[Non-A Non-B Aortic Dissection Complicated with Right Aortic Arch Treated by Extended Thoracic Aortic Repair]

A 44-year old man with a history of Stanford type B acute aortic dissection was admitted for the treatment of acute aortic dissection. Computed tomography( CT) scan showed a descending entry-type non-A non-B aortic dissection with a maximum diameter of 65 mm occurring in a patient with Edwards typeⅢ right aortic arch whose left subclavian artery was obliterated. The patient was initially treated conservatively and underwent one-stage extended aortic repair from the ascending aorta to the descending thoracic aorta via median sternotomy 22 days after the symptom onset. Although the patient suffered from right empyema postoperatively, he was discharged from the hospital on postoperative day 64 after 4 weeks antibiotics therapy. The patient was also complicated by right recurrent nerve palsy, hoarseness improved over the 8 months after surgery.

Design improvement of the conversion mechanism from balloon inflation to bending motion for inflatable film actuators

Various soft actuators have been investigated to overcome the drawbacks of conventional solid machines and explore the applications of soft robotics. In particular, and because they are expected to be applicable in minimally invasive medicine because of their safety, soft inflatable microactuators using an actuation conversion mechanism from balloon inflation to bending motion have been proposed for high-output bending motion. These microactuators could be applied to create an operation space by safely moving organs and tissues; however, the conversion efficiency could be further improved. This study aimed to improve conversion efficiency by investigating the design of the conversion mechanism. The contact conditions between the inflated balloon and conversion film were examined to improve the contact area for force transmission, with the contact area dependent on the length of the contact arc between the balloon and force conversion mechanism and on the amount of balloon deformation. In addition, surface contact friction between the balloon and film, which affects actuator performance, was also investigated. The generated force of the improved device is 1.21 N at 80 kPa when it bends 10 mm, which is 2.2 times the generated force of the previous design. This improved soft inflatable microactuator is expected to assist in performing operations in a limited space, such as in endoscopic or laparoscopic operations.

[A Case of Carcinomatosis of the Bone Marrow Due to Rectal Cancer]

A 33-year-old man was admitted due to dyschezia and melena. Colonoscopy revealed a circulating type 4 rectal tumor. Further examination revealed intestinal obstruction due to rectal cancer, paraaortic lymph node metastasis, and multiple bone metastases, and an ileus tube was transanally inserted for decompression. Bone scintigraphy revealed multiple abnormal uptake regions in the entire skeleton. We planned to perform primary tumor resection and postoperative adjuvant chemotherapy and radiotherapy administration. Peritoneal signs in the lower abdomen appeared after 6 days of tube insertion. Abdominal computed tomography demonstrated intestinal perforation, and emergency surgery was performed. During the surgery, tube penetration in the anterior abdominal wall was observed in the sigmoid colon proximal to the tumor. Postoperatively, the patient developed disseminated intravascular coagulation(DIC). The patient had multiple bone metastases and juvenile cells in peripheral blood figure analysis; therefore, we concluded that DIC was caused by carcinomatosis of the bone marrow. After an informed consent was obtained, FOLFOX4 with simultaneous DIC treatment was initiated, and DIC remission was observed. The patient was transferred to a different hospital near his home, but died 35 days postoperatively.

[Successful Control of Hyperammonemia with BRTO of a Splenorenal Shunt Induced by CAPOX Therapy]

Among portosystemic shunts, splenorenal shunts can cause increased portal pressure, which in turn can bring about hyperammonemia, resulting in hepatic encephalopathy. In recent years, it has been reported that oxaliplatin(OX), a key chemotherapy drug in colorectal cancer, can precipitate splenorenal shunts due to sinusoidal injury. We report a case of hyperammonemia post oxaliplatin therapy. A 72-year-old male patient who had undergone surgical resection for(RS)rectal cancer with hepatic metastasis had been receiving capecitabine plus OX(CAPOX)as adjuvant chemotherapy. During his 7th course of treatment, he visited the outpatient clinic with complaints of weakness, dysarthria, and urinary incontinence. Laboratory findings showed an elevated NH3 level (200 μg/dL), and subsequent abdominal computed tomography revealed a splenorenal shunt, which was attributed to OX. Balloon-occluded retrograde transvenous obliteration(BRTO)was then performed. The patient has been routinely followed up in the outpatient clinic and has had no recurrence of hyperammonemia or cancer 14 months after the procedure. In retrospect, the splenorenal shunt was present on his first visit, therefore, hyperammonemia could have been prevented at the time of commencement of chemotherapy. We report our case, along with the relevant literature.

Time-to-onset of diabetes with everolimus use: analysis of a spontaneous reporting system database

The incidence of hyperglycemia and diabetes induced by everolimus has been shown in previous studies. Our study analyzed diabetes time-to-onset profiles after everolimus use in patients who underwent transplantation and patients with cancer. Using data from April 2007 to December 2018 in the Japanese Adverse Drug Event Report database, the reports with everolimus were classified according to its use as an immunosuppressant or anticancer drug. The median (25%-75%) days of diabetes time-to-onset in patients who underwent transplantation and patients with cancer were 172 (56-315) and 32 (18.5-57), respectively. There were no significant variations among patients with breast cancer, neuroendocrine tumor, and renal cell carcinoma. By conducting a Weibull shape parameter test, the lower limits of the 95% confidence intervals of the shape parameter β values for the indications of the cancer types were >1, indicating the wear out failure type profile, whereas those for transplantation data indicated a random failure type profile. The diabetes time-to-onset profiles after everolimus use differed between usage as an anticancer drug and immunosuppressant and there were no significant variations among the type of cancer. It was suggested that the incidence of diabetes should be monitored for 1-2 months in patients with cancer, whereas continuous monitoring is needed in patients who undergo transplantation.

Intravenous transplantation of human muse cells improves blood perfusion in a mouse model of limb ischemia

Introduction

Critical limb ischemia (CLI) is the end-stage of peripheral artery disease caused by atherosclerosis and inflammation. Despite advances in treatment of CLI, substantial number of patients with CLI suffer from severe pain, ulceration, and gangrene. Although the advent of stem cell-based therapy has opened a new avenue for the treatment of various diseases, accumulating evidence suggests current cell-based therapies are safe, but their efficacy is modest in CLI patients. Multilineage-differentiating stress enduring (Muse) cells were first reported by one of the authors and colleagues as endogenous pluripotent-like stem cells residing in the bone marrow, peripheral blood and connective tissue of many organs. Previous studies have demonstrated that systemic administration of exogenous Muse cells improves functional recovery after ischemic organ injury such as myocardial infarction. However, their therapeutic potential in CLI remains unclear.

Objective

The goal of this study is to elucidate the efficacy and safety of exogenous Muse cell transplantation with animal models of CLI.

Methods

Muse cells were isolated from human bone marrow-derived mesenchymal stem cells (MSCs) by fluorescence-activated cell sorting with anti-SSEA-3 antibody. To establish an animal model of CLI, 12–14-week-old male BALB/c mice were anesthetized and subjected to left femoral artery and vein resection. At 24 hours after establishment of hindlimb ischemia, mice were randomly divided into 5 groups and treated as follows: Group 1, intravenous injection of PBS as control group; group 2, intravenous injection of 3 × 104 SSEA3-negative MSCs (non-Muse MSCs); group 3, intravenous injection of 3 × 104 Muse cells; group 4, intramuscular injection of 3 × 104 Muse cells into ischemic limb; group 5, intramuscular injection of 2 × 105 mouse bone marrow-derived mononuclear cells (BM-MNCs) into ischemic limb (n=5 for each group). Hindlimb blood flow was evaluated by laser Doppler flowmetry for 14 days and expressed as the ratio of ischemic to non-ischemic hindlimb.

Results

We found that intramuscular injection of xenogeneic Muse cells without immunosuppression significantly improved the blood flow in the ischemic hindlimb compared to control at day 7 and 14 (0.67 vs. 0.52, p=0.0002 and 0.74 vs. 0.53, p<0.0001, respectively) similar to intramuscular injection of allogenic BM-MNCs. In addition, we also found that intravenous injection of xenogeneic Muse cells without immunosuppression significantly improved the blood flow in the ischemic hindlimb compared to control at day 7 and 14 (0.72, p<0.0001 and 0.67, p=0.004, respectively). In contrast, intravenous injection of xenogeneic non-Muse MSCs did not improve blood flow in the ischemic hindlimb.

Conclusion

Our result suggests that Muse cell-based regenerative therapy could be a novel, less invasive, cost-effective, and subsequently more effective treatment for CLI patients.

Funding Acknowledgement

Type of funding source: Public grant(s) – National budget only. Main funding source(s): Grant-in-Aid for Scientific Research (KAKENHI)

The correlations between anti-factor Xa activity values and PT/APTT at peak and trough times in patients with venous thromboembolism using high dose of apixaban

Background

The high dose (20mg/day) of apixaban is used for the initial treatment of venous thromboembolism for the first week. Although patients taking direct oral anticoagulants do not require routine coagulation monitoring, the correlations between anti-factor Xa activity (AXA) and routine coagulation markers such as prothrombin time (PT) and activated partial thromboplastin time (APTT) at peak and trough times especially when using high dose of apixaban have not been reported so far.

Purpose

The purpose is to assess the correlations between AXA values and PT/APTT at peak and trough times in patients with venous thromboembolism using high dose of Apixaban.

Methods

Twenty-six patients (10 male; 71±15 years) with proximal venous thromboembolism or pulmonary embolism using high dose (20mg/day) of apixaban were enrolled. We measured AXA, using chromogenic assay with the HemosIL Liquid Heparin kit, PT and APTT at peak and trough times. The peak time was defined as 3 hours after the intake of apixaban, and the trough time was defined as that immediately before the intake of apixaban.

Results

A significant and strong positive correlation was observed between AXA and PT at both peak and trough times (R=0.795, p<0.01 and R=0.766, p<0.01, respectively). A significant and moderate positive correlation was observed between AXA and APTT at trough time (R=0.527, p<0.01), but no correlation was observed between AXA and APTT at peak time (R=0.366, p=0.07).

Conclusion

Our findings reveal the relationship between AXA and PT at peak and trough times has a significant strong correlation. These results suggest measuring of PT may be alternative and effective way of monitoring of AXA values when using high dose of apixaban.

Figure 1

Funding Acknowledgement

Type of funding source: None

The distribution of anti-factor Xa activity value, PT and APTT at peak and trough times in patients with direct anti-factor Xa inhibitors

Background

Although patients taking direct oral anticoagulants (DOACs) do not require routine coagulation monitoring, the distribution of anti-factor Xa activity (AXA) values, prothrombin time (PT), PT-international normalized ratio (INR) and activated partial thromboplastin time (APTT) in patients on apixaban, edoxaban and rivaroxaban therapy is still not clear.

Purpose

The aim is to set the standard values of AXA values, PT, PT-INR and APTT in patients using DOACs.

Methods

We measured AXA, using chromogenic assay with the HemosIL Liquid Heparin kit, PT, PT-INR and APTT at trough and peak times in 224 patients with non-valvular atrial fibrillation and venous thromboembolism, of whom 90 received apixaban, 100 received edoxaban and 34 received rivaroxaban. The peak time was defined as 3 hours after the intake of apixaban or rivaroxaban, and 2 hours after the intake of edoxaban. The trough time was defined as that immediately before the intake. The AXA values, PT, PT-INR and APTT were measured at least 72 hours after the start of treatment. The dosage of DOACs is defined according to the prescribing information in Japan.

Results

(The order of results below is apixaban, edoxaban and rivaroxaban, respectively.) The average AXA values were 2.29, 0.23 and 0.39 (IU/mL) at trough time, and 3.04, 1.01 and 1.70 (IU/mL) at peak time. The average PT values were 17.9, 12.9 and 13.1 (s) at trough time, and 19.7, 15.5 and 17.5 (s) at peak time. The average PT-INR values were 1.49, 1.07 and 1.08 at trough time, and 1.65, 1.29 and 1.45 at peak time. The average APPT values were 34.5, 31.3 and 32.0 (s) at trough time, and 39.5, 35.9 and 39.8 (s) at peak time.

Conclusion

Our findings reveal the standard values of AXA, PT, PT-INR and APTT in patients using apixaban, edoxaban and rivaroxaban in each dosage. The DOACs should be changed if the measured value is out of those standard values in 90% confidence interval.

Funding Acknowledgement

Type of funding source: None

Psoriasis associated with ACE inhibitors: an analysis of the FAERS database

Many case reports have been published concerning the development or exacerbation of psoriasis after administration of angiotensin-converting enzyme (ACE) inhibitors. The aim of the present study was to investigate the association between psoriasis and ACE inhibitors using the US Food and Drug Administration Adverse Event Reporting System (FAERS) data. After excluding patients with psoriasis-related primary diseases, the association of psoriasis with 14 ACE inhibitors was examined using disproportional analyses reporting odds ratio (ROR) and information component (IC). Signals were detected for all 14 ACE inhibitors combined (ROR: 1.25, 95% confidence interval [CI]: 1.14-1.37; IC: 0.31, 95% CI: 0.17-0.44) and individually for lisinopril (ROR: 1.20, 95% CI: 1.05-1.37; IC: 0.25, 95% CI: 0.06-0.45), perindopril (ROR: 1.86, 95% CI: 1.38-2.52; IC: 0.86, 95% CI: 0.43-1.30), and ramipril (ROR: 1.63, 95% CI: 1.36-1.96; IC: 0.69, 95% CI: 0.42-0.96). ACE inhibitors are widely used in patients with hypertension, heart failure, and diabetes mellitus, which are considered comorbidities of psoriasis. Our results suggest that the involvement of ACE inhibitors should be considered in patients on ACE inhibitor therapy who have developed (or show exacerbated) psoriasis.

Erratum: Evolution of π^{0} Suppression in Au+Au Collisions from sqrt[s_{NN}]=39 to 200 GeV [Phys. Rev. Lett. 109, 152301 (2012)]

This corrects the article DOI: 10.1103/PhysRevLett.109.152301.

The natural course of the paravertebral muscles after the onset of osteoporotic vertebral fracture

This study revealed the change in the paravertebral muscles in patients with osteoporotic vertebral fracture. Increased pain is likely to be the driver for reduced activity, reduced activities of daily living, and consequent increase in fat infiltration of the paravertebral muscles, assumed to be secondary to reduced activity level or, conversely, partial immobilization.

INTRODUCTION

To reveal the time courses and impact of the paravertebral muscles (PVMs) on the healing process of osteoporotic vertebral fractures and risk factors for PVM decrease.

METHODS

Consecutive patients with symptomatic osteoporotic vertebral fractures were enrolled in 11 hospitals. At enrollment and 3- and 6-month follow-up, PVMs, including the multifidus and erector spinae, were examined using magnetic resonance imaging (MRI). The PVM cross-sectional area (CSA) and fat signal fraction (FSF) were measured at L3. Low back pain (LBP), activities of daily living (ADLs), and risk factors for PVM decrease at the 6-month follow-up were investigated. PVM decrease was defined as > 1 standard deviation decrease of the CSA or > 1 standard deviation increase of the FSF.

RESULTS

Among 153 patients who completed the 6-month follow-up, 117 (92 women, 79%) had MRI of L3 at enrollment and 3- and 6-month follow-up (mean age at enrollment, 78.5 years). The CSA did not change 6 months from onset (p for trend = 0.634), whereas the FSF significantly increased (p for trend = 0.033). PVM decrease was observed in 30 patients (26%). LBP was more severe, and delayed union was more frequent in patients with PVM decrease (p = 0.021 mixed-effect model and p = 0.029 chi-square test, respectively). The risk factors for PVM decrease were ADL decline at the 3-month follow-up (adjusted odds ratio = 5.35, p = 0.026).

CONCLUSION

PVM decrease was significantly related to LBP and delayed union after osteoporotic vertebral fracture onset. ADL decline at the 3-month follow-up was a risk factor for PVM decrease. Therefore, restoring ADLs within 3 months after onset is important.

