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Caldwell R, Cui Y, Guo HK, Mandic V, Mariotti A, No JM, Ramsey-Musolf MJ, Sakellariadou M, Sinha K, Wang LT, White G, Zhao Y, An H, Bian L, Caprini C, Clesse S, Cline JM, Cusin G, Fornal B, Jinno R, Laurent B, Levi N, Lyu KF, Martinez M, Miller AL, Redigolo D, Scarlata C, Sevrin A, Haghi BSE, Shu J, Siemens X, Steer DA, Sundrum R, Tamarit C, Weir DJ, Xie KP, Yang FW, Zhou S. Detection of early-universe gravitational-wave signatures and fundamental physics. Gen Relativ Gravit 2022; 54:156. [PMID: 36465478 PMCID: PMC9712380 DOI: 10.1007/s10714-022-03027-x] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Key Words] [Grants] [Track Full Text] [Figures] [Subscribe] [Scholar Register] [Received: 04/23/2022] [Accepted: 10/20/2022] [Indexed: 06/17/2023]
Abstract
Detection of a gravitational-wave signal of non-astrophysical origin would be a landmark discovery, potentially providing a significant clue to some of our most basic, big-picture scientific questions about the Universe. In this white paper, we survey the leading early-Universe mechanisms that may produce a detectable signal-including inflation, phase transitions, topological defects, as well as primordial black holes-and highlight the connections to fundamental physics. We review the complementarity with collider searches for new physics, and multimessenger probes of the large-scale structure of the Universe.
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Affiliation(s)
- Robert Caldwell
- Department of Physics and Astronomy, Dartmouth College, Hanover, NH 03755 USA
| | - Yanou Cui
- Department of Physics and Astronomy, University of California, Riverside, CA 92521 USA
| | - Huai-Ke Guo
- Department of Physics and Astronomy, University of Utah, Salt Lake City, UT 84112 USA
| | - Vuk Mandic
- School of Physics and Astronomy, University of Minnesota, Minneapolis, MN 55455 USA
| | - Alberto Mariotti
- Theoretische Natuurkunde and IIHE/ELEM, Vrije Universiteit Brussel, and International Solvay Institutes, Pleinlaan 2, 1050 Brussels, Belgium
| | - Jose Miguel No
- Instituto de Física Teórica UAM/CSIC, C/ Nicolás Cabrera 13- 15, Campus de Cantoblanco, 28049 Madrid, Spain
| | - Michael J. Ramsey-Musolf
- Tsung Dao Lee Institute/Shanghai Jiao Tong University, Shanghai, 200120 People’s Republic of China
- University of Massachusetts, Amherst, MA 01003 USA
| | | | - Kuver Sinha
- Department of Physics and Astronomy, University of Oklahoma, Norman, OK 73019 USA
| | - Lian-Tao Wang
- Department of Physics, University of Chicago, Chicago, IL 60637 USA
| | - Graham White
- Kavli IPMU (WPI), UTIAS, The University of Tokyo, Kashiwa, Chiba 277-8583 Japan
| | - Yue Zhao
- Department of Physics and Astronomy, University of Utah, Salt Lake City, UT 84112 USA
| | - Haipeng An
- Department of Physics, Tsinghua University, Beijing, 100084 People’s Republic of China
- Center for High Energy Physics, Tsinghua University, Beijing, 100084 People’s Republic of China
- Center for High Energy Physics, Peking University, Beijing, 100871 People’s Republic of China
| | - Ligong Bian
- Center for High Energy Physics, Peking University, Beijing, 100871 People’s Republic of China
- Department of Physics and Chongqing Key Laboratory for Strongly Coupled Physics, Chongqing University, Chongqing, 401331 People’s Republic of China
| | - Chiara Caprini
- Theoretical Physics Department, University of Geneva, 1211 Geneva, Switzerland
- CERN, Theoretical Physics Department, 1 Esplanade des Particules, 1211 Genève 23, Switzerland
| | - Sebastien Clesse
- Service de Physique Théorique (CP225), University of Brussels (ULB), Boulevard du Triomphe, 1050 Brussels, Belgium
| | - James M. Cline
- Department of Physics, McGill University, Montréal, QC H3A2T8 Canada
| | - Giulia Cusin
- Theoretical Physics Department, University of Geneva, 1211 Geneva, Switzerland
- Sorbonne Université, CNRS, UMR 7095, Institut d’Astrophysique de Paris, 75014 Paris, France
| | - Bartosz Fornal
- Department of Chemistry and Physics, Barry University, Miami Shores, FL 33161 USA
| | - Ryusuke Jinno
- Instituto de Física Teórica UAM/CSIC, C/ Nicolás Cabrera 13- 15, Campus de Cantoblanco, 28049 Madrid, Spain
| | - Benoit Laurent
- Department of Physics, McGill University, Montréal, QC H3A2T8 Canada
| | - Noam Levi
- Raymond and Beverly Sackler School of Physics and Astronomy, Tel-Aviv University, Tel-Aviv, 69978 Israel
| | - Kun-Feng Lyu
- School of Physics and Astronomy, University of Minnesota, Minneapolis, MN 55455 USA
| | - Mario Martinez
- Institut de Física d’Altes Energies, Barcelona Institute of Science and Technology and ICREA, 08193 Barcelona, Spain
| | - Andrew L. Miller
- Université catholique de Louvain, 1348 Louvain-la-Neuve, Belgium
| | - Diego Redigolo
- INFN, Sezione di Firenze Via G. Sansone 1, 50019 Sesto Fiorentino, Italy
| | - Claudia Scarlata
- School of Physics and Astronomy, University of Minnesota, Minneapolis, MN 55455 USA
| | - Alexander Sevrin
- Theoretische Natuurkunde and IIHE/ELEM, Vrije Universiteit Brussel, and International Solvay Institutes, Pleinlaan 2, 1050 Brussels, Belgium
| | - Barmak Shams Es Haghi
- Department of Physics and Astronomy, University of Utah, Salt Lake City, UT 84112 USA
| | - Jing Shu
- CAS Key Laboratory of Theoretical Physics, Insitute of Theoretical Physics, Chinese Academy of Sciences, Beijing, 100190 People’s Republic of China
- School of Physical Sciences, University of Chinese Academy of Sciences, Beijing, 100049 People’s Republic of China
- School of Fundamental Physics and Mathematical Sciences, Hangzhou Institute for Advanced Study, University of Chinese Academy of Sciences, Hangzhou, 310024 People’s Republic of China
- International Center for Theoretical Physics Asia-Pacific, Beijing, Hanzhou, People’s Republic of China
| | - Xavier Siemens
- Department of Physics, Oregon State University, Corvallis, OR 97331 USA
| | - Danièle A. Steer
- Laboratoire Astroparticule et Cosmologie, CNRS, Université Paris Cité, 75013 Paris, France
| | | | - Carlos Tamarit
- Physik-Department T70, Technische Universität München, James-Franck-Straße, 85748 Garching, Germany
| | - David J. Weir
- Department of Physics and Helsinki Institute of Physics, University of Helsinki, P.O. Box 64, 00014 Helsinki, Finland
| | - Ke-Pan Xie
- Department of Physics and Astronomy, University of Nebraska, Lincoln, NE 68588 USA
| | - Feng-Wei Yang
- Department of Physics and Astronomy, University of Utah, Salt Lake City, UT 84112 USA
| | - Siyi Zhou
- Department of Physics, Kobe University, Kobe, 657-8501 Japan
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Romero A, Martinovic K, Callister TA, Guo HK, Martínez M, Sakellariadou M, Yang FW, Zhao Y. Implications for First-Order Cosmological Phase Transitions from the Third LIGO-Virgo Observing Run. Phys Rev Lett 2021; 126:151301. [PMID: 33929242 DOI: 10.1103/physrevlett.126.151301] [Citation(s) in RCA: 2] [Impact Index Per Article: 0.7] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Received: 01/14/2021] [Accepted: 03/23/2021] [Indexed: 06/12/2023]
Abstract
We place constraints on the normalized energy density in gravitational waves from first-order strong phase transitions using data from Advanced LIGO and Virgo's first, second, and third observing runs. First, adopting a broken power law model, we place 95% confidence level upper limits simultaneously on the gravitational-wave energy density at 25 Hz from unresolved compact binary mergers, Ω_{CBC}<6.1×10^{-9}, and strong first-order phase transitions, Ω_{BPL}<4.4×10^{-9}. The inclusion of the former is necessary since we expect this astrophysical signal to be the foreground of any detected spectrum. We then consider two more complex phenomenological models, limiting at 25 Hz the gravitational-wave background due to bubble collisions to Ω_{pt}<5.0×10^{-9} and the background due to sound waves to Ω_{pt}<5.8×10^{-9} at 95% confidence level for phase transitions occurring at temperatures above 10^{8} GeV.
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Affiliation(s)
- Alba Romero
- Institut de Física d'Altes Energies (IFAE), Barcelona Institute of Science and Technology, E-08193 Barcelona, Spain
| | - Katarina Martinovic
- Theoretical Particle Physics and Cosmology Group, Physics Department, King's College London, University of London, Strand, London WC2R 2LS, United Kingdom
| | - Thomas A Callister
- Center for Computational Astrophysics, Flatiron Institute, New York, New York 10010, USA
| | - Huai-Ke Guo
- Department of Physics and Astronomy, University of Oklahoma, Norman, Oklahoma 73019, USA
| | - Mario Martínez
- Institut de Física d'Altes Energies (IFAE), Barcelona Institute of Science and Technology, E-08193 Barcelona, Spain
- Catalan Institution for Research and Advanced Studies (ICREA), E-08010 Barcelona, Spain
| | - Mairi Sakellariadou
- Theoretical Particle Physics and Cosmology Group, Physics Department, King's College London, University of London, Strand, London WC2R 2LS, United Kingdom
- Theoretical Physics Department, CERN, 1211 Geneva 23, Switzerland
| | - Feng-Wei Yang
- Department of Physics and Astronomy, University of Utah, Salt Lake City, Utah 84112, USA
| | - Yue Zhao
- Department of Physics and Astronomy, University of Utah, Salt Lake City, Utah 84112, USA
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Feng K, Guo HK, Zhang YL, Wu Z. [Visual quality comparison after multifocal toric intraocular lens or monofocal toric intraocular lens implantation]. Zhonghua Yan Ke Za Zhi 2017; 53:274-280. [PMID: 28412800 DOI: 10.3760/cma.j.issn.0412-4081.2017.04.009] [Citation(s) in RCA: 2] [Impact Index Per Article: 0.3] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Key Words] [Subscribe] [Scholar Register] [Indexed: 11/05/2022]
Abstract
Objective: To compare visual quality and satisfaction after multifocal toric intraocular lens (Acrysof IQ Restor toric, ART) and monofocal toric intraocular lens implantation in patients. Methods: It was a prospective nonrandomized Phase Ⅲ clinical trial. Patients with age-related cataract and corneal astigmatism were enrolled and accepted phacoemulsification combined with implantation of intraocular lens (IOL) in Henan Provincial Eye Hospital during March 2013 to December 2014. Fifty-six cases were divided into two groups according to which IOL they chose. ART group included 28 cases (3l eyes) aged from 41.0 to 72.0 years, with an average age of 61.5 years; toric group included 28 cases (33 eyes) aged from 42.0 to 75.0 years, with an average age of 63.5 years. Three months postoperatively, uncorrected distance visual acuity (UDVA) at 5, 70, 40 cm, corrected distance, intermediate, and near visual acuities, defocus curve, residual refractive astigmatism, rotational stability of the IOL, contrast sensitivity and patientsatisfaction were evaluated. All data were processed by statistic package deal SPSS 16.0. Postoperative visual acuity, residual astigmatism, IOL axial rotation and contrast sensitivity were compared by independent samples t test; preoperative and postoperative corneal astigmatism were compared by paired t-test; spectacle independency and halo incidence were processed by χ(2) test; visual satisfaction score was analyzed by Mann-Whitney test. Results: At 3 months postoperatively, in ART group, UDVA was (0.04±0.05), UIVA was (0.24±0.15), UNVA was (0.20±0.24). While in Toric group, UDVA was (0.06±0.04), UIVA was (0.30±0.13), UNVA was (0.47±0.21). There was no significant difference in UDVA between two groups(t=0.79, P=0.433). But in ART group, UIVA and UNVA were markedly better than those in Toric group(t=2.74, P=0.008; t=3.45, P<0.01). Depth of focus was 5.50 D (+2.00--3.50 D) in the ART group and 2.50 D (+1.00--1.50 D) in the Toric group. Average postoperative residual astigmatism was (-0.45±0.41)D in ART group and (-0.41±0.32)D in the Toric group. There was no significant difference between two groups (t=1.05, P=0.304). Average IOL rotation test was (2.95°±1.34°) in the ART group and (2.75°±1.64°) in the Toric group. There was no significant difference between two groups (t=0.67, P=0.452). Spectacle independency was achieved by 85.7% of patients in the ART group and 32.1% in the Toric group. There was no signifcant difference in distant visual satisfaction scores between the two groups(Z=0.71, P>0.05), while the intermediate and near visual satisfaction scores were significantly different(Z=2.27, P<0.05; Z=2.60, P<0.05) Conclusions: Both of the ART IOL and toric IOL can correct patients astigmatism. Implantation of ART IOL in patients with cataract and corneal astigmatism provided excellent distance, intermediate, and near visual outcomes. It provided better predictability of the refractive results, nice rotational stability, and good optical performance. At the same time, it improved the spectacle independency of cataract patients with astigmatism. (Chin J Ophthalmol, 2017, 53: 274-280).
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Affiliation(s)
- K Feng
- Henan Eye Hospital, Zhengzhou 450000, China
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