan V, Grebeniouk O, Gregor IM, Hadjidakis C, Hafidi K, Hartig M, Hasch D, Henoch M, Hesselink WHA, Hillenbrand A, Hoek M, Holler Y, Hommez B, Hristova I, Iarygin G, Ilyichev A, Ivanilov A, Izotov A, Jackson HE, Jgoun A, Kaiser R, Kinney E, Kisselev A, Kobayashi T, Kopytin M, Korotkov V, Kozlov V, Krauss B, Krivokhijine VG, Lagamba L, Lapikás L, Laziev A, Lenisa P, Liebing P, Linden-Levy LA, Lorenzon W, Lu H, Lu J, Lu S, Ma BQ, Maiheu B, Makins NCR, Mao Y, Marianski B, Marukyan H, Masoli F, Mexner V, Meyners N, Michler T, Mikloukho O, Miller CA, Miyachi Y, Muccifora V, Nagaitsev A, Nappi E, Naryshkin Y, Nass A, Negodaev M, Nowak WD, Oganessyan K, Ohsuga H, Osborne A, Pickert N, Potterveld DH, Raithel M, Reggiani D, Reimer PE, Reischl A, Reolon AR, Riedl C, Rith K, Rosner G, Rostomyan A, Rubacek L, Rubin J, Ryckbosch D, Salomatin Y, Sanjiev I, Savin I, Schäfer A, Schill C, Schnell G, Schüler KP, Seele J, Seidl R, Seitz B, Shanidze R, Shearer C, Shibata TA, Shutov V, Sinram K, Sommer W, Stancari M, Statera M, Steffens E, Steijger JJM, Stenzel H, Stewart J, Stinzing F, Tait P, Tanaka H, Taroian S, Tchuiko B, Terkulov A, Trzcinski A, Tytgat M, Vandenbroucke A, van der Nat PB, van der Steenhoven G, van Haarlem Y, Vetterli MC, Vikhrov V, Vincter MG, Vogel C, Volmer J, Wang S, Wendland J, Wilbert J, Smit GY, Ye Y, Ye Z, Yen S, Zihlmann B, Zupranski P. Single-spin asymmetries in semi-inclusive deep-inelastic scattering on a transversely polarized hydrogen target. Phys Rev Lett 2005; 94:012002. [PMID: 15698069 DOI: 10.1103/physrevlett.94.012002] [Citation(s) in RCA: 61] [Impact Index Per Article: 3.2] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Received: 08/06/2004] [Indexed: 05/24/2023]
Abstract
Single-spin asymmetries for semi-inclusive electroproduction of charged pions in deep-inelastic scattering of positrons are measured for the first time with transverse target polarization. The asymmetry depends on the azimuthal angles of both the pion (phi) and the target spin axis (phi(S)) about the virtual-photon direction and relative to the lepton scattering plane. The extracted Fourier component sin((phi+phi(S))(pi)(UT) is a signal of the previously unmeasured quark transversity distribution, in conjunction with the Collins fragmentation function, also unknown. The component sin((phi-phi(S)(pi)(UT) arises from a correlation between the transverse polarization of the target nucleon and the intrinsic transverse momentum of quarks, as represented by the previously unmeasured Sivers distribution function. Evidence for both signals is observed, but the Sivers asymmetry may be affected by exclusive vector meson production.
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Affiliation(s)
- A Airapetian
- Randall Laboratory of Physics, University of Michigan, Ann Arbor, MI 48109-1120, USA
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Zhang H, Miller CA, Garrett PR, Raney KH. Lauryl alcohol and amine oxide as foam stabilizers in the presence of hardness and oily soil. J SURFACTANTS DETERG 2005. [DOI: 10.1007/s11743-005-0337-3] [Citation(s) in RCA: 29] [Impact Index Per Article: 1.5] [Reference Citation Analysis] [What about the content of this article? (0)] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/30/2022]
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Abstract
The effect of calcium oleate on foam stability was studied for aqueous solutions of two commonly used surfactants (anionic and nonionic) under alkaline conditions in the absence of oil. For the anionic surfactant, defoaming by calcium oleate appears to involve two mechanisms. One is that oleate and calcium ions are presumably incorporated into the surfactant monolayers with a resulting decrease in the maximum of the disjoining pressure curve and therefore produces less stable thin films. The other is bridging of the films by calcium oleate particles. The latter mechanism was especially important in freshly made solutions where precipitation in the aqueous phase was still occurring when the foam was generated. Foams generated after aging (hours) when precipitation was nearly complete were more stable even though solution turbidities were greater. Foams of the nonionic surfactant were less stable than those of the anionic surfactant but were also destabilized by sufficient amounts of calcium oleate and exhibited a similar aging effect. A simplified model was developed for estimating the sodium oleate concentration at which precipitation commences in solutions of the anionic surfactant containing dissolved calcium. It includes enhancement of calcium content in the electrical double layers of the surfactant micelles. Predictions of the model were in agreement with experiment.
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Affiliation(s)
- Hui Zhang
- Department of Chemical Engineering, Rice University, Houston, TX 77251-1892, USA
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Affiliation(s)
- Alejandro A. Peña
- Department of Chemical Engineering, Rice University, 6100 Main Street, MS 362, Houston, Texas 77005
| | - George J. Hirasaki
- Department of Chemical Engineering, Rice University, 6100 Main Street, MS 362, Houston, Texas 77005
| | - Clarence A. Miller
- Department of Chemical Engineering, Rice University, 6100 Main Street, MS 362, Houston, Texas 77005
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Abstract
Emissions of sulfur trioxide (SO3) are a key component of plume opacity and acid deposition. Consequently, these emissions need to be low enough to not cause opacity violations and acid deposition. Generally, a small fraction of sulfur (S) in coal is converted to SO3 in coal-fired combustion devices such as electric utility boilers. The emissions of SO3 from such a boiler depend on coal S content, combustion conditions, flue gas characteristics, and air pollution devices being used. It is well known that the catalyst used in the selective catalytic reduction (SCR) technology for nitrogen oxides control oxidizes a small fraction of sulfur dioxide in the flue gas to SO3. The extent of this oxidation depends on the catalyst formulation and SCR operating conditions. Gas-phase SO3 and sulfuric acid, on being quenched in plant equipment (e.g., air preheater and wet scrubber), result in fine acidic mist, which can cause increased plume opacity and undesirable emissions. Recently, such effects have been observed at plants firing high-S coal and equipped with SCR systems and wet scrubbers. This paper investigates the factors that affect acidic mist production in coal-fired electric utility boilers and discusses approaches for mitigating emission of this mist.
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Affiliation(s)
- R K Srivastava
- Office of Research and Development, National Risk Management Research Laboratory, Air Pollution Prevention and Control Division, US Environmental Protection Agency, Research Triangle Park, North Carolina 27711, USA.
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Airapetian A, Akopov N, Akopov Z, Amarian M, Ammosov VV, Andrus A, Aschenauer EC, Augustyniak W, Avakian R, Avetissian A, Avetissian E, Bailey P, Baturin V, Baumgarten C, Beckmann M, Belostotski S, Bernreuther S, Bianchi N, Blok HP, Böttcher H, Borissov A, Bouwhuis M, Brack J, Brüll A, Bryzgalov V, Capitani GP, Chiang HC, Ciullo G, Contalbrigo M, Dalpiaz PF, De Leo R, De Nardo L, De Sanctis E, Devitsin E, Di Nezza P, Düren M, Ehrenfried M, Elalaoui-Moulay A, Elbakian G, Ellinghaus F, Elschenbroich U, Ely J, Fabbri R, Fantoni A, Fechtchenko A, Felawka L, Fox B, Franz J, Frullani S, Gärber Y, Gapienko G, Gapienko V, Garibaldi F, Garrow K, Garutti E, Gaskell D, Gavrilov G, Gharibyan V, Graw G, Grebeniouk O, Greeniaus LG, Hafidi K, Hartig M, Hasch D, Heesbeen D, Henoch M, Hertenberger R, Hesselink WHA, Hillenbrand A, Hoek M, Holler Y, Hommez B, Iarygin G, Ivanilov A, Izotov A, Jackson HE, Jgoun A, Kaiser R, Kinney E, Kisselev A, Königsmann K, Kopytin M, Korotkov V, Kozlov V, Krauss B, Krivokhijine VG, Lagamba L, Lapikás L, Laziev A, Lenisa P, Liebing P, Lindemann T, Lipka K, Lorenzon W, Lu J, Maiheu B, Makins NCR, Marianski B, Marukyan H, Masoli F, Mexner V, Meyners N, Mikloukho O, Miller CA, Miyachi Y, Muccifora V, Nagaitsev A, Nappi E, Naryshkin Y, Nass A, Negodaev M, Nowak WD, Oganessyan K, Ohsuga H, Orlandi G, Pickert N, Potashov S, Potterveld DH, Raithel M, Reggiani D, Reimer PE, Reischl A, Reolon AR, Riedl C, Rith K, Rosner G, Rostomyan A, Rubacek L, Ryckbosch D, Salomatin Y, Sanjiev I, Savin I, Scarlett C, Schäfer A, Schill C, Schnell G, Schüler KP, Schwind A, Seele J, Seidl R, Seitz B, Shanidze R, Shearer C, Shibata TA, Shutov V, Simani MC, Sinram K, Stancari M, Statera M, Steffens E, Steijger JJM, Stewart J, Stösslein U, Tait P, Tanaka H, Taroian S, Tchuiko B, Terkulov A, Tkabladze A, Trzcinski A, Tytgat M, Vandenbroucke A, Van Der Nat P, Van Der Steenhoven G, Vetterli MC, Vikhrov V, Vincter MG, Visser J, Vogel C, Vogt M, Volmer J, Weiskopf C, Wendland J, Wilbert J, Ybeles Smit G, Yen S, Zihlmann B, Zohrabian H, Zupranski P. Flavor decomposition of the sea-quark helicity distributions in the nucleon from semiinclusive deep inelastic scattering. Phys Rev Lett 2004; 92:012005. [PMID: 14753985 DOI: 10.1103/physrevlett.92.012005] [Citation(s) in RCA: 6] [Impact Index Per Article: 0.3] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Received: 07/25/2003] [Indexed: 05/24/2023]
Abstract
Double-spin asymmetries of semiinclusive cross sections for the production of identified pions and kaons have been measured in deep inelastic scattering of polarized positrons on a polarized deuterium target. Five helicity distributions including those for three sea quark flavors were extracted from these data together with reanalyzed previous data for identified pions from a hydrogen target. These distributions are consistent with zero for all three sea flavors. A recently predicted flavor asymmetry in the polarization of the light quark sea appears to be disfavored by the data.
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Affiliation(s)
- A Airapetian
- Yerevan Physics Institute, 375036 Yerevan, Armenia
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Hurrell-Gillingham K, Reaney IM, Miller CA, Crawford A, Hatton PV. Devitrification of ionomer glass and its effect on the in vitro biocompatibility of glass-ionomer cements. Biomaterials 2003; 24:3153-60. [PMID: 12895588 DOI: 10.1016/s0142-9612(03)00124-8] [Citation(s) in RCA: 25] [Impact Index Per Article: 1.2] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [MESH Headings] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/30/2022]
Abstract
The effects of devitrification of an ionomer glass with a molar composition 4.5SiO(2).3Al(2)O(3).1.5P(2)O(5).3CaO.2CaF(2) on cement formation and in vitro biocompatibility were investigated. Differential thermal analysis was used to study the phase evolution in the glass, and to determine the heat treatments for production of glass-ceramics. X-ray diffraction patterns from glass frit heat-treated at 750 degrees C for 2h contained peaks corresponding to apatite (JCPDS 15-876), whereas for samples heat-treated at 950 degrees C for 2h apatite and mullite (JCPDS 15-776) were the major phases detected. Transmission electron microscopy (TEM) confirmed that apatite and apatite-mullite phases were present after heat treatments at 750 degrees C and 950 degrees C respectively. Glass and glass-ceramics were ground to prepare <45microm powders and glass ionomer cements were produced using a ratio of 1g powder: 0.2g PAA: 0.3g 10% m/v tartaric acid solution in water. In vitro biocompatibility was evaluated using cultured rat osteosarcoma (ROS) cells. Scanning electron microscopy (SEM) showed that cells colonised the surfaces of cements prepared using untreated ionomer glass and glass crystallised to form apatite (750 degrees C/2h). However, quantitative evaluation using MTT and total protein assays indicated that more cell growth occurred in the presence of cements prepared using ionomer glasses crystallised to apatite than cements prepared using untreated glass. The least cell growth and respiratory activity was observed on cements made with crystallised glass containing both apatite and mullite. It was concluded that the controlled devitrification of ionomer glasses could be used to produce GIC bone cements with improved biocompatibility.
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Affiliation(s)
- K Hurrell-Gillingham
- Department of Engineering Materials, Sir Robert Hadfield Building, University of Sheffield, Sheffield S1 3JD, UK
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Abstract
The effect of oils, hardness, and calcium soap on foam stability of aqueous solutions of commercial surfactants was investigated. For conditions where negligible calcium soap was formed, stability of foams made with 0.1 wt% solutions of a seven-EO alcohol ethoxylate containing dispersed drops of n-hexadecane, triolein, or mixtures of these oils with small amounts of oleic acid could be understood in terms of entry, spreading, and bridging coefficients, i.e., ESB analysis. However, foams made from solutions containing 0.01 wt% of three-EO alcohol ethoxysulfate sodium salt and the same dispersed oils were frequently more stable than expected based on ESB analysis, reflecting that repulsion due to overlap of electrical double layers in the asymmetric oil-water-air film made oil entry into the air-water interface more difficult than the theory predicts. When calcium soap was formed in situ by the reaction of fatty acids in the oil with calcium, solid soap particles were observed at the surfaces of the oil drops. The combination of oil and calcium soap produced a synergistic effect facilitating the well-known bridging instability of foam films or Plateau borders and producing a substantial defoaming effect. A possible mechanism of instability involving increases in disjoining pressure at locations where small soap particles approach the air-water interface is discussed. For both surfactants with the triolein-oleic acid mixtures, calculated entry and bridging coefficients for conditions when calcium soap formed were positive shortly after foam generation but negative at equilibrium. These results are consistent with the experimental observation that most defoaming action occurred shortly after foam generation rather than at later times.
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Affiliation(s)
- Hui Zhang
- Department of Chemical Engineering, Rice University, Houston, TX 77251-1892, USA
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