Left ventricular outflow tract pressure gradient changes after carvedilol-disopyramide cotherapy in a cat with hypertrophic obstructive cardiomyopathy

Disopyramide reduces the left ventricular outflow tract (LVOT) pressure gradient and improves symptoms in humans with hypertrophic obstructive cardiomyopathy (HOCM). However, the efficacy of disopyramide in cats has not been reported. We treated a cat with HOCM with carvedilol and disopyramide cotherapy and monitored the changes in LVOT flow velocity and N-terminal pro B-type natriuretic peptide (NT-proBNP) concentration. A 10-month-old neutered male Norwegian Forest cat was referred with a moderate systolic cardiac murmur. Echocardiography revealed thickening of the left ventricular wall, systolic anterior motion of the mitral valve leaflets, and turbulent aortic flow in the LVOT at systole. The LVOT flow velocity was 5.6 m/s. The plasma NT-proBNP concentration exceeded 1,500 pmol/L. The cat was diagnosed with HOCM and the β-blocker carvedilol was started and gradually increased to 0.30 mg/kg, bid. After 57 days, the LVOT flow velocity (4.8 m/s) and plasma NT-proBNP concentration (870 pmol/L) had decreased but remained elevated. Therefore, disopyramide was added at 5.4 mg/kg po bid and increased to 10.9 mg/kg po bid after 22 days. After 141 days of carvedilol and disopyramide treatment, the systolic anterior motion of the mitral valve leaflets had disappeared and the LVOT flow velocity and plasma NT-proBNP concentration had decreased to 0.7 m/s and 499 pmol/L, respectively. No adverse effect has been observed during the follow-up. Disopyramide might relieve feline LVOT obstruction after only partial response to a beta-blocker. Further large-scale studies are required to investigate the efficacy and safety of disopyramide use in cats with moderate to severe HOCM.

Evaluation of syncope association with α1-adrenoceptor blockers in males using the FAERS database: impact of concomitant hypertension

Previous studies have revealed an association between the administration of α₁-adrenoceptor blockers (α1Bs) and episodes of syncope in patients with benign prostatic hyperplasia (BPH). The objective of the present study was to evaluate the association between α1Bs and syncope in BPH patients with hypertension using two different pharmacoepidemiological indices. Using the US Food and Drug Administration Adverse Event Reporting System, we analyzed the whole dataset and subsets for specific indications, including hypertension, diabetes, and dyslipidemia, for males older than 40 years. The drugs of interest were alfuzosin, doxazosin, and terazosin as non-selective α1Bs and silodosin and tamsulosin as selective α1Bs. The reporting odds ratio (ROR) and information component (IC) were used for signal detection. The association between the non-selective α1Bs and syncope was observed for all the items examined. The results obtained using the whole dataset, as well as the diabetes and dyslipidemia subsets, were same for the selective and non-selective α1Bs in terms of the association with syncope, while no association with syncope was observed for both silodosin [ROR: 1.09, 95% confidence interval (CI): 0.61-1.93; IC: 0.10, 95% CI: -0.72-0.92] and tamsulosin (ROR: 1.08, 95% CI: 0.90-1.30; IC: 0.10, 95% CI: -0.17-0.37) in patients with hypertension. The data suggested that α1Bs, even those with receptor subtype selectivity, were associated with syncope. Thus, careful attention should be paid when prescribing α1Bs, especially to patients who do not take medications for hypertension.

[A Case of Long-Term Survival of a Patient with a Nodal Recurrence of Intrahepatic Cholangiocarcinoma Who Attained Complete Remission with S-1 Monotherapy]

An 82-year-old man was referred to our hospital after a hepatic tumor was identified on ultrasonography.Computed tomography(CT)revealed a hypovascular tumor measuring 3 cm in diameter in the lateral section.He was diagnosed as having intrahepatic cholangiocarcinoma(ICC), and a left hemihepatectomy was performed in November 2012. During the postoperative follow-up in August 2013, CT revealed swollen lymph nodes around the greater curvature of the stomach and upper edge of the pancreas.By using endoscopic ultrasonography fine-needle aspiration(EUS-FNA), lymph node metastases of the ICC was diagnosed.S -1 monotherapy was initiated instead of gemcitabine and cisplatin regimens because of renal dysfunction.In July 2014, CT revealed that both lymph nodes were shrinking, and in January 2015, S-1 administration was discontinued upon the patient's request.However, the patient survived for 4 years without S-1 administration, and no recurrent tumors were recognized on CT in November 2018.O ur diagnosis indicates complete remission.

Beam Energy and Centrality Dependence of Direct-Photon Emission from Ultrarelativistic Heavy-Ion Collisions

The PHENIX collaboration presents first measurements of low-momentum (0.4<p_{T}<3  GeV/c) direct-photon yields from Au+Au collisions at sqrt[s_{NN}]=39 and 62.4 GeV. For both beam energies the direct-photon yields are substantially enhanced with respect to expectations from prompt processes, similar to the yields observed in Au+Au collisions at sqrt[s_{NN}]=200. Analyzing the photon yield as a function of the experimental observable dN_{ch}/dη reveals that the low-momentum (>1  GeV/c) direct-photon yield dN_{γ}^{dir}/dη is a smooth function of dN_{ch}/dη and can be well described as proportional to (dN_{ch}/dη)^{α} with α≈1.25. This scaling behavior holds for a wide range of beam energies at the Relativistic Heavy Ion Collider and the Large Hadron Collider, for centrality selected samples, as well as for different A+A collision systems. At a given beam energy, the scaling also holds for high p_{T} (>5  GeV/c), but when results from different collision energies are compared, an additional sqrt[s_{NN}]-dependent multiplicative factor is needed to describe the integrated-direct-photon yield.

Diagnostic accuracy of plasma atrial natriuretic peptide concentrations in cats with and without cardiomyopathies

OBJECTIVES

Plasma atrial natriuretic peptide (ANP) levels have been reported to be elevated in cats with cardiomyopathy. We investigated the diagnostic accuracy of plasma ANP concentration as an indicator of the severity of cardiomyopathies.

ANIMALS

This study included 78 control cats and 83 cats with various types of cardiomyopathy.

METHODS

This was a prospective multicentre study. Control cats were determined to have a normal heart, and diseased cats were diagnosed by echocardiography. Diseased cats were divided into asymptomatic cats without left atrial dilation (LAD), asymptomatic cats with LAD, and cats with heart failure. Plasma C-terminal ANP concentrations were measured using chemiluminescence.

RESULTS

The median plasma ANP concentration in controls was 43.3 (interquartile range, 33.0-56.3) pg/mL. Plasma ANP values were significantly higher in the cardiomyopathic cats with LAD and heart failure, but the values in cats without LAD were comparable to those in control cats. To distinguish cats with cardiomyopathy from controls, a plasma ANP concentration >77.5 pg/mL afforded sensitivity of 66.3% and specificity of 84.6%. Use of plasma ANP concentration >110.9 pg/mL to identify cats with LAD had a sensitivity of 73.6% and specificity of 93.5%. The areas under the receiver-operating characteristic curve were 0.80 and 0.86.

CONCLUSIONS

Plasma ANP concentrations were higher in cats with more advanced cardiomyopathy. Although assaying the ANP concentration alone may not help to diagnose cardiac disease, measuring provides additional information that is useful for assessing the severity of cardiomyopathies.

Tissue Engineering of the Small Intestine by Acellular Collagen Sponge Scaffold Grafting

Tissue engineering of the small intestine will prove a great benefit to patients suffering from short bowel disease. However cell seeding in tissue engineering, such as fetal cell use, is accompanied by problems of ethical issues, rejection, and short supply. To overcome these problems, we carried out an experimental study on tissue engineering of the small intestine by acellular collagen sponge scaffold grafting. We resected the 5 cm long jejunum from beagle dogs and reconstructed it by acellular collagen sponge grafting with a silicon tube stent. The graft was covered with the omentum. At 1 month after operation, the silicon stent was removed endoscopically. Animals were sacrificed 1 and 4 months after operation, and were examined microscopically. Neo-intestinal regeneration was observed and the intestinal mucosa covered the luminal side of the regenerated intestine across the anastomosis. Thus, the small intestine was regenerated by tissue engineering technology using an acellular collagen sponge scaffold.

Artificial Trachea and Long Term follow-up in Carinal Reconstruction in Dogs

We have already reported “del” successful carinal reconstruction of the trachea with an observation period of 1 – 2 years. In this study, we evaluate the long-term safety and efficacy of the reconstruction after 5-years of follow-up.

The Y-shaped Marlex® mesh tube was reinforced with a polypropylene spiral and coated with atelocollagen made from porcine skin. The prosthesis was 60 mm long with an outer diameter of 18 mm. Replacement of the tracheobronchial bifurcation was preformed through a right thoracotomy in a beagle dog. Bronchoscopical examination and sampling of the tracheal epithelium was performed periodically to check the function of cilia.

The implanted prothesis was promptly infiltrated by the surrounding connective tissue and completely incorporated by the host trachea and bronchus. Bronchoscopically, sufficient epithelization was confirmed from the upper to the lower site of anastomosis. After 5 years neither stenosis nor dehiscence was observed. In spite of there being mesh-exposure at the luminal surface, the dog had no clinical symptoms until sacrifice for pathological examination. The bent frequency of the cilia was maintained within the normal range, indicating “del” functional recovery of the regenerating airway.

Our tracheal prosthesis is promising for clinical “del” repair of the tracheobronchial bifurcation.

The B allele with a 5·8 kb deletion in intron 1 of the ABO gene is the major allele in Japanese individuals with Bm and A1 Bm phenotypes

B_m and A₁ B_m phenotypes are the most frequent ABO variants in the Japanese population. The B antigen on B_m red blood cells is only detectable by adsorption and elution tests, and plasma B-transferase activity is usually detected at half or less levels compared with that of common B. Recently, a B allele lacking an erythroid cell-specific transcription enhancer in intron 1 of the ABO gene was identified from individuals with B_m and A₁ B_m phenotypes, which could explain the unique serologic properties of B_m . In the Japanese Red Cross Society, eight Blood Centers tested blood samples from donors throughout Japan and collected blood samples from 888 B_m and 415 A₁ B_m individuals. DNA analysis revealed that 1300 of 1303 (99·77%) individuals had the B allele with a 5·8 kb deletion (c.28 + 5110_10889del), which included the enhancer element.

Measurements of Elliptic and Triangular Flow in High-Multiplicity 3He+Au Collisions at √(s(NN))=200 GeV

We present the first measurement of elliptic (v(2)) and triangular (v(3)) flow in high-multiplicity (3)He+Au collisions at √(s(NN))=200  GeV. Two-particle correlations, where the particles have a large separation in pseudorapidity, are compared in (3)He+Au and in p+p collisions and indicate that collective effects dominate the second and third Fourier components for the correlations observed in the (3)He+Au system. The collective behavior is quantified in terms of elliptic v(2) and triangular v(3) anisotropy coefficients measured with respect to their corresponding event planes. The v(2) values are comparable to those previously measured in d+Au collisions at the same nucleon-nucleon center-of-mass energy. Comparisons with various theoretical predictions are made, including to models where the hot spots created by the impact of the three (3)He nucleons on the Au nucleus expand hydrodynamically to generate the triangular flow. The agreement of these models with data may indicate the formation of low-viscosity quark-gluon plasma even in these small collision systems.

Acotiamide Hydrochloride, a Therapeutic Agent for Functional Dyspepsia, Enhances Acetylcholine-induced Contraction via Inhibition of Acetylcholinesterase Activity in Circular Muscle Strips of Guinea Pig Stomach

Acotiamide is a first-in-class prokinetic drug approved in Japan for the treatment of functional dyspepsia. Given that acotiamide enhances gastric motility in conscious dogs and rats, we assessed the in vitro effects of this drug on the contraction of guinea pig stomach strips and on acetylcholinesterase (AChE) activity in stomach homogenate following fundus removal. We also investigated the serotonin 5-HT4 receptor agonist mosapride, dopamine D2 receptor and AChE inhibitor itopride, and representative AChE inhibitor neostigmine. Acotiamide (0.3 and 1 μM) and itopride (1 and 3 μM) significantly enhanced the contraction of gastric body strips induced by electrical field stimulation (EFS), but mosapride (1 and 10 μM) did not. Acotiamide and itopride significantly enhanced the contraction of gastric body and antrum strips induced by acetylcholine (ACh), but not that induced by carbachol (CCh). Neostigmine also significantly enhanced the contraction of gastric body strips induced by ACh, but not that by CCh. In contrast, mosapride failed to enhance contractions induced by either ACh or CCh in gastric antrum strips. Acotiamide exerted mixed inhibition of AChE, and the percentage inhibition of acotiamide (100 μM) against AChE activity was markedly reduced after the reaction mixture was dialyzed. In contrast, itopride exerted noncompetitive inhibition on AChE activity. These results indicate that acotiamide enhances ACh-dependent contraction in gastric strips of guinea pigs via the inhibition of AChE activity, and that it exerts mixed and reversible inhibition of AChE derived from guinea pig stomach.

Measurement of Long-Range Angular Correlation and Quadrupole Anisotropy of Pions and (Anti)Protons in Central d+Au Collisions at sqrt[s_{NN}]=200 GeV

We present azimuthal angular correlations between charged hadrons and energy deposited in calorimeter towers in central d+Au and minimum bias p+p collisions at sqrt[s_{NN}]=200 GeV. The charged hadron is measured at midrapidity |η|<0.35, and the energy is measured at large rapidity (-3.7<η<-3.1, Au-going direction). An enhanced near-side angular correlation across |Δη|>2.75 is observed in d+Au collisions. Using the event plane method applied to the Au-going energy distribution, we extract the anisotropy strength v_{2} for inclusive charged hadrons at midrapidity up to p_{T}=4.5 GeV/c. We also present the measurement of v_{2} for identified π^{±} and (anti)protons in central d+Au collisions, and observe a mass-ordering pattern similar to that seen in heavy-ion collisions. These results are compared with viscous hydrodynamic calculations and measurements from p+Pb at sqrt[s_{NN}]=5.02 TeV. The magnitude of the mass ordering in d+Au is found to be smaller than that in p+Pb collisions, which may indicate smaller radial flow in lower energy d+Au collisions.

AN ULTRASTRUCTURAL OBSERVATION OF INTRACYTOPLASMIC DESMOSOMES IN DARIER'S DISEASE

In a typical case of Darier's disease, intracytoplasmic desmosomes, gap junctions and many vesicles were observed in the cytoplasm of epidermal keratinocytes. Intracytoplasmic desmosomes were found in the cytoplasm of the excessively keratinized cells, vacuolated cells and acantholytic cells. They were not associated with tonofilaments as much as with ordinal intercellular desmosome-tonofilament complexes, and some of them lacked a central strip and looked similar to the denatured intercellular desmosomes in the morphology of the abnormal keratinocytes of Darier's disease. These intracytoplasmic desmosomes were long and undulating and some of the showed a "tennis racket" image (Caputo). Furthermore, some were combined with the gap junction and the intermediate junction, forming a bounded vesicle in the cytoplasm.

Correction: Highly selective aluminium-catalysed intramolecular Prins reaction for l-menthol synthesis

Correction for ‘Highly selective aluminium-catalysed intramolecular Prins reaction for l-menthol synthesis’ by H. Itoh et al., RSC Adv., 2014, 4, 61619–61623.

Measurement of the cosmic microwave background polarization lensing power spectrum with the POLARBEAR experiment

Gravitational lensing due to the large-scale distribution of matter in the cosmos distorts the primordial cosmic microwave background (CMB) and thereby induces new, small-scale B-mode polarization. This signal carries detailed information about the distribution of all the gravitating matter between the observer and CMB last scattering surface. We report the first direct evidence for polarization lensing based on purely CMB information, from using the four-point correlations of even- and odd-parity E- and B-mode polarization mapped over ∼30 square degrees of the sky measured by the POLARBEAR experiment. These data were analyzed using a blind analysis framework and checked for spurious systematic contamination using null tests and simulations. Evidence for the signal of polarization lensing and lensing B modes is found at 4.2σ (stat+sys) significance. The amplitude of matter fluctuations is measured with a precision of 27%, and is found to be consistent with the Lambda cold dark matter cosmological model. This measurement demonstrates a new technique, capable of mapping all gravitating matter in the Universe, sensitive to the sum of neutrino masses, and essential for cleaning the lensing B-mode signal in searches for primordial gravitational waves.

Cold-nuclear-matter effects on heavy-quark production at forward and backward rapidity in d + Au collisions at √sNN = 200 GeV

The PHENIX experiment has measured open heavy-flavor production via semileptonic decay over the transverse momentum range 1 < p(T) < 6  GeV/c at forward and backward rapidity (1.4 < |y| < 2.0) in d+Au and p + p collisions at √sNN = 200  GeV. In central d+Au collisions, relative to the yield in p + p collisions scaled by the number of binary nucleon-nucleon collisions, a suppression is observed at forward rapidity (in the d-going direction) and an enhancement at backward rapidity (in the Au-going direction). Predictions using nuclear-modified-parton-distribution functions, even with additional nuclear-p(T) broadening, cannot simultaneously reproduce the data at both rapidity ranges, which implies that these models are incomplete and suggests the possible importance of final-state interactions in the asymmetric d + Au collision system. These results can be used to probe cold-nuclear-matter effects, which may significantly affect heavy-quark production, in addition to helping constrain the magnitude of charmonia-breakup effects in nuclear matter.

Evidence for gravitational lensing of the cosmic microwave background polarization from cross-correlation with the cosmic infrared background

We reconstruct the gravitational lensing convergence signal from cosmic microwave background (CMB) polarization data taken by the Polarbear experiment and cross-correlate it with cosmic infrared background maps from the Herschel satellite. From the cross spectra, we obtain evidence for gravitational lensing of the CMB polarization at a statistical significance of 4.0σ and indication of the presence of a lensing B-mode signal at a significance of 2.3σ. We demonstrate that our results are not biased by instrumental and astrophysical systematic errors by performing null tests, checks with simulated and real data, and analytical calculations. This measurement of polarization lensing, made via the robust cross-correlation channel, not only reinforces POLARBEAR auto-correlation measurements, but also represents one of the early steps towards establishing CMB polarization lensing as a powerful new probe of cosmology and astrophysics.

[A case of complete response(CR)to S-1 and paclitaxel(PTX)combination therapy in a patient with unresectable gastric cancer]

We report a case of a patient with unresectable gastric cancer who showed complete response(CR)to S-1 and paclitaxel (PTX)combination therapy. The patient(a 67-year-old woman)was diagnosed with unresectable advanced gastric cancer with metastases in the Virchow's lymph nodes and para-aortic lymph nodes. Systemic chemotherapy with 70mg/m2 S-1 (days 1-14)and 70mg/m2 PTX(day 1)was administered every 3 weeks. At the end of 7 courses of chemotherapy, the primary lesion and swollen lymph nodes became markedly smaller. After 7 courses, an additional 39 courses were administered over 2.5 years. No notable adverse events were seen, and the patient's performance status(PS)was 0. CR was monitored by imaging studies. No cancer cells were detected on cytological examination of the primary lesion. Monotherapy with 70mg/m2 S-1(days 1-28, 2-week drug holiday)has been administered for the past 3 years. The patient is currently treated as an outpatient and maintains CR and a PS of 0.

Highly selective aluminium-catalysed intramolecular Prins reaction for l-menthol synthesis

The perfect production of l-menthol.

Energy dependence of the transverse momentum distributions of charged particles in pp collisions measured by ALICE

Differential cross sections of charged particles in inelastic pp collisions as a function of p_T have been measured at [Formula: see text] at the LHC. The p_T spectra are compared to NLO-pQCD calculations. Though the differential cross section for an individual [Formula: see text] cannot be described by NLO-pQCD, the relative increase of cross section with [Formula: see text] is in agreement with NLO-pQCD. Based on these measurements and observations, procedures are discussed to construct pp reference spectra at [Formula: see text] up to p_T=50 GeV/c as required for the calculation of the nuclear modification factor in nucleus-nucleus and proton-nucleus collisions.

Directed flow of charged particles at midrapidity relative to the spectator plane in Pb-Pb collisions at √(s(NN))=2.76 TeV

The directed flow of charged particles at midrapidity is measured in Pb-Pb collisions at √(s(NN))=2.76 TeV relative to the collision symmetry plane defined by the spectator nucleons. A negative slope of the rapidity-odd directed flow component with approximately 3 times smaller magnitude than found at the highest RHIC energy is observed. This suggests a smaller longitudinal tilt of the initial system and disfavors the strong fireball rotation predicted for the LHC energies. The rapidity-even directed flow component is measured for the first time with spectators and found to be independent of pseudorapidity with a sign change at transverse momenta p(T) between 1.2 and 1.7  GeV/c. Combined with the observation of a vanishing rapidity-even p(T) shift along the spectator deflection this is strong evidence for dipolelike initial density fluctuations in the overlap zone of the nuclei. Similar trends in the rapidity-even directed flow and the estimate from two-particle correlations at midrapidity, which is larger by about a factor of 40, indicate a weak correlation between fluctuating participant and spectator symmetry planes. These observations open new possibilities for investigation of the initial conditions in heavy-ion collisions with spectator nucleons.

K(S)0 and Λ production in Pb-Pb collisions at √(s(NN))=2.76 TeV

The ALICE measurement of K(S)(0) and Λ production at midrapidity in Pb-Pb collisions at √(s(NN))=2.76 TeV is presented. The transverse momentum (p(T)) spectra are shown for several collision centrality intervals and in the p(T) range from 0.4 GeV/c (0.6 GeV/c for Λ) to 12 GeV/c. The p(T) dependence of the Λ/K(S)(0) ratios exhibits maxima in the vicinity of 3 GeV/c, and the positions of the maxima shift towards higher p(T) with increasing collision centrality. The magnitude of these maxima increases by almost a factor of three between most peripheral and most central Pb-Pb collisions. This baryon excess at intermediate p(T) is not observed in pp interactions at √s=0.9 TeV and at √s=7 TeV. Qualitatively, the baryon enhancement in heavy-ion collisions is expected from radial flow. However, the measured p(T) spectra above 2 GeV/c progressively decouple from hydrodynamical-model calculations. For higher values of p(T), models that incorporate the influence of the medium on the fragmentation and hadronization processes describe qualitatively the p(T) dependence of the Λ/K(S)(0) ratio.

Charmonium and e+e- pair photoproduction at mid-rapidity in ultra-peripheral Pb-Pb collisions at [Formula: see text]

The ALICE Collaboration at the LHC has measured the J/ψ and ψ' photoproduction at mid-rapidity in ultra-peripheral Pb-Pb collisions at [Formula: see text]. The charmonium is identified via its leptonic decay for events where the hadronic activity is required to be minimal. The analysis is based on an event sample corresponding to an integrated luminosity of about 23 μb-1. The cross section for coherent and incoherent J/ψ production in the rapidity interval -0.9 Collapse

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Affiliation(s)

The ALICE Collaboration CERN, 1211 Geneva 23, Switzerland
E. Abbas Academy of Scientific Research and Technology (ASRT), Cairo, Egypt Fachhochschule Köln, Köln, Germany Department of Physics, Gauhati University, Guwahati, India Suranaree University of Technology, Nakhon Ratchasima, Thailand University of Technology and Austrian Academy of Sciences, Vienna, Austria
B. Abelev Lawrence Livermore National Laboratory, Livermore, California United States
J. Adam Faculty of Nuclear Sciences and Physical Engineering, Czech Technical University in Prague, Prague, Czech Republic
D. Adamová Nuclear Physics Institute, Academy of Sciences of the Czech Republic, Řež u Prahy, Czech Republic
A. M. Adare Yale University, New Haven, Connecticut United States
M. M. Aggarwal Physics Department, Panjab University, Chandigarh, India
G. Aglieri Rinella European Organization for Nuclear Research (CERN), Geneva, Switzerland
M. Agnello Politecnico di Torino, Turin, Italy Sezione INFN, Turin, Italy
A. G. Agocs Wigner Research Centre for Physics, Hungarian Academy of Sciences, Budapest, Hungary
A. Agostinelli Dipartimento di Fisica e Astronomia dell’Università and Sezione INFN, Bologna, Italy
Z. Ahammed Variable Energy Cyclotron Centre, Kolkata, India
N. Ahmad Department of Physics, Aligarh Muslim University, Aligarh, India
A. Ahmad Masoodi Department of Physics, Aligarh Muslim University, Aligarh, India
I. Ahmed COMSATS Institute of Information Technology (CIIT), Islamabad, Pakistan
S. A. Ahn Korea Institute of Science and Technology Information, Daejeon, South Korea
S. U. Ahn Korea Institute of Science and Technology Information, Daejeon, South Korea
I. Aimo Dipartimento di Fisica dell’Università and Sezione INFN, Turin, Italy Politecnico di Torino, Turin, Italy Sezione INFN, Turin, Italy
M. Ajaz COMSATS Institute of Information Technology (CIIT), Islamabad, Pakistan
A. Akindinov Institute for Theoretical and Experimental Physics, Moscow, Russia
D. Aleksandrov Russian Research Centre Kurchatov Institute, Moscow, Russia
B. Alessandro Sezione INFN, Turin, Italy
D. Alexandre School of Physics and Astronomy, University of Birmingham, Birmingham, United Kingdom
A. Alici Centro Fermi - Museo Storico della Fisica e Centro Studi e Ricerche “Enrico Fermi”, Rome, Italy Sezione INFN, Bologna, Italy
A. Alkin Bogolyubov Institute for Theoretical Physics, Kiev, Ukraine
E. Almaráz Aviña Instituto de Física, Universidad Nacional Autónoma de México, Mexico City, Mexico
J. Alme Faculty of Engineering, Bergen University College, Bergen, Norway
T. Alt Frankfurt Institute for Advanced Studies, Johann Wolfgang Goethe-Universität Frankfurt, Frankfurt, Germany
V. Altini Dipartimento Interateneo di Fisica ‘M. Merlin’ and Sezione INFN, Bari, Italy
S. Altinpinar Department of Physics and Technology, University of Bergen, Bergen, Norway
I. Altsybeev V. Fock Institute for Physics, St. Petersburg State University, St. Petersburg, Russia
C. Andrei National Institute for Physics and Nuclear Engineering, Bucharest, Romania
A. Andronic Research Division and ExtreMe Matter Institute EMMI, GSI Helmholtzzentrum für Schwerionenforschung, Darmstadt, Germany
V. Anguelov Physikalisches Institut, Ruprecht-Karls-Universität Heidelberg, Heidelberg, Germany
J. Anielski Institut für Kernphysik, Westfälische Wilhelms-Universität Münster, Münster, Germany
C. Anson Department of Physics, Ohio State University, Columbus, Ohio United States
T. Antičić Rudjer Bošković Institute, Zagreb, Croatia
F. Antinori Sezione INFN, Padova, Italy
P. Antonioli Sezione INFN, Bologna, Italy
L. Aphecetche SUBATECH, Ecole des Mines de Nantes, Université de Nantes, CNRS-IN2P3, Nantes, France
H. Appelshäuser Institut für Kernphysik, Johann Wolfgang Goethe-Universität Frankfurt, Frankfurt, Germany
N. Arbor Laboratoire de Physique Subatomique et de Cosmologie (LPSC), Université Joseph Fourier, CNRS-IN2P3, Institut Polytechnique de Grenoble, Grenoble, France
S. Arcelli Dipartimento di Fisica e Astronomia dell’Università and Sezione INFN, Bologna, Italy
A. Arend Institut für Kernphysik, Johann Wolfgang Goethe-Universität Frankfurt, Frankfurt, Germany
N. Armesto Departamento de Física de Partículas and IGFAE, Universidad de Santiago de Compostela, Santiago de Compostela, Spain
R. Arnaldi Sezione INFN, Turin, Italy
T. Aronsson Yale University, New Haven, Connecticut United States
I. C. Arsene Research Division and ExtreMe Matter Institute EMMI, GSI Helmholtzzentrum für Schwerionenforschung, Darmstadt, Germany
M. Arslandok Institut für Kernphysik, Johann Wolfgang Goethe-Universität Frankfurt, Frankfurt, Germany
A. Asryan V. Fock Institute for Physics, St. Petersburg State University, St. Petersburg, Russia
A. Augustinus European Organization for Nuclear Research (CERN), Geneva, Switzerland
R. Averbeck Research Division and ExtreMe Matter Institute EMMI, GSI Helmholtzzentrum für Schwerionenforschung, Darmstadt, Germany
T. C. Awes Oak Ridge National Laboratory, Oak Ridge, Tennessee United States
J. Äystö Helsinki Institute of Physics (HIP) and University of Jyväskylä, Jyväskylä, Finland
M. D. Azmi Department of Physics, Aligarh Muslim University, Aligarh, India Physics Department, University of Cape Town and iThemba LABS, National Research Foundation, Somerset West, South Africa
M. Bach Frankfurt Institute for Advanced Studies, Johann Wolfgang Goethe-Universität Frankfurt, Frankfurt, Germany
A. Badalà Sezione INFN, Catania, Italy
Y. W. Baek Gangneung-Wonju National University, Gangneung, South Korea Laboratoire de Physique Corpusculaire (LPC), Clermont Université, Université Blaise Pascal, CNRS–IN2P3, Clermont-Ferrand, France
R. Bailhache Institut für Kernphysik, Johann Wolfgang Goethe-Universität Frankfurt, Frankfurt, Germany
R. Bala Physics Department, University of Jammu, Jammu, India Sezione INFN, Turin, Italy
A. Baldisseri Commissariat à l’Energie Atomique, IRFU, Saclay, France
F. Baltasar Dos Santos Pedrosa European Organization for Nuclear Research (CERN), Geneva, Switzerland
J. Bán Institute of Experimental Physics, Slovak Academy of Sciences, Košice, Slovakia
R. C. Baral Institute of Physics, Bhubaneswar, India
R. Barbera Dipartimento di Fisica e Astronomia dell’Università and Sezione INFN, Catania, Italy
F. Barile Dipartimento Interateneo di Fisica ‘M. Merlin’ and Sezione INFN, Bari, Italy
G. G. Barnaföldi Wigner Research Centre for Physics, Hungarian Academy of Sciences, Budapest, Hungary
L. S. Barnby School of Physics and Astronomy, University of Birmingham, Birmingham, United Kingdom
V. Barret Laboratoire de Physique Corpusculaire (LPC), Clermont Université, Université Blaise Pascal, CNRS–IN2P3, Clermont-Ferrand, France
J. Bartke The Henryk Niewodniczanski Institute of Nuclear Physics, Polish Academy of Sciences, Cracow, Poland
M. Basile Dipartimento di Fisica e Astronomia dell’Università and Sezione INFN, Bologna, Italy
N. Bastid Laboratoire de Physique Corpusculaire (LPC), Clermont Université, Université Blaise Pascal, CNRS–IN2P3, Clermont-Ferrand, France
S. Basu Variable Energy Cyclotron Centre, Kolkata, India
B. Bathen Institut für Kernphysik, Westfälische Wilhelms-Universität Münster, Münster, Germany
G. Batigne SUBATECH, Ecole des Mines de Nantes, Université de Nantes, CNRS-IN2P3, Nantes, France
B. Batyunya Joint Institute for Nuclear Research (JINR), Dubna, Russia
P. C. Batzing Department of Physics, University of Oslo, Oslo, Norway
C. Baumann Institut für Kernphysik, Johann Wolfgang Goethe-Universität Frankfurt, Frankfurt, Germany
I. G. Bearden Niels Bohr Institute, University of Copenhagen, Copenhagen, Denmark
H. Beck Institut für Kernphysik, Johann Wolfgang Goethe-Universität Frankfurt, Frankfurt, Germany
N. K. Behera Indian Institute of Technology Bombay (IIT), Mumbai, India
I. Belikov Institut Pluridisciplinaire Hubert Curien (IPHC), Université de Strasbourg, CNRS-IN2P3, Strasbourg, France
F. Bellini Dipartimento di Fisica e Astronomia dell’Università and Sezione INFN, Bologna, Italy
R. Bellwied University of Houston, Houston, Texas United States
E. Belmont-Moreno Instituto de Física, Universidad Nacional Autónoma de México, Mexico City, Mexico
G. Bencedi Wigner Research Centre for Physics, Hungarian Academy of Sciences, Budapest, Hungary
S. Beole Dipartimento di Fisica dell’Università and Sezione INFN, Turin, Italy
I. Berceanu National Institute for Physics and Nuclear Engineering, Bucharest, Romania
A. Bercuci National Institute for Physics and Nuclear Engineering, Bucharest, Romania
Y. Berdnikov Petersburg Nuclear Physics Institute, Gatchina, Russia
D. Berenyi Wigner Research Centre for Physics, Hungarian Academy of Sciences, Budapest, Hungary
A. A. E. Bergognon SUBATECH, Ecole des Mines de Nantes, Université de Nantes, CNRS-IN2P3, Nantes, France
R. A. Bertens Nikhef, National Institute for Subatomic Physics and Institute for Subatomic Physics of Utrecht University, Utrecht, Netherlands
D. Berzano Dipartimento di Fisica dell’Università and Sezione INFN, Turin, Italy Sezione INFN, Turin, Italy
L. Betev European Organization for Nuclear Research (CERN), Geneva, Switzerland
A. Bhasin Physics Department, University of Jammu, Jammu, India
A. K. Bhati Physics Department, Panjab University, Chandigarh, India
J. Bhom University of Tsukuba, Tsukuba, Japan
L. Bianchi Dipartimento di Fisica dell’Università and Sezione INFN, Turin, Italy
N. Bianchi Laboratori Nazionali di Frascati, INFN, Frascati, Italy
C. Bianchin Nikhef, National Institute for Subatomic Physics and Institute for Subatomic Physics of Utrecht University, Utrecht, Netherlands
J. Bielčík Faculty of Nuclear Sciences and Physical Engineering, Czech Technical University in Prague, Prague, Czech Republic
J. Bielčíková Nuclear Physics Institute, Academy of Sciences of the Czech Republic, Řež u Prahy, Czech Republic
A. Bilandzic Niels Bohr Institute, University of Copenhagen, Copenhagen, Denmark
S. Bjelogrlic Nikhef, National Institute for Subatomic Physics and Institute for Subatomic Physics of Utrecht University, Utrecht, Netherlands
F. Blanco Centro de Investigaciones Energéticas Medioambientales y Tecnológicas (CIEMAT), Madrid, Spain
F. Blanco University of Houston, Houston, Texas United States
D. Blau Russian Research Centre Kurchatov Institute, Moscow, Russia
C. Blume Institut für Kernphysik, Johann Wolfgang Goethe-Universität Frankfurt, Frankfurt, Germany
M. Boccioli European Organization for Nuclear Research (CERN), Geneva, Switzerland
S. Böttger Institut für Informatik, Johann Wolfgang Goethe-Universität Frankfurt, Frankfurt, Germany
A. Bogdanov Moscow Engineering Physics Institute, Moscow, Russia
H. Bøggild Niels Bohr Institute, University of Copenhagen, Copenhagen, Denmark
M. Bogolyubsky Institute for High Energy Physics, Protvino, Russia
L. Boldizsár Wigner Research Centre for Physics, Hungarian Academy of Sciences, Budapest, Hungary
M. Bombara Faculty of Science, P.J. Šafárik University, Košice, Slovakia
J. Book Institut für Kernphysik, Johann Wolfgang Goethe-Universität Frankfurt, Frankfurt, Germany
H. Borel Commissariat à l’Energie Atomique, IRFU, Saclay, France
A. Borissov Wayne State University, Detroit, Michigan United States
F. Bossú Physics Department, University of Cape Town and iThemba LABS, National Research Foundation, Somerset West, South Africa
M. Botje Nikhef, National Institute for Subatomic Physics, Amsterdam, Netherlands
E. Botta Dipartimento di Fisica dell’Università and Sezione INFN, Turin, Italy
E. Braidot Lawrence Berkeley National Laboratory, Berkeley, California United States
P. Braun-Munzinger Research Division and ExtreMe Matter Institute EMMI, GSI Helmholtzzentrum für Schwerionenforschung, Darmstadt, Germany
M. Bregant SUBATECH, Ecole des Mines de Nantes, Université de Nantes, CNRS-IN2P3, Nantes, France
T. Breitner Institut für Informatik, Johann Wolfgang Goethe-Universität Frankfurt, Frankfurt, Germany
T. A. Broker Institut für Kernphysik, Johann Wolfgang Goethe-Universität Frankfurt, Frankfurt, Germany
T. A. Browning Purdue University, West Lafayette, Indiana United States
M. Broz Faculty of Mathematics, Physics and Informatics, Comenius University, Bratislava, Slovakia
R. Brun European Organization for Nuclear Research (CERN), Geneva, Switzerland
E. Bruna Dipartimento di Fisica dell’Università and Sezione INFN, Turin, Italy Sezione INFN, Turin, Italy
G. E. Bruno Dipartimento Interateneo di Fisica ‘M. Merlin’ and Sezione INFN, Bari, Italy
D. Budnikov Russian Federal Nuclear Center (VNIIEF), Sarov, Russia
H. Buesching Institut für Kernphysik, Johann Wolfgang Goethe-Universität Frankfurt, Frankfurt, Germany
S. Bufalino Dipartimento di Fisica dell’Università and Sezione INFN, Turin, Italy Sezione INFN, Turin, Italy
P. Buncic European Organization for Nuclear Research (CERN), Geneva, Switzerland
O. Busch Physikalisches Institut, Ruprecht-Karls-Universität Heidelberg, Heidelberg, Germany
Z. Buthelezi Physics Department, University of Cape Town and iThemba LABS, National Research Foundation, Somerset West, South Africa
D. Caffarri Dipartimento di Fisica e Astronomia dell’Università and Sezione INFN, Padova, Italy Sezione INFN, Padova, Italy
X. Cai Central China Normal University, Wuhan, China
H. Caines Yale University, New Haven, Connecticut United States
E. Calvo Villar Sección Física, Departamento de Ciencias, Pontificia Universidad Católica del Perú, Lima, Peru
P. Camerini Dipartimento di Fisica dell’Università and Sezione INFN, Trieste, Italy
V. Canoa Roman Centro de Investigación y de Estudios Avanzados (CINVESTAV), Mexico City and Mérida, Mexico
G. Cara Romeo Sezione INFN, Bologna, Italy
W. Carena European Organization for Nuclear Research (CERN), Geneva, Switzerland
F. Carena European Organization for Nuclear Research (CERN), Geneva, Switzerland
N. Carlin Filho Universidade de São Paulo (USP), São Paulo, Brazil
F. Carminati European Organization for Nuclear Research (CERN), Geneva, Switzerland
A. Casanova Díaz Laboratori Nazionali di Frascati, INFN, Frascati, Italy
J. Castillo Castellanos Commissariat à l’Energie Atomique, IRFU, Saclay, France
J. F. Castillo Hernandez Research Division and ExtreMe Matter Institute EMMI, GSI Helmholtzzentrum für Schwerionenforschung, Darmstadt, Germany
E. A. R. Casula Dipartimento di Fisica dell’Università and Sezione INFN, Cagliari, Italy
V. Catanescu National Institute for Physics and Nuclear Engineering, Bucharest, Romania
C. Cavicchioli European Organization for Nuclear Research (CERN), Geneva, Switzerland
C. Ceballos Sanchez Centro de Aplicaciones Tecnológicas y Desarrollo Nuclear (CEADEN), Havana, Cuba
J. Cepila Faculty of Nuclear Sciences and Physical Engineering, Czech Technical University in Prague, Prague, Czech Republic
P. Cerello Sezione INFN, Turin, Italy
B. Chang Helsinki Institute of Physics (HIP) and University of Jyväskylä, Jyväskylä, Finland Yonsei University, Seoul, South Korea
S. Chapeland European Organization for Nuclear Research (CERN), Geneva, Switzerland
J. L. Charvet Commissariat à l’Energie Atomique, IRFU, Saclay, France
S. Chattopadhyay Variable Energy Cyclotron Centre, Kolkata, India
S. Chattopadhyay Saha Institute of Nuclear Physics, Kolkata, India
M. Cherney Physics Department, Creighton University, Omaha, Nebraska United States
C. Cheshkov European Organization for Nuclear Research (CERN), Geneva, Switzerland Université de Lyon, Université Lyon 1, CNRS/IN2P3, IPN-Lyon, Villeurbanne, France
B. Cheynis Université de Lyon, Université Lyon 1, CNRS/IN2P3, IPN-Lyon, Villeurbanne, France
V. Chibante Barroso European Organization for Nuclear Research (CERN), Geneva, Switzerland
D. D. Chinellato University of Houston, Houston, Texas United States
P. Chochula European Organization for Nuclear Research (CERN), Geneva, Switzerland
M. Chojnacki Niels Bohr Institute, University of Copenhagen, Copenhagen, Denmark
S. Choudhury Variable Energy Cyclotron Centre, Kolkata, India
P. Christakoglou Nikhef, National Institute for Subatomic Physics, Amsterdam, Netherlands
C. H. Christensen Niels Bohr Institute, University of Copenhagen, Copenhagen, Denmark
P. Christiansen Division of Experimental High Energy Physics, University of Lund, Lund, Sweden
T. Chujo University of Tsukuba, Tsukuba, Japan
S. U. Chung Pusan National University, Pusan, South Korea
C. Cicalo Sezione INFN, Cagliari, Italy
L. Cifarelli Centro Fermi - Museo Storico della Fisica e Centro Studi e Ricerche “Enrico Fermi”, Rome, Italy Dipartimento di Fisica e Astronomia dell’Università and Sezione INFN, Bologna, Italy
F. Cindolo Sezione INFN, Bologna, Italy
J. Cleymans Physics Department, University of Cape Town and iThemba LABS, National Research Foundation, Somerset West, South Africa
F. Colamaria Dipartimento Interateneo di Fisica ‘M. Merlin’ and Sezione INFN, Bari, Italy
D. Colella Dipartimento Interateneo di Fisica ‘M. Merlin’ and Sezione INFN, Bari, Italy
A. Collu Dipartimento di Fisica dell’Università and Sezione INFN, Cagliari, Italy
G. Conesa Balbastre Laboratoire de Physique Subatomique et de Cosmologie (LPSC), Université Joseph Fourier, CNRS-IN2P3, Institut Polytechnique de Grenoble, Grenoble, France
Z. Conesa del Valle European Organization for Nuclear Research (CERN), Geneva, Switzerland Institut de Physique Nucléaire d’Orsay (IPNO), Université Paris-Sud, CNRS-IN2P3, Orsay, France
M. E. Connors Yale University, New Haven, Connecticut United States
G. Contin Dipartimento di Fisica dell’Università and Sezione INFN, Trieste, Italy
J. G. Contreras Centro de Investigación y de Estudios Avanzados (CINVESTAV), Mexico City and Mérida, Mexico
T. M. Cormier Wayne State University, Detroit, Michigan United States
Y. Corrales Morales Dipartimento di Fisica dell’Università and Sezione INFN, Turin, Italy
P. Cortese Dipartimento di Scienze e Innovazione Tecnologica dell’Università del Piemonte Orientale and Gruppo Collegato INFN, Alessandria, Italy
I. Cortés Maldonado Benemérita Universidad Autónoma de Puebla, Puebla, Mexico
M. R. Cosentino Lawrence Berkeley National Laboratory, Berkeley, California United States
F. Costa European Organization for Nuclear Research (CERN), Geneva, Switzerland
M. E. Cotallo Centro de Investigaciones Energéticas Medioambientales y Tecnológicas (CIEMAT), Madrid, Spain
E. Crescio Centro de Investigación y de Estudios Avanzados (CINVESTAV), Mexico City and Mérida, Mexico
P. Crochet Laboratoire de Physique Corpusculaire (LPC), Clermont Université, Université Blaise Pascal, CNRS–IN2P3, Clermont-Ferrand, France
E. Cruz Alaniz Instituto de Física, Universidad Nacional Autónoma de México, Mexico City, Mexico
R. Cruz Albino Centro de Investigación y de Estudios Avanzados (CINVESTAV), Mexico City and Mérida, Mexico
E. Cuautle Instituto de Ciencias Nucleares, Universidad Nacional Autónoma de México, Mexico City, Mexico
L. Cunqueiro Laboratori Nazionali di Frascati, INFN, Frascati, Italy
A. Dainese Dipartimento di Fisica e Astronomia dell’Università and Sezione INFN, Padova, Italy Sezione INFN, Padova, Italy
R. Dang Central China Normal University, Wuhan, China
A. Danu Institute of Space Sciences (ISS), Bucharest, Romania
K. Das Saha Institute of Nuclear Physics, Kolkata, India
I. Das Institut de Physique Nucléaire d’Orsay (IPNO), Université Paris-Sud, CNRS-IN2P3, Orsay, France
S. Das Department of Physics and Centre for Astroparticle Physics and Space Science (CAPSS), Bose Institute, Kolkata, India
D. Das Saha Institute of Nuclear Physics, Kolkata, India
S. Dash Indian Institute of Technology Bombay (IIT), Mumbai, India
A. Dash Universidade Estadual de Campinas (UNICAMP), Campinas, Brazil
S. De Variable Energy Cyclotron Centre, Kolkata, India
G. O. V. de Barros Universidade de São Paulo (USP), São Paulo, Brazil
A. De Caro Centro Fermi - Museo Storico della Fisica e Centro Studi e Ricerche “Enrico Fermi”, Rome, Italy Dipartimento di Fisica ‘E.R. Caianiello’ dell’Università and Gruppo Collegato INFN, Salerno, Italy
G. de Cataldo Sezione INFN, Bari, Italy
J. de Cuveland Frankfurt Institute for Advanced Studies, Johann Wolfgang Goethe-Universität Frankfurt, Frankfurt, Germany
A. De Falco Dipartimento di Fisica dell’Università and Sezione INFN, Cagliari, Italy
D. De Gruttola Centro Fermi - Museo Storico della Fisica e Centro Studi e Ricerche “Enrico Fermi”, Rome, Italy Dipartimento di Fisica ‘E.R. Caianiello’ dell’Università and Gruppo Collegato INFN, Salerno, Italy
H. Delagrange SUBATECH, Ecole des Mines de Nantes, Université de Nantes, CNRS-IN2P3, Nantes, France
A. Deloff National Centre for Nuclear Studies, Warsaw, Poland
N. De Marco Sezione INFN, Turin, Italy
E. Dénes Wigner Research Centre for Physics, Hungarian Academy of Sciences, Budapest, Hungary
S. De Pasquale Dipartimento di Fisica ‘E.R. Caianiello’ dell’Università and Gruppo Collegato INFN, Salerno, Italy
A. Deppman Universidade de São Paulo (USP), São Paulo, Brazil
G. D Erasmo Dipartimento Interateneo di Fisica ‘M. Merlin’ and Sezione INFN, Bari, Italy
R. de Rooij Nikhef, National Institute for Subatomic Physics and Institute for Subatomic Physics of Utrecht University, Utrecht, Netherlands
M. A. Diaz Corchero Centro de Investigaciones Energéticas Medioambientales y Tecnológicas (CIEMAT), Madrid, Spain
D. Di Bari Dipartimento Interateneo di Fisica ‘M. Merlin’ and Sezione INFN, Bari, Italy
T. Dietel Institut für Kernphysik, Westfälische Wilhelms-Universität Münster, Münster, Germany
C. Di Giglio Dipartimento Interateneo di Fisica ‘M. Merlin’ and Sezione INFN, Bari, Italy
S. Di Liberto Sezione INFN, Rome, Italy
A. Di Mauro European Organization for Nuclear Research (CERN), Geneva, Switzerland
P. Di Nezza Laboratori Nazionali di Frascati, INFN, Frascati, Italy
R. Divià European Organization for Nuclear Research (CERN), Geneva, Switzerland
Ø. Djuvsland Department of Physics and Technology, University of Bergen, Bergen, Norway
A. Dobrin Division of Experimental High Energy Physics, University of Lund, Lund, Sweden Nikhef, National Institute for Subatomic Physics and Institute for Subatomic Physics of Utrecht University, Utrecht, Netherlands Wayne State University, Detroit, Michigan United States
T. Dobrowolski National Centre for Nuclear Studies, Warsaw, Poland
B. Dönigus Research Division and ExtreMe Matter Institute EMMI, GSI Helmholtzzentrum für Schwerionenforschung, Darmstadt, Germany
O. Dordic Department of Physics, University of Oslo, Oslo, Norway
A. K. Dubey Variable Energy Cyclotron Centre, Kolkata, India
A. Dubla Nikhef, National Institute for Subatomic Physics and Institute for Subatomic Physics of Utrecht University, Utrecht, Netherlands
L. Ducroux Université de Lyon, Université Lyon 1, CNRS/IN2P3, IPN-Lyon, Villeurbanne, France
P. Dupieux Laboratoire de Physique Corpusculaire (LPC), Clermont Université, Université Blaise Pascal, CNRS–IN2P3, Clermont-Ferrand, France
A. K. Dutta Majumdar Saha Institute of Nuclear Physics, Kolkata, India
D. Elia Sezione INFN, Bari, Italy
D. Emschermann Institut für Kernphysik, Westfälische Wilhelms-Universität Münster, Münster, Germany
H. Engel Institut für Informatik, Johann Wolfgang Goethe-Universität Frankfurt, Frankfurt, Germany
B. Erazmus European Organization for Nuclear Research (CERN), Geneva, Switzerland SUBATECH, Ecole des Mines de Nantes, Université de Nantes, CNRS-IN2P3, Nantes, France
H. A. Erdal Faculty of Engineering, Bergen University College, Bergen, Norway
D. Eschweiler Frankfurt Institute for Advanced Studies, Johann Wolfgang Goethe-Universität Frankfurt, Frankfurt, Germany
B. Espagnon Institut de Physique Nucléaire d’Orsay (IPNO), Université Paris-Sud, CNRS-IN2P3, Orsay, France
M. Estienne SUBATECH, Ecole des Mines de Nantes, Université de Nantes, CNRS-IN2P3, Nantes, France
S. Esumi University of Tsukuba, Tsukuba, Japan
D. Evans School of Physics and Astronomy, University of Birmingham, Birmingham, United Kingdom
S. Evdokimov Institute for High Energy Physics, Protvino, Russia
G. Eyyubova Department of Physics, University of Oslo, Oslo, Norway
D. Fabris Dipartimento di Fisica e Astronomia dell’Università and Sezione INFN, Padova, Italy Sezione INFN, Padova, Italy
J. Faivre Laboratoire de Physique Subatomique et de Cosmologie (LPSC), Université Joseph Fourier, CNRS-IN2P3, Institut Polytechnique de Grenoble, Grenoble, France
D. Falchieri Dipartimento di Fisica e Astronomia dell’Università and Sezione INFN, Bologna, Italy
A. Fantoni Laboratori Nazionali di Frascati, INFN, Frascati, Italy
M. Fasel Physikalisches Institut, Ruprecht-Karls-Universität Heidelberg, Heidelberg, Germany
D. Fehlker Department of Physics and Technology, University of Bergen, Bergen, Norway
L. Feldkamp Institut für Kernphysik, Westfälische Wilhelms-Universität Münster, Münster, Germany
D. Felea Institute of Space Sciences (ISS), Bucharest, Romania
A. Feliciello Sezione INFN, Turin, Italy
B. Fenton-Olsen Lawrence Berkeley National Laboratory, Berkeley, California United States
G. Feofilov V. Fock Institute for Physics, St. Petersburg State University, St. Petersburg, Russia
A. Fernández Téllez Benemérita Universidad Autónoma de Puebla, Puebla, Mexico
A. Ferretti Dipartimento di Fisica dell’Università and Sezione INFN, Turin, Italy
A. Festanti Dipartimento di Fisica e Astronomia dell’Università and Sezione INFN, Padova, Italy
J. Figiel The Henryk Niewodniczanski Institute of Nuclear Physics, Polish Academy of Sciences, Cracow, Poland
M. A. S. Figueredo Universidade de São Paulo (USP), São Paulo, Brazil
S. Filchagin Russian Federal Nuclear Center (VNIIEF), Sarov, Russia
D. Finogeev Institute for Nuclear Research, Academy of Sciences, Moscow, Russia
F. M. Fionda Dipartimento Interateneo di Fisica ‘M. Merlin’ and Sezione INFN, Bari, Italy
E. M. Fiore Dipartimento Interateneo di Fisica ‘M. Merlin’ and Sezione INFN, Bari, Italy
E. Floratos Physics Department, University of Athens, Athens, Greece
M. Floris European Organization for Nuclear Research (CERN), Geneva, Switzerland
S. Foertsch Physics Department, University of Cape Town and iThemba LABS, National Research Foundation, Somerset West, South Africa
P. Foka Research Division and ExtreMe Matter Institute EMMI, GSI Helmholtzzentrum für Schwerionenforschung, Darmstadt, Germany
S. Fokin Russian Research Centre Kurchatov Institute, Moscow, Russia
E. Fragiacomo Sezione INFN, Trieste, Italy
A. Francescon Dipartimento di Fisica e Astronomia dell’Università and Sezione INFN, Padova, Italy European Organization for Nuclear Research (CERN), Geneva, Switzerland
U. Frankenfeld Research Division and ExtreMe Matter Institute EMMI, GSI Helmholtzzentrum für Schwerionenforschung, Darmstadt, Germany
U. Fuchs European Organization for Nuclear Research (CERN), Geneva, Switzerland
C. Furget Laboratoire de Physique Subatomique et de Cosmologie (LPSC), Université Joseph Fourier, CNRS-IN2P3, Institut Polytechnique de Grenoble, Grenoble, France
M. Fusco Girard Dipartimento di Fisica ‘E.R. Caianiello’ dell’Università and Gruppo Collegato INFN, Salerno, Italy
J. J. Gaardhøje Niels Bohr Institute, University of Copenhagen, Copenhagen, Denmark
M. Gagliardi Dipartimento di Fisica dell’Università and Sezione INFN, Turin, Italy
A. Gago Sección Física, Departamento de Ciencias, Pontificia Universidad Católica del Perú, Lima, Peru
M. Gallio Dipartimento di Fisica dell’Università and Sezione INFN, Turin, Italy
D. R. Gangadharan Department of Physics, Ohio State University, Columbus, Ohio United States
P. Ganoti Oak Ridge National Laboratory, Oak Ridge, Tennessee United States
C. Garabatos Research Division and ExtreMe Matter Institute EMMI, GSI Helmholtzzentrum für Schwerionenforschung, Darmstadt, Germany
E. Garcia-Solis Chicago State University, Chicago, United States
C. Gargiulo European Organization for Nuclear Research (CERN), Geneva, Switzerland
I. Garishvili Lawrence Livermore National Laboratory, Livermore, California United States
J. Gerhard Frankfurt Institute for Advanced Studies, Johann Wolfgang Goethe-Universität Frankfurt, Frankfurt, Germany
M. Germain SUBATECH, Ecole des Mines de Nantes, Université de Nantes, CNRS-IN2P3, Nantes, France
C. Geuna Commissariat à l’Energie Atomique, IRFU, Saclay, France
M. Gheata European Organization for Nuclear Research (CERN), Geneva, Switzerland Institute of Space Sciences (ISS), Bucharest, Romania
A. Gheata European Organization for Nuclear Research (CERN), Geneva, Switzerland
B. Ghidini Dipartimento Interateneo di Fisica ‘M. Merlin’ and Sezione INFN, Bari, Italy
P. Ghosh Variable Energy Cyclotron Centre, Kolkata, India
P. Gianotti Laboratori Nazionali di Frascati, INFN, Frascati, Italy
P. Giubellino European Organization for Nuclear Research (CERN), Geneva, Switzerland
E. Gladysz-Dziadus The Henryk Niewodniczanski Institute of Nuclear Physics, Polish Academy of Sciences, Cracow, Poland
P. Glässel Physikalisches Institut, Ruprecht-Karls-Universität Heidelberg, Heidelberg, Germany
R. Gomez Centro de Investigación y de Estudios Avanzados (CINVESTAV), Mexico City and Mérida, Mexico Universidad Autónoma de Sinaloa, Culiacán, Mexico
E. G. Ferreiro Departamento de Física de Partículas and IGFAE, Universidad de Santiago de Compostela, Santiago de Compostela, Spain
L. H. González-Trueba Instituto de Física, Universidad Nacional Autónoma de México, Mexico City, Mexico
P. González-Zamora Centro de Investigaciones Energéticas Medioambientales y Tecnológicas (CIEMAT), Madrid, Spain
S. Gorbunov Frankfurt Institute for Advanced Studies, Johann Wolfgang Goethe-Universität Frankfurt, Frankfurt, Germany
A. Goswami Physics Department, University of Rajasthan, Jaipur, India
S. Gotovac Technical University of Split FESB, Split, Croatia
L. K. Graczykowski Warsaw University of Technology, Warsaw, Poland
R. Grajcarek Physikalisches Institut, Ruprecht-Karls-Universität Heidelberg, Heidelberg, Germany
A. Grelli Nikhef, National Institute for Subatomic Physics and Institute for Subatomic Physics of Utrecht University, Utrecht, Netherlands
C. Grigoras European Organization for Nuclear Research (CERN), Geneva, Switzerland
A. Grigoras European Organization for Nuclear Research (CERN), Geneva, Switzerland
V. Grigoriev Moscow Engineering Physics Institute, Moscow, Russia
A. Grigoryan A. I. Alikhanyan National Science Laboratory (Yerevan Physics Institute) Foundation, Yerevan, Armenia
S. Grigoryan Joint Institute for Nuclear Research (JINR), Dubna, Russia
B. Grinyov Bogolyubov Institute for Theoretical Physics, Kiev, Ukraine
N. Grion Sezione INFN, Trieste, Italy
P. Gros Division of Experimental High Energy Physics, University of Lund, Lund, Sweden
J. F. Grosse-Oetringhaus European Organization for Nuclear Research (CERN), Geneva, Switzerland
J.-Y. Grossiord Université de Lyon, Université Lyon 1, CNRS/IN2P3, IPN-Lyon, Villeurbanne, France
R. Grosso European Organization for Nuclear Research (CERN), Geneva, Switzerland
F. Guber Institute for Nuclear Research, Academy of Sciences, Moscow, Russia
R. Guernane Laboratoire de Physique Subatomique et de Cosmologie (LPSC), Université Joseph Fourier, CNRS-IN2P3, Institut Polytechnique de Grenoble, Grenoble, France
B. Guerzoni Dipartimento di Fisica e Astronomia dell’Università and Sezione INFN, Bologna, Italy
M. Guilbaud Université de Lyon, Université Lyon 1, CNRS/IN2P3, IPN-Lyon, Villeurbanne, France
K. Gulbrandsen Niels Bohr Institute, University of Copenhagen, Copenhagen, Denmark
H. Gulkanyan A. I. Alikhanyan National Science Laboratory (Yerevan Physics Institute) Foundation, Yerevan, Armenia
T. Gunji University of Tokyo, Tokyo, Japan
A. Gupta Physics Department, University of Jammu, Jammu, India
R. Gupta Physics Department, University of Jammu, Jammu, India
R. Haake Institut für Kernphysik, Westfälische Wilhelms-Universität Münster, Münster, Germany
Ø. Haaland Department of Physics and Technology, University of Bergen, Bergen, Norway
C. Hadjidakis Institut de Physique Nucléaire d’Orsay (IPNO), Université Paris-Sud, CNRS-IN2P3, Orsay, France
M. Haiduc Institute of Space Sciences (ISS), Bucharest, Romania
H. Hamagaki University of Tokyo, Tokyo, Japan
G. Hamar Wigner Research Centre for Physics, Hungarian Academy of Sciences, Budapest, Hungary
B. H. Han Department of Physics, Sejong University, Seoul, South Korea
L. D. Hanratty School of Physics and Astronomy, University of Birmingham, Birmingham, United Kingdom
A. Hansen Niels Bohr Institute, University of Copenhagen, Copenhagen, Denmark
Z. Harmanová-Tóthová Faculty of Science, P.J. Šafárik University, Košice, Slovakia
J. W. Harris Yale University, New Haven, Connecticut United States
M. Hartig Institut für Kernphysik, Johann Wolfgang Goethe-Universität Frankfurt, Frankfurt, Germany
A. Harton Chicago State University, Chicago, United States
D. Hatzifotiadou Sezione INFN, Bologna, Italy
S. Hayashi University of Tokyo, Tokyo, Japan
A. Hayrapetyan A. I. Alikhanyan National Science Laboratory (Yerevan Physics Institute) Foundation, Yerevan, Armenia European Organization for Nuclear Research (CERN), Geneva, Switzerland
S. T. Heckel Institut für Kernphysik, Johann Wolfgang Goethe-Universität Frankfurt, Frankfurt, Germany
M. Heide Institut für Kernphysik, Westfälische Wilhelms-Universität Münster, Münster, Germany
H. Helstrup Faculty of Engineering, Bergen University College, Bergen, Norway
A. Herghelegiu National Institute for Physics and Nuclear Engineering, Bucharest, Romania
G. Herrera Corral Centro de Investigación y de Estudios Avanzados (CINVESTAV), Mexico City and Mérida, Mexico
N. Herrmann Physikalisches Institut, Ruprecht-Karls-Universität Heidelberg, Heidelberg, Germany
B. A. Hess Eberhard Karls Universität Tübingen, Tübingen, Germany
K. F. Hetland Faculty of Engineering, Bergen University College, Bergen, Norway
B. Hicks Yale University, New Haven, Connecticut United States
B. Hippolyte Institut Pluridisciplinaire Hubert Curien (IPHC), Université de Strasbourg, CNRS-IN2P3, Strasbourg, France
Y. Hori University of Tokyo, Tokyo, Japan
P. Hristov European Organization for Nuclear Research (CERN), Geneva, Switzerland
I. Hřivnáčová Institut de Physique Nucléaire d’Orsay (IPNO), Université Paris-Sud, CNRS-IN2P3, Orsay, France
M. Huang Department of Physics and Technology, University of Bergen, Bergen, Norway
T. J. Humanic Department of Physics, Ohio State University, Columbus, Ohio United States
D. S. Hwang Department of Physics, Sejong University, Seoul, South Korea
R. Ichou Laboratoire de Physique Corpusculaire (LPC), Clermont Université, Université Blaise Pascal, CNRS–IN2P3, Clermont-Ferrand, France
R. Ilkaev Russian Federal Nuclear Center (VNIIEF), Sarov, Russia
I. Ilkiv National Centre for Nuclear Studies, Warsaw, Poland
M. Inaba University of Tsukuba, Tsukuba, Japan
E. Incani Dipartimento di Fisica dell’Università and Sezione INFN, Cagliari, Italy
G. M. Innocenti Dipartimento di Fisica dell’Università and Sezione INFN, Turin, Italy
P. G. Innocenti European Organization for Nuclear Research (CERN), Geneva, Switzerland
M. Ippolitov Russian Research Centre Kurchatov Institute, Moscow, Russia
M. Irfan Department of Physics, Aligarh Muslim University, Aligarh, India
C. Ivan Research Division and ExtreMe Matter Institute EMMI, GSI Helmholtzzentrum für Schwerionenforschung, Darmstadt, Germany
M. Ivanov Research Division and ExtreMe Matter Institute EMMI, GSI Helmholtzzentrum für Schwerionenforschung, Darmstadt, Germany
A. Ivanov V. Fock Institute for Physics, St. Petersburg State University, St. Petersburg, Russia
V. Ivanov Petersburg Nuclear Physics Institute, Gatchina, Russia
O. Ivanytskyi Bogolyubov Institute for Theoretical Physics, Kiev, Ukraine
A. Jachołkowski Dipartimento di Fisica e Astronomia dell’Università and Sezione INFN, Catania, Italy
P. M. Jacobs Lawrence Berkeley National Laboratory, Berkeley, California United States
C. Jahnke Universidade de São Paulo (USP), São Paulo, Brazil
H. J. Jang Korea Institute of Science and Technology Information, Daejeon, South Korea
M. A. Janik Warsaw University of Technology, Warsaw, Poland
P. H. S. Y. Jayarathna University of Houston, Houston, Texas United States
S. Jena Indian Institute of Technology Bombay (IIT), Mumbai, India
D. M. Jha Wayne State University, Detroit, Michigan United States
R. T. Jimenez Bustamante Instituto de Ciencias Nucleares, Universidad Nacional Autónoma de México, Mexico City, Mexico
P. G. Jones School of Physics and Astronomy, University of Birmingham, Birmingham, United Kingdom
H. Jung Gangneung-Wonju National University, Gangneung, South Korea
A. Jusko School of Physics and Astronomy, University of Birmingham, Birmingham, United Kingdom
A. B. Kaidalov Institute for Theoretical and Experimental Physics, Moscow, Russia
S. Kalcher Frankfurt Institute for Advanced Studies, Johann Wolfgang Goethe-Universität Frankfurt, Frankfurt, Germany
P. Kaliňák Institute of Experimental Physics, Slovak Academy of Sciences, Košice, Slovakia
T. Kalliokoski Helsinki Institute of Physics (HIP) and University of Jyväskylä, Jyväskylä, Finland
A. Kalweit European Organization for Nuclear Research (CERN), Geneva, Switzerland
J. H. Kang Yonsei University, Seoul, South Korea
V. Kaplin Moscow Engineering Physics Institute, Moscow, Russia
S. Kar Variable Energy Cyclotron Centre, Kolkata, India
A. Karasu Uysal European Organization for Nuclear Research (CERN), Geneva, Switzerland KTO Karatay University, Konya, Turkey Yildiz Technical University, Istanbul, Turkey
O. Karavichev Institute for Nuclear Research, Academy of Sciences, Moscow, Russia
T. Karavicheva Institute for Nuclear Research, Academy of Sciences, Moscow, Russia
E. Karpechev Institute for Nuclear Research, Academy of Sciences, Moscow, Russia
A. Kazantsev Russian Research Centre Kurchatov Institute, Moscow, Russia
U. Kebschull Institut für Informatik, Johann Wolfgang Goethe-Universität Frankfurt, Frankfurt, Germany
R. Keidel Zentrum für Technologietransfer und Telekommunikation (ZTT), Fachhochschule Worms, Worms, Germany
B. Ketzer Institut für Kernphysik, Johann Wolfgang Goethe-Universität Frankfurt, Frankfurt, Germany Technische Universität München, Munich, Germany
M. M. Khan Department of Physics, Aligarh Muslim University, Aligarh, India
P. Khan Saha Institute of Nuclear Physics, Kolkata, India
S. A. Khan Variable Energy Cyclotron Centre, Kolkata, India
K. H. Khan COMSATS Institute of Information Technology (CIIT), Islamabad, Pakistan
A. Khanzadeev Petersburg Nuclear Physics Institute, Gatchina, Russia
Y. Kharlov Institute for High Energy Physics, Protvino, Russia
B. Kileng Faculty of Engineering, Bergen University College, Bergen, Norway
M. Kim Yonsei University, Seoul, South Korea
T. Kim Yonsei University, Seoul, South Korea
B. Kim Yonsei University, Seoul, South Korea
S. Kim Department of Physics, Sejong University, Seoul, South Korea
M. Kim Gangneung-Wonju National University, Gangneung, South Korea
D. J. Kim Helsinki Institute of Physics (HIP) and University of Jyväskylä, Jyväskylä, Finland
J. S. Kim Gangneung-Wonju National University, Gangneung, South Korea
J. H. Kim Department of Physics, Sejong University, Seoul, South Korea
D. W. Kim Gangneung-Wonju National University, Gangneung, South Korea Korea Institute of Science and Technology Information, Daejeon, South Korea
S. Kirsch Frankfurt Institute for Advanced Studies, Johann Wolfgang Goethe-Universität Frankfurt, Frankfurt, Germany
I. Kisel Frankfurt Institute for Advanced Studies, Johann Wolfgang Goethe-Universität Frankfurt, Frankfurt, Germany
S. Kiselev Institute for Theoretical and Experimental Physics, Moscow, Russia
A. Kisiel Warsaw University of Technology, Warsaw, Poland
J. L. Klay California Polytechnic State University, San Luis Obispo, California United States
J. Klein Physikalisches Institut, Ruprecht-Karls-Universität Heidelberg, Heidelberg, Germany
C. Klein-Bösing Institut für Kernphysik, Westfälische Wilhelms-Universität Münster, Münster, Germany
M. Kliemant Institut für Kernphysik, Johann Wolfgang Goethe-Universität Frankfurt, Frankfurt, Germany
A. Kluge European Organization for Nuclear Research (CERN), Geneva, Switzerland
M. L. Knichel Research Division and ExtreMe Matter Institute EMMI, GSI Helmholtzzentrum für Schwerionenforschung, Darmstadt, Germany
A. G. Knospe Physics Department, The University of Texas at Austin, Austin, TX United States
M. K. Köhler Research Division and ExtreMe Matter Institute EMMI, GSI Helmholtzzentrum für Schwerionenforschung, Darmstadt, Germany
T. Kollegger Frankfurt Institute for Advanced Studies, Johann Wolfgang Goethe-Universität Frankfurt, Frankfurt, Germany
A. Kolojvari V. Fock Institute for Physics, St. Petersburg State University, St. Petersburg, Russia
M. Kompaniets V. Fock Institute for Physics, St. Petersburg State University, St. Petersburg, Russia
V. Kondratiev V. Fock Institute for Physics, St. Petersburg State University, St. Petersburg, Russia
N. Kondratyeva Moscow Engineering Physics Institute, Moscow, Russia
A. Konevskikh Institute for Nuclear Research, Academy of Sciences, Moscow, Russia
V. Kovalenko V. Fock Institute for Physics, St. Petersburg State University, St. Petersburg, Russia
M. Kowalski The Henryk Niewodniczanski Institute of Nuclear Physics, Polish Academy of Sciences, Cracow, Poland
S. Kox Laboratoire de Physique Subatomique et de Cosmologie (LPSC), Université Joseph Fourier, CNRS-IN2P3, Institut Polytechnique de Grenoble, Grenoble, France
G. Koyithatta Meethaleveedu Indian Institute of Technology Bombay (IIT), Mumbai, India
J. Kral Helsinki Institute of Physics (HIP) and University of Jyväskylä, Jyväskylä, Finland
I. Králik Institute of Experimental Physics, Slovak Academy of Sciences, Košice, Slovakia
F. Kramer Institut für Kernphysik, Johann Wolfgang Goethe-Universität Frankfurt, Frankfurt, Germany
A. Kravčáková Faculty of Science, P.J. Šafárik University, Košice, Slovakia
M. Krelina Faculty of Nuclear Sciences and Physical Engineering, Czech Technical University in Prague, Prague, Czech Republic
M. Kretz Frankfurt Institute for Advanced Studies, Johann Wolfgang Goethe-Universität Frankfurt, Frankfurt, Germany
M. Krivda Institute of Experimental Physics, Slovak Academy of Sciences, Košice, Slovakia School of Physics and Astronomy, University of Birmingham, Birmingham, United Kingdom
F. Krizek Helsinki Institute of Physics (HIP) and University of Jyväskylä, Jyväskylä, Finland
M. Krus Faculty of Nuclear Sciences and Physical Engineering, Czech Technical University in Prague, Prague, Czech Republic
E. Kryshen Petersburg Nuclear Physics Institute, Gatchina, Russia
M. Krzewicki Research Division and ExtreMe Matter Institute EMMI, GSI Helmholtzzentrum für Schwerionenforschung, Darmstadt, Germany
V. Kucera Nuclear Physics Institute, Academy of Sciences of the Czech Republic, Řež u Prahy, Czech Republic
Y. Kucheriaev Russian Research Centre Kurchatov Institute, Moscow, Russia
T. Kugathasan European Organization for Nuclear Research (CERN), Geneva, Switzerland
C. Kuhn Institut Pluridisciplinaire Hubert Curien (IPHC), Université de Strasbourg, CNRS-IN2P3, Strasbourg, France
P. G. Kuijer Nikhef, National Institute for Subatomic Physics, Amsterdam, Netherlands
I. Kulakov Institut für Kernphysik, Johann Wolfgang Goethe-Universität Frankfurt, Frankfurt, Germany
J. Kumar Indian Institute of Technology Bombay (IIT), Mumbai, India
P. Kurashvili National Centre for Nuclear Studies, Warsaw, Poland
A. Kurepin Institute for Nuclear Research, Academy of Sciences, Moscow, Russia
A. B. Kurepin Institute for Nuclear Research, Academy of Sciences, Moscow, Russia
A. Kuryakin Russian Federal Nuclear Center (VNIIEF), Sarov, Russia
V. Kushpil Nuclear Physics Institute, Academy of Sciences of the Czech Republic, Řež u Prahy, Czech Republic
S. Kushpil Nuclear Physics Institute, Academy of Sciences of the Czech Republic, Řež u Prahy, Czech Republic
H. Kvaerno Department of Physics, University of Oslo, Oslo, Norway
M. J. Kweon Physikalisches Institut, Ruprecht-Karls-Universität Heidelberg, Heidelberg, Germany
Y. Kwon Yonsei University, Seoul, South Korea
P. Ladrón de Guevara Instituto de Ciencias Nucleares, Universidad Nacional Autónoma de México, Mexico City, Mexico
C. Lagana Fernandes Universidade de São Paulo (USP), São Paulo, Brazil
I. Lakomov Institut de Physique Nucléaire d’Orsay (IPNO), Université Paris-Sud, CNRS-IN2P3, Orsay, France
R. Langoy Department of Physics and Technology, University of Bergen, Bergen, Norway Vestfold University College, Tonsberg, Norway
S. L. La Pointe Nikhef, National Institute for Subatomic Physics and Institute for Subatomic Physics of Utrecht University, Utrecht, Netherlands
C. Lara Institut für Informatik, Johann Wolfgang Goethe-Universität Frankfurt, Frankfurt, Germany
A. Lardeux SUBATECH, Ecole des Mines de Nantes, Université de Nantes, CNRS-IN2P3, Nantes, France
P. La Rocca Dipartimento di Fisica e Astronomia dell’Università and Sezione INFN, Catania, Italy
R. Lea Dipartimento di Fisica dell’Università and Sezione INFN, Trieste, Italy
M. Lechman European Organization for Nuclear Research (CERN), Geneva, Switzerland
S. C. Lee Gangneung-Wonju National University, Gangneung, South Korea
G. R. Lee School of Physics and Astronomy, University of Birmingham, Birmingham, United Kingdom
I. Legrand European Organization for Nuclear Research (CERN), Geneva, Switzerland
J. Lehnert Institut für Kernphysik, Johann Wolfgang Goethe-Universität Frankfurt, Frankfurt, Germany
R. C. Lemmon Nuclear Physics Group, STFC Daresbury Laboratory, Daresbury, United Kingdom
M. Lenhardt Research Division and ExtreMe Matter Institute EMMI, GSI Helmholtzzentrum für Schwerionenforschung, Darmstadt, Germany
V. Lenti Sezione INFN, Bari, Italy
H. León Instituto de Física, Universidad Nacional Autónoma de México, Mexico City, Mexico
M. Leoncino Dipartimento di Fisica dell’Università and Sezione INFN, Turin, Italy
I. León Monzón Universidad Autónoma de Sinaloa, Culiacán, Mexico
P. Lévai Wigner Research Centre for Physics, Hungarian Academy of Sciences, Budapest, Hungary
S. Li Central China Normal University, Wuhan, China Laboratoire de Physique Corpusculaire (LPC), Clermont Université, Université Blaise Pascal, CNRS–IN2P3, Clermont-Ferrand, France
J. Lien Department of Physics and Technology, University of Bergen, Bergen, Norway Vestfold University College, Tonsberg, Norway
R. Lietava School of Physics and Astronomy, University of Birmingham, Birmingham, United Kingdom
S. Lindal Department of Physics, University of Oslo, Oslo, Norway
V. Lindenstruth Frankfurt Institute for Advanced Studies, Johann Wolfgang Goethe-Universität Frankfurt, Frankfurt, Germany
C. Lippmann European Organization for Nuclear Research (CERN), Geneva, Switzerland Research Division and ExtreMe Matter Institute EMMI, GSI Helmholtzzentrum für Schwerionenforschung, Darmstadt, Germany
M. A. Lisa Department of Physics, Ohio State University, Columbus, Ohio United States
H. M. Ljunggren Division of Experimental High Energy Physics, University of Lund, Lund, Sweden
D. F. Lodato Nikhef, National Institute for Subatomic Physics and Institute for Subatomic Physics of Utrecht University, Utrecht, Netherlands
P. I. Loenne Department of Physics and Technology, University of Bergen, Bergen, Norway
V. R. Loggins Wayne State University, Detroit, Michigan United States
V. Loginov Moscow Engineering Physics Institute, Moscow, Russia
D. Lohner Physikalisches Institut, Ruprecht-Karls-Universität Heidelberg, Heidelberg, Germany
C. Loizides Lawrence Berkeley National Laboratory, Berkeley, California United States
K. K. Loo Helsinki Institute of Physics (HIP) and University of Jyväskylä, Jyväskylä, Finland
X. Lopez Laboratoire de Physique Corpusculaire (LPC), Clermont Université, Université Blaise Pascal, CNRS–IN2P3, Clermont-Ferrand, France
E. López Torres Centro de Aplicaciones Tecnológicas y Desarrollo Nuclear (CEADEN), Havana, Cuba
G. Løvhøiden Department of Physics, University of Oslo, Oslo, Norway
X.-G. Lu Physikalisches Institut, Ruprecht-Karls-Universität Heidelberg, Heidelberg, Germany
P. Luettig Institut für Kernphysik, Johann Wolfgang Goethe-Universität Frankfurt, Frankfurt, Germany
M. Lunardon Dipartimento di Fisica e Astronomia dell’Università and Sezione INFN, Padova, Italy
J. Luo Central China Normal University, Wuhan, China
G. Luparello Nikhef, National Institute for Subatomic Physics and Institute for Subatomic Physics of Utrecht University, Utrecht, Netherlands
C. Luzzi European Organization for Nuclear Research (CERN), Geneva, Switzerland
R. Ma Yale University, New Haven, Connecticut United States
K. Ma Central China Normal University, Wuhan, China
D. M. Madagodahettige-Don University of Houston, Houston, Texas United States
A. Maevskaya Institute for Nuclear Research, Academy of Sciences, Moscow, Russia
M. Mager European Organization for Nuclear Research (CERN), Geneva, Switzerland Institut für Kernphysik, Technische Universität Darmstadt, Darmstadt, Germany
D. P. Mahapatra Institute of Physics, Bhubaneswar, India
A. Maire Physikalisches Institut, Ruprecht-Karls-Universität Heidelberg, Heidelberg, Germany
M. Malaev Petersburg Nuclear Physics Institute, Gatchina, Russia
I. Maldonado Cervantes Instituto de Ciencias Nucleares, Universidad Nacional Autónoma de México, Mexico City, Mexico
L. Malinina Joint Institute for Nuclear Research (JINR), Dubna, Russia
D. Mal’Kevich Institute for Theoretical and Experimental Physics, Moscow, Russia
P. Malzacher Research Division and ExtreMe Matter Institute EMMI, GSI Helmholtzzentrum für Schwerionenforschung, Darmstadt, Germany
A. Mamonov Russian Federal Nuclear Center (VNIIEF), Sarov, Russia
L. Manceau Sezione INFN, Turin, Italy
L. Mangotra Physics Department, University of Jammu, Jammu, India
V. Manko Russian Research Centre Kurchatov Institute, Moscow, Russia
F. Manso Laboratoire de Physique Corpusculaire (LPC), Clermont Université, Université Blaise Pascal, CNRS–IN2P3, Clermont-Ferrand, France
V. Manzari Sezione INFN, Bari, Italy
Y. Mao Central China Normal University, Wuhan, China
M. Marchisone Dipartimento di Fisica dell’Università and Sezione INFN, Turin, Italy Laboratoire de Physique Corpusculaire (LPC), Clermont Université, Université Blaise Pascal, CNRS–IN2P3, Clermont-Ferrand, France
J. Mareš Institute of Physics, Academy of Sciences of the Czech Republic, Prague, Czech Republic
G. V. Margagliotti Dipartimento di Fisica dell’Università and Sezione INFN, Trieste, Italy Sezione INFN, Trieste, Italy
A. Margotti Sezione INFN, Bologna, Italy
A. Marín Research Division and ExtreMe Matter Institute EMMI, GSI Helmholtzzentrum für Schwerionenforschung, Darmstadt, Germany
C. Markert Physics Department, The University of Texas at Austin, Austin, TX United States
M. Marquard Institut für Kernphysik, Johann Wolfgang Goethe-Universität Frankfurt, Frankfurt, Germany
I. Martashvili University of Tennessee, Knoxville, Tennessee United States
N. A. Martin Research Division and ExtreMe Matter Institute EMMI, GSI Helmholtzzentrum für Schwerionenforschung, Darmstadt, Germany
P. Martinengo European Organization for Nuclear Research (CERN), Geneva, Switzerland
M. I. Martínez Benemérita Universidad Autónoma de Puebla, Puebla, Mexico
G. Martínez García SUBATECH, Ecole des Mines de Nantes, Université de Nantes, CNRS-IN2P3, Nantes, France
Y. Martynov Bogolyubov Institute for Theoretical Physics, Kiev, Ukraine
A. Mas SUBATECH, Ecole des Mines de Nantes, Université de Nantes, CNRS-IN2P3, Nantes, France
S. Masciocchi Research Division and ExtreMe Matter Institute EMMI, GSI Helmholtzzentrum für Schwerionenforschung, Darmstadt, Germany
M. Masera Dipartimento di Fisica dell’Università and Sezione INFN, Turin, Italy
A. Masoni Sezione INFN, Cagliari, Italy
L. Massacrier SUBATECH, Ecole des Mines de Nantes, Université de Nantes, CNRS-IN2P3, Nantes, France
A. Mastroserio Dipartimento Interateneo di Fisica ‘M. Merlin’ and Sezione INFN, Bari, Italy
A. Matyja The Henryk Niewodniczanski Institute of Nuclear Physics, Polish Academy of Sciences, Cracow, Poland
C. Mayer The Henryk Niewodniczanski Institute of Nuclear Physics, Polish Academy of Sciences, Cracow, Poland
J. Mazer University of Tennessee, Knoxville, Tennessee United States
R. Mazumder Indian Institute of Technology Indore (IITI), Indore, India
M. A. Mazzoni Sezione INFN, Rome, Italy
F. Meddi Dipartimento di Fisica dell’Università ‘La Sapienza’ and Sezione INFN, Rome, Italy
A. Menchaca-Rocha Instituto de Física, Universidad Nacional Autónoma de México, Mexico City, Mexico
J. Mercado Pérez Physikalisches Institut, Ruprecht-Karls-Universität Heidelberg, Heidelberg, Germany
M. Meres Faculty of Mathematics, Physics and Informatics, Comenius University, Bratislava, Slovakia
Y. Miake University of Tsukuba, Tsukuba, Japan
K. Mikhaylov Institute for Theoretical and Experimental Physics, Moscow, Russia Joint Institute for Nuclear Research (JINR), Dubna, Russia
L. Milano Dipartimento di Fisica dell’Università and Sezione INFN, Turin, Italy European Organization for Nuclear Research (CERN), Geneva, Switzerland
J. Milosevic Department of Physics, University of Oslo, Oslo, Norway
A. Mischke Nikhef, National Institute for Subatomic Physics and Institute for Subatomic Physics of Utrecht University, Utrecht, Netherlands
A. N. Mishra Indian Institute of Technology Indore (IITI), Indore, India Physics Department, University of Rajasthan, Jaipur, India
D. Miśkowiec Research Division and ExtreMe Matter Institute EMMI, GSI Helmholtzzentrum für Schwerionenforschung, Darmstadt, Germany
C. Mitu Institute of Space Sciences (ISS), Bucharest, Romania
S. Mizuno University of Tsukuba, Tsukuba, Japan
J. Mlynarz Wayne State University, Detroit, Michigan United States
B. Mohanty National Institute of Science Education and Research, Bhubaneswar, India Variable Energy Cyclotron Centre, Kolkata, India
L. Molnar Institut Pluridisciplinaire Hubert Curien (IPHC), Université de Strasbourg, CNRS-IN2P3, Strasbourg, France Wigner Research Centre for Physics, Hungarian Academy of Sciences, Budapest, Hungary
L. Montaño Zetina Centro de Investigación y de Estudios Avanzados (CINVESTAV), Mexico City and Mérida, Mexico
M. Monteno Sezione INFN, Turin, Italy
E. Montes Centro de Investigaciones Energéticas Medioambientales y Tecnológicas (CIEMAT), Madrid, Spain
T. Moon Yonsei University, Seoul, South Korea
M. Morando Dipartimento di Fisica e Astronomia dell’Università and Sezione INFN, Padova, Italy
D. A. Moreira De Godoy Universidade de São Paulo (USP), São Paulo, Brazil
S. Moretto Dipartimento di Fisica e Astronomia dell’Università and Sezione INFN, Padova, Italy
A. Morreale Helsinki Institute of Physics (HIP) and University of Jyväskylä, Jyväskylä, Finland
A. Morsch European Organization for Nuclear Research (CERN), Geneva, Switzerland
V. Muccifora Laboratori Nazionali di Frascati, INFN, Frascati, Italy
E. Mudnic Technical University of Split FESB, Split, Croatia
S. Muhuri Variable Energy Cyclotron Centre, Kolkata, India
M. Mukherjee Variable Energy Cyclotron Centre, Kolkata, India
H. Müller European Organization for Nuclear Research (CERN), Geneva, Switzerland
M. G. Munhoz Universidade de São Paulo (USP), São Paulo, Brazil
S. Murray Physics Department, University of Cape Town and iThemba LABS, National Research Foundation, Somerset West, South Africa
L. Musa European Organization for Nuclear Research (CERN), Geneva, Switzerland
J. Musinsky Institute of Experimental Physics, Slovak Academy of Sciences, Košice, Slovakia
B. K. Nandi Indian Institute of Technology Bombay (IIT), Mumbai, India
R. Nania Sezione INFN, Bologna, Italy
E. Nappi Sezione INFN, Bari, Italy
C. Nattrass University of Tennessee, Knoxville, Tennessee United States
T. K. Nayak Variable Energy Cyclotron Centre, Kolkata, India
S. Nazarenko Russian Federal Nuclear Center (VNIIEF), Sarov, Russia
A. Nedosekin Institute for Theoretical and Experimental Physics, Moscow, Russia
M. Nicassio Dipartimento Interateneo di Fisica ‘M. Merlin’ and Sezione INFN, Bari, Italy Research Division and ExtreMe Matter Institute EMMI, GSI Helmholtzzentrum für Schwerionenforschung, Darmstadt, Germany
M. Niculescu European Organization for Nuclear Research (CERN), Geneva, Switzerland Institute of Space Sciences (ISS), Bucharest, Romania
B. S. Nielsen Niels Bohr Institute, University of Copenhagen, Copenhagen, Denmark
T. Niida University of Tsukuba, Tsukuba, Japan
S. Nikolaev Russian Research Centre Kurchatov Institute, Moscow, Russia
V. Nikolic Rudjer Bošković Institute, Zagreb, Croatia
S. Nikulin Russian Research Centre Kurchatov Institute, Moscow, Russia
V. Nikulin Petersburg Nuclear Physics Institute, Gatchina, Russia
B. S. Nilsen Physics Department, Creighton University, Omaha, Nebraska United States
M. S. Nilsson Department of Physics, University of Oslo, Oslo, Norway
F. Noferini Centro Fermi - Museo Storico della Fisica e Centro Studi e Ricerche “Enrico Fermi”, Rome, Italy Sezione INFN, Bologna, Italy
P. Nomokonov Joint Institute for Nuclear Research (JINR), Dubna, Russia
G. Nooren Nikhef, National Institute for Subatomic Physics and Institute for Subatomic Physics of Utrecht University, Utrecht, Netherlands
A. Nyanin Russian Research Centre Kurchatov Institute, Moscow, Russia
A. Nyatha Indian Institute of Technology Bombay (IIT), Mumbai, India
C. Nygaard Niels Bohr Institute, University of Copenhagen, Copenhagen, Denmark
J. Nystrand Department of Physics and Technology, University of Bergen, Bergen, Norway
A. Ochirov V. Fock Institute for Physics, St. Petersburg State University, St. Petersburg, Russia
H. Oeschler European Organization for Nuclear Research (CERN), Geneva, Switzerland Institut für Kernphysik, Technische Universität Darmstadt, Darmstadt, Germany Physikalisches Institut, Ruprecht-Karls-Universität Heidelberg, Heidelberg, Germany
S. Oh Yale University, New Haven, Connecticut United States
S. K. Oh Gangneung-Wonju National University, Gangneung, South Korea
J. Oleniacz Warsaw University of Technology, Warsaw, Poland
A. C. Oliveira Da Silva Universidade de São Paulo (USP), São Paulo, Brazil
J. Onderwaater Research Division and ExtreMe Matter Institute EMMI, GSI Helmholtzzentrum für Schwerionenforschung, Darmstadt, Germany
C. Oppedisano Sezione INFN, Turin, Italy
A. Ortiz Velasquez Division of Experimental High Energy Physics, University of Lund, Lund, Sweden Instituto de Ciencias Nucleares, Universidad Nacional Autónoma de México, Mexico City, Mexico
A. Oskarsson Division of Experimental High Energy Physics, University of Lund, Lund, Sweden
P. Ostrowski Warsaw University of Technology, Warsaw, Poland
J. Otwinowski Research Division and ExtreMe Matter Institute EMMI, GSI Helmholtzzentrum für Schwerionenforschung, Darmstadt, Germany
K. Oyama Physikalisches Institut, Ruprecht-Karls-Universität Heidelberg, Heidelberg, Germany
K. Ozawa University of Tokyo, Tokyo, Japan
Y. Pachmayer Physikalisches Institut, Ruprecht-Karls-Universität Heidelberg, Heidelberg, Germany
M. Pachr Faculty of Nuclear Sciences and Physical Engineering, Czech Technical University in Prague, Prague, Czech Republic
F. Padilla Dipartimento di Fisica dell’Università and Sezione INFN, Turin, Italy
P. Pagano Dipartimento di Fisica ‘E.R. Caianiello’ dell’Università and Gruppo Collegato INFN, Salerno, Italy
G. Paić Instituto de Ciencias Nucleares, Universidad Nacional Autónoma de México, Mexico City, Mexico
F. Painke Frankfurt Institute for Advanced Studies, Johann Wolfgang Goethe-Universität Frankfurt, Frankfurt, Germany
C. Pajares Departamento de Física de Partículas and IGFAE, Universidad de Santiago de Compostela, Santiago de Compostela, Spain
S. K. Pal Variable Energy Cyclotron Centre, Kolkata, India
A. Palaha School of Physics and Astronomy, University of Birmingham, Birmingham, United Kingdom
A. Palmeri Sezione INFN, Catania, Italy
V. Papikyan A. I. Alikhanyan National Science Laboratory (Yerevan Physics Institute) Foundation, Yerevan, Armenia
G. S. Pappalardo Sezione INFN, Catania, Italy
W. J. Park Research Division and ExtreMe Matter Institute EMMI, GSI Helmholtzzentrum für Schwerionenforschung, Darmstadt, Germany
A. Passfeld Institut für Kernphysik, Westfälische Wilhelms-Universität Münster, Münster, Germany
D. I. Patalakha Institute for High Energy Physics, Protvino, Russia
V. Paticchio Sezione INFN, Bari, Italy
B. Paul Saha Institute of Nuclear Physics, Kolkata, India
A. Pavlinov Wayne State University, Detroit, Michigan United States
T. Pawlak Warsaw University of Technology, Warsaw, Poland
T. Peitzmann Nikhef, National Institute for Subatomic Physics and Institute for Subatomic Physics of Utrecht University, Utrecht, Netherlands
H. Pereira Da Costa Commissariat à l’Energie Atomique, IRFU, Saclay, France
E. Pereira De Oliveira Filho Universidade de São Paulo (USP), São Paulo, Brazil
D. Peresunko Russian Research Centre Kurchatov Institute, Moscow, Russia
C. E. Pérez Lara Nikhef, National Institute for Subatomic Physics, Amsterdam, Netherlands
D. Perrino Dipartimento Interateneo di Fisica ‘M. Merlin’ and Sezione INFN, Bari, Italy
W. Peryt Warsaw University of Technology, Warsaw, Poland
A. Pesci Sezione INFN, Bologna, Italy
Y. Pestov Budker Institute for Nuclear Physics, Novosibirsk, Russia
V. Petráček Faculty of Nuclear Sciences and Physical Engineering, Czech Technical University in Prague, Prague, Czech Republic
M. Petran Faculty of Nuclear Sciences and Physical Engineering, Czech Technical University in Prague, Prague, Czech Republic
M. Petris National Institute for Physics and Nuclear Engineering, Bucharest, Romania
P. Petrov School of Physics and Astronomy, University of Birmingham, Birmingham, United Kingdom
M. Petrovici National Institute for Physics and Nuclear Engineering, Bucharest, Romania
C. Petta Dipartimento di Fisica e Astronomia dell’Università and Sezione INFN, Catania, Italy
S. Piano Sezione INFN, Trieste, Italy
M. Pikna Faculty of Mathematics, Physics and Informatics, Comenius University, Bratislava, Slovakia
P. Pillot SUBATECH, Ecole des Mines de Nantes, Université de Nantes, CNRS-IN2P3, Nantes, France
O. Pinazza European Organization for Nuclear Research (CERN), Geneva, Switzerland
L. Pinsky University of Houston, Houston, Texas United States
N. Pitz Institut für Kernphysik, Johann Wolfgang Goethe-Universität Frankfurt, Frankfurt, Germany
D. B. Piyarathna University of Houston, Houston, Texas United States
M. Planinic Rudjer Bošković Institute, Zagreb, Croatia
M. Płoskoń Lawrence Berkeley National Laboratory, Berkeley, California United States
J. Pluta Warsaw University of Technology, Warsaw, Poland
T. Pocheptsov Joint Institute for Nuclear Research (JINR), Dubna, Russia
S. Pochybova Wigner Research Centre for Physics, Hungarian Academy of Sciences, Budapest, Hungary
P. L. M. Podesta-Lerma Universidad Autónoma de Sinaloa, Culiacán, Mexico
M. G. Poghosyan European Organization for Nuclear Research (CERN), Geneva, Switzerland
K. Polák Institute of Physics, Academy of Sciences of the Czech Republic, Prague, Czech Republic
B. Polichtchouk Institute for High Energy Physics, Protvino, Russia
N. Poljak Nikhef, National Institute for Subatomic Physics and Institute for Subatomic Physics of Utrecht University, Utrecht, Netherlands Rudjer Bošković Institute, Zagreb, Croatia
A. Pop National Institute for Physics and Nuclear Engineering, Bucharest, Romania
S. Porteboeuf-Houssais Laboratoire de Physique Corpusculaire (LPC), Clermont Université, Université Blaise Pascal, CNRS–IN2P3, Clermont-Ferrand, France
V. Pospíšil Faculty of Nuclear Sciences and Physical Engineering, Czech Technical University in Prague, Prague, Czech Republic
B. Potukuchi Physics Department, University of Jammu, Jammu, India
S. K. Prasad Wayne State University, Detroit, Michigan United States
R. Preghenella Centro Fermi - Museo Storico della Fisica e Centro Studi e Ricerche “Enrico Fermi”, Rome, Italy Sezione INFN, Bologna, Italy
F. Prino Sezione INFN, Turin, Italy
C. A. Pruneau Wayne State University, Detroit, Michigan United States
I. Pshenichnov Institute for Nuclear Research, Academy of Sciences, Moscow, Russia
G. Puddu Dipartimento di Fisica dell’Università and Sezione INFN, Cagliari, Italy
V. Punin Russian Federal Nuclear Center (VNIIEF), Sarov, Russia
J. Putschke Wayne State University, Detroit, Michigan United States
H. Qvigstad Department of Physics, University of Oslo, Oslo, Norway
A. Rachevski Sezione INFN, Trieste, Italy
A. Rademakers European Organization for Nuclear Research (CERN), Geneva, Switzerland
T. S. Räihä Helsinki Institute of Physics (HIP) and University of Jyväskylä, Jyväskylä, Finland
J. Rak Helsinki Institute of Physics (HIP) and University of Jyväskylä, Jyväskylä, Finland
A. Rakotozafindrabe Commissariat à l’Energie Atomique, IRFU, Saclay, France
L. Ramello Dipartimento di Scienze e Innovazione Tecnologica dell’Università del Piemonte Orientale and Gruppo Collegato INFN, Alessandria, Italy
S. Raniwala Physics Department, University of Rajasthan, Jaipur, India
R. Raniwala Physics Department, University of Rajasthan, Jaipur, India
S. S. Räsänen Helsinki Institute of Physics (HIP) and University of Jyväskylä, Jyväskylä, Finland
B. T. Rascanu Institut für Kernphysik, Johann Wolfgang Goethe-Universität Frankfurt, Frankfurt, Germany
D. Rathee Physics Department, Panjab University, Chandigarh, India
W. Rauch European Organization for Nuclear Research (CERN), Geneva, Switzerland
A. W. Rauf COMSATS Institute of Information Technology (CIIT), Islamabad, Pakistan
V. Razazi Dipartimento di Fisica dell’Università and Sezione INFN, Cagliari, Italy
K. F. Read University of Tennessee, Knoxville, Tennessee United States
J. S. Real Laboratoire de Physique Subatomique et de Cosmologie (LPSC), Université Joseph Fourier, CNRS-IN2P3, Institut Polytechnique de Grenoble, Grenoble, France
K. Redlich National Centre for Nuclear Studies, Warsaw, Poland
R. J. Reed Yale University, New Haven, Connecticut United States
A. Rehman Department of Physics and Technology, University of Bergen, Bergen, Norway
P. Reichelt Institut für Kernphysik, Johann Wolfgang Goethe-Universität Frankfurt, Frankfurt, Germany
M. Reicher Nikhef, National Institute for Subatomic Physics and Institute for Subatomic Physics of Utrecht University, Utrecht, Netherlands
R. Renfordt Institut für Kernphysik, Johann Wolfgang Goethe-Universität Frankfurt, Frankfurt, Germany
A. R. Reolon Laboratori Nazionali di Frascati, INFN, Frascati, Italy
A. Reshetin Institute for Nuclear Research, Academy of Sciences, Moscow, Russia
F. Rettig Frankfurt Institute for Advanced Studies, Johann Wolfgang Goethe-Universität Frankfurt, Frankfurt, Germany
J.-P. Revol European Organization for Nuclear Research (CERN), Geneva, Switzerland
K. Reygers Physikalisches Institut, Ruprecht-Karls-Universität Heidelberg, Heidelberg, Germany
L. Riccati Sezione INFN, Turin, Italy
R. A. Ricci Laboratori Nazionali di Legnaro, INFN, Legnaro, Italy
T. Richert Division of Experimental High Energy Physics, University of Lund, Lund, Sweden
M. Richter Department of Physics, University of Oslo, Oslo, Norway
P. Riedler European Organization for Nuclear Research (CERN), Geneva, Switzerland
W. Riegler European Organization for Nuclear Research (CERN), Geneva, Switzerland
F. Riggi Dipartimento di Fisica e Astronomia dell’Università and Sezione INFN, Catania, Italy Sezione INFN, Catania, Italy
A. Rivetti Sezione INFN, Turin, Italy
M. Rodríguez Cahuantzi Benemérita Universidad Autónoma de Puebla, Puebla, Mexico
A. Rodriguez Manso Nikhef, National Institute for Subatomic Physics, Amsterdam, Netherlands
K. Røed Department of Physics and Technology, University of Bergen, Bergen, Norway Department of Physics, University of Oslo, Oslo, Norway
E. Rogochaya Joint Institute for Nuclear Research (JINR), Dubna, Russia
D. Rohr Frankfurt Institute for Advanced Studies, Johann Wolfgang Goethe-Universität Frankfurt, Frankfurt, Germany
D. Röhrich Department of Physics and Technology, University of Bergen, Bergen, Norway
R. Romita Research Division and ExtreMe Matter Institute EMMI, GSI Helmholtzzentrum für Schwerionenforschung, Darmstadt, Germany Nuclear Physics Group, STFC Daresbury Laboratory, Daresbury, United Kingdom
F. Ronchetti Laboratori Nazionali di Frascati, INFN, Frascati, Italy
P. Rosnet Laboratoire de Physique Corpusculaire (LPC), Clermont Université, Université Blaise Pascal, CNRS–IN2P3, Clermont-Ferrand, France
S. Rossegger European Organization for Nuclear Research (CERN), Geneva, Switzerland
A. Rossi European Organization for Nuclear Research (CERN), Geneva, Switzerland
P. Roy Saha Institute of Nuclear Physics, Kolkata, India
C. Roy Institut Pluridisciplinaire Hubert Curien (IPHC), Université de Strasbourg, CNRS-IN2P3, Strasbourg, France
A. J. Rubio Montero Centro de Investigaciones Energéticas Medioambientales y Tecnológicas (CIEMAT), Madrid, Spain
R. Rui Dipartimento di Fisica dell’Università and Sezione INFN, Trieste, Italy
R. Russo Dipartimento di Fisica dell’Università and Sezione INFN, Turin, Italy
E. Ryabinkin Russian Research Centre Kurchatov Institute, Moscow, Russia
A. Rybicki The Henryk Niewodniczanski Institute of Nuclear Physics, Polish Academy of Sciences, Cracow, Poland
S. Sadovsky Institute for High Energy Physics, Protvino, Russia
K. Šafařík European Organization for Nuclear Research (CERN), Geneva, Switzerland
R. Sahoo Indian Institute of Technology Indore (IITI), Indore, India
P. K. Sahu Institute of Physics, Bhubaneswar, India
J. Saini Variable Energy Cyclotron Centre, Kolkata, India
H. Sakaguchi Hiroshima University, Hiroshima, Japan
S. Sakai Lawrence Berkeley National Laboratory, Berkeley, California United States
D. Sakata University of Tsukuba, Tsukuba, Japan
C. A. Salgado Departamento de Física de Partículas and IGFAE, Universidad de Santiago de Compostela, Santiago de Compostela, Spain
J. Salzwedel Department of Physics, Ohio State University, Columbus, Ohio United States
S. Sambyal Physics Department, University of Jammu, Jammu, India
V. Samsonov Petersburg Nuclear Physics Institute, Gatchina, Russia
X. Sanchez Castro Institut Pluridisciplinaire Hubert Curien (IPHC), Université de Strasbourg, CNRS-IN2P3, Strasbourg, France
L. Šándor Institute of Experimental Physics, Slovak Academy of Sciences, Košice, Slovakia
A. Sandoval Instituto de Física, Universidad Nacional Autónoma de México, Mexico City, Mexico
M. Sano University of Tsukuba, Tsukuba, Japan
G. Santagati Dipartimento di Fisica e Astronomia dell’Università and Sezione INFN, Catania, Italy
R. Santoro Centro Fermi - Museo Storico della Fisica e Centro Studi e Ricerche “Enrico Fermi”, Rome, Italy European Organization for Nuclear Research (CERN), Geneva, Switzerland
J. Sarkamo Helsinki Institute of Physics (HIP) and University of Jyväskylä, Jyväskylä, Finland
D. Sarkar Variable Energy Cyclotron Centre, Kolkata, India
E. Scapparone Sezione INFN, Bologna, Italy
F. Scarlassara Dipartimento di Fisica e Astronomia dell’Università and Sezione INFN, Padova, Italy
R. P. Scharenberg Purdue University, West Lafayette, Indiana United States
C. Schiaua National Institute for Physics and Nuclear Engineering, Bucharest, Romania
R. Schicker Physikalisches Institut, Ruprecht-Karls-Universität Heidelberg, Heidelberg, Germany
H. R. Schmidt Eberhard Karls Universität Tübingen, Tübingen, Germany
C. Schmidt Research Division and ExtreMe Matter Institute EMMI, GSI Helmholtzzentrum für Schwerionenforschung, Darmstadt, Germany
S. Schuchmann Institut für Kernphysik, Johann Wolfgang Goethe-Universität Frankfurt, Frankfurt, Germany
J. Schukraft European Organization for Nuclear Research (CERN), Geneva, Switzerland
T. Schuster Yale University, New Haven, Connecticut United States
Y. Schutz European Organization for Nuclear Research (CERN), Geneva, Switzerland SUBATECH, Ecole des Mines de Nantes, Université de Nantes, CNRS-IN2P3, Nantes, France
K. Schwarz Research Division and ExtreMe Matter Institute EMMI, GSI Helmholtzzentrum für Schwerionenforschung, Darmstadt, Germany
K. Schweda Research Division and ExtreMe Matter Institute EMMI, GSI Helmholtzzentrum für Schwerionenforschung, Darmstadt, Germany
G. Scioli Dipartimento di Fisica e Astronomia dell’Università and Sezione INFN, Bologna, Italy
E. Scomparin Sezione INFN, Turin, Italy
R. Scott University of Tennessee, Knoxville, Tennessee United States
P. A. Scott School of Physics and Astronomy, University of Birmingham, Birmingham, United Kingdom
G. Segato Dipartimento di Fisica e Astronomia dell’Università and Sezione INFN, Padova, Italy
I. Selyuzhenkov Research Division and ExtreMe Matter Institute EMMI, GSI Helmholtzzentrum für Schwerionenforschung, Darmstadt, Germany
S. Senyukov Institut Pluridisciplinaire Hubert Curien (IPHC), Université de Strasbourg, CNRS-IN2P3, Strasbourg, France
J. Seo Pusan National University, Pusan, South Korea
S. Serci Dipartimento di Fisica dell’Università and Sezione INFN, Cagliari, Italy
E. Serradilla Centro de Investigaciones Energéticas Medioambientales y Tecnológicas (CIEMAT), Madrid, Spain Instituto de Física, Universidad Nacional Autónoma de México, Mexico City, Mexico
A. Sevcenco Institute of Space Sciences (ISS), Bucharest, Romania
A. Shabetai SUBATECH, Ecole des Mines de Nantes, Université de Nantes, CNRS-IN2P3, Nantes, France
G. Shabratova Joint Institute for Nuclear Research (JINR), Dubna, Russia
R. Shahoyan European Organization for Nuclear Research (CERN), Geneva, Switzerland
S. Sharma Physics Department, University of Jammu, Jammu, India
N. Sharma University of Tennessee, Knoxville, Tennessee United States
S. Rohni Physics Department, University of Jammu, Jammu, India
K. Shigaki Hiroshima University, Hiroshima, Japan
K. Shtejer Centro de Aplicaciones Tecnológicas y Desarrollo Nuclear (CEADEN), Havana, Cuba
Y. Sibiriak Russian Research Centre Kurchatov Institute, Moscow, Russia
E. Sicking Institut für Kernphysik, Westfälische Wilhelms-Universität Münster, Münster, Germany
S. Siddhanta Sezione INFN, Cagliari, Italy
T. Siemiarczuk National Centre for Nuclear Studies, Warsaw, Poland
D. Silvermyr Oak Ridge National Laboratory, Oak Ridge, Tennessee United States
C. Silvestre Laboratoire de Physique Subatomique et de Cosmologie (LPSC), Université Joseph Fourier, CNRS-IN2P3, Institut Polytechnique de Grenoble, Grenoble, France
G. Simatovic Instituto de Ciencias Nucleares, Universidad Nacional Autónoma de México, Mexico City, Mexico Rudjer Bošković Institute, Zagreb, Croatia
G. Simonetti European Organization for Nuclear Research (CERN), Geneva, Switzerland
R. Singaraju Variable Energy Cyclotron Centre, Kolkata, India
R. Singh Physics Department, University of Jammu, Jammu, India
S. Singha National Institute of Science Education and Research, Bhubaneswar, India Variable Energy Cyclotron Centre, Kolkata, India
V. Singhal Variable Energy Cyclotron Centre, Kolkata, India
T. Sinha Saha Institute of Nuclear Physics, Kolkata, India
B. C. Sinha Variable Energy Cyclotron Centre, Kolkata, India
B. Sitar Faculty of Mathematics, Physics and Informatics, Comenius University, Bratislava, Slovakia
M. Sitta Dipartimento di Scienze e Innovazione Tecnologica dell’Università del Piemonte Orientale and Gruppo Collegato INFN, Alessandria, Italy
T. B. Skaali Department of Physics, University of Oslo, Oslo, Norway
K. Skjerdal Department of Physics and Technology, University of Bergen, Bergen, Norway
R. Smakal Faculty of Nuclear Sciences and Physical Engineering, Czech Technical University in Prague, Prague, Czech Republic
N. Smirnov Yale University, New Haven, Connecticut United States
R. J. M. Snellings Nikhef, National Institute for Subatomic Physics and Institute for Subatomic Physics of Utrecht University, Utrecht, Netherlands
C. Søgaard Division of Experimental High Energy Physics, University of Lund, Lund, Sweden
R. Soltz Lawrence Livermore National Laboratory, Livermore, California United States
M. Song Yonsei University, Seoul, South Korea
J. Song Pusan National University, Pusan, South Korea
C. Soos European Organization for Nuclear Research (CERN), Geneva, Switzerland
F. Soramel Dipartimento di Fisica e Astronomia dell’Università and Sezione INFN, Padova, Italy
I. Sputowska The Henryk Niewodniczanski Institute of Nuclear Physics, Polish Academy of Sciences, Cracow, Poland
M. Spyropoulou-Stassinaki Physics Department, University of Athens, Athens, Greece
B. K. Srivastava Purdue University, West Lafayette, Indiana United States
J. Stachel Physikalisches Institut, Ruprecht-Karls-Universität Heidelberg, Heidelberg, Germany
I. Stan Institute of Space Sciences (ISS), Bucharest, Romania
G. Stefanek National Centre for Nuclear Studies, Warsaw, Poland
M. Steinpreis Department of Physics, Ohio State University, Columbus, Ohio United States
E. Stenlund Division of Experimental High Energy Physics, University of Lund, Lund, Sweden
G. Steyn Physics Department, University of Cape Town and iThemba LABS, National Research Foundation, Somerset West, South Africa
J. H. Stiller Physikalisches Institut, Ruprecht-Karls-Universität Heidelberg, Heidelberg, Germany
D. Stocco SUBATECH, Ecole des Mines de Nantes, Université de Nantes, CNRS-IN2P3, Nantes, France
M. Stolpovskiy Institute for High Energy Physics, Protvino, Russia
P. Strmen Faculty of Mathematics, Physics and Informatics, Comenius University, Bratislava, Slovakia
A. A. P. Suaide Universidade de São Paulo (USP), São Paulo, Brazil
M. A. Subieta Vásquez Dipartimento di Fisica dell’Università and Sezione INFN, Turin, Italy
T. Sugitate Hiroshima University, Hiroshima, Japan
C. Suire Institut de Physique Nucléaire d’Orsay (IPNO), Université Paris-Sud, CNRS-IN2P3, Orsay, France
M. Suleymanov COMSATS Institute of Information Technology (CIIT), Islamabad, Pakistan
R. Sultanov Institute for Theoretical and Experimental Physics, Moscow, Russia
M. Šumbera Nuclear Physics Institute, Academy of Sciences of the Czech Republic, Řež u Prahy, Czech Republic
T. Susa Rudjer Bošković Institute, Zagreb, Croatia
T. J. M. Symons Lawrence Berkeley National Laboratory, Berkeley, California United States
A. Szanto de Toledo Universidade de São Paulo (USP), São Paulo, Brazil
I. Szarka Faculty of Mathematics, Physics and Informatics, Comenius University, Bratislava, Slovakia
A. Szczepankiewicz European Organization for Nuclear Research (CERN), Geneva, Switzerland
M. Szymański Warsaw University of Technology, Warsaw, Poland
J. Takahashi Universidade Estadual de Campinas (UNICAMP), Campinas, Brazil
M. A. Tangaro Dipartimento Interateneo di Fisica ‘M. Merlin’ and Sezione INFN, Bari, Italy
J. D. Tapia Takaki Institut de Physique Nucléaire d’Orsay (IPNO), Université Paris-Sud, CNRS-IN2P3, Orsay, France
A. Tarantola Peloni Institut für Kernphysik, Johann Wolfgang Goethe-Universität Frankfurt, Frankfurt, Germany
A. Tarazona Martinez European Organization for Nuclear Research (CERN), Geneva, Switzerland
A. Tauro European Organization for Nuclear Research (CERN), Geneva, Switzerland
G. Tejeda Muñoz Benemérita Universidad Autónoma de Puebla, Puebla, Mexico
A. Telesca European Organization for Nuclear Research (CERN), Geneva, Switzerland
A. Ter Minasyan Russian Research Centre Kurchatov Institute, Moscow, Russia
C. Terrevoli Dipartimento Interateneo di Fisica ‘M. Merlin’ and Sezione INFN, Bari, Italy
J. Thäder Research Division and ExtreMe Matter Institute EMMI, GSI Helmholtzzentrum für Schwerionenforschung, Darmstadt, Germany
D. Thomas Nikhef, National Institute for Subatomic Physics and Institute for Subatomic Physics of Utrecht University, Utrecht, Netherlands
R. Tieulent Université de Lyon, Université Lyon 1, CNRS/IN2P3, IPN-Lyon, Villeurbanne, France
A. R. Timmins University of Houston, Houston, Texas United States
D. Tlusty Faculty of Nuclear Sciences and Physical Engineering, Czech Technical University in Prague, Prague, Czech Republic
A. Toia Dipartimento di Fisica e Astronomia dell’Università and Sezione INFN, Padova, Italy Frankfurt Institute for Advanced Studies, Johann Wolfgang Goethe-Universität Frankfurt, Frankfurt, Germany Sezione INFN, Padova, Italy
H. Torii University of Tokyo, Tokyo, Japan
L. Toscano Sezione INFN, Turin, Italy
V. Trubnikov Bogolyubov Institute for Theoretical Physics, Kiev, Ukraine
D. Truesdale Department of Physics, Ohio State University, Columbus, Ohio United States
W. H. Trzaska Helsinki Institute of Physics (HIP) and University of Jyväskylä, Jyväskylä, Finland
T. Tsuji University of Tokyo, Tokyo, Japan
A. Tumkin Russian Federal Nuclear Center (VNIIEF), Sarov, Russia
R. Turrisi Sezione INFN, Padova, Italy
T. S. Tveter Department of Physics, University of Oslo, Oslo, Norway
J. Ulery Institut für Kernphysik, Johann Wolfgang Goethe-Universität Frankfurt, Frankfurt, Germany
K. Ullaland Department of Physics and Technology, University of Bergen, Bergen, Norway
J. Ulrich Institut für Informatik, Johann Wolfgang Goethe-Universität Frankfurt, Frankfurt, Germany Kirchhoff-Institut für Physik, Ruprecht-Karls-Universität Heidelberg, Heidelberg, Germany
A. Uras Université de Lyon, Université Lyon 1, CNRS/IN2P3, IPN-Lyon, Villeurbanne, France
G. M. Urciuoli Sezione INFN, Rome, Italy
G. L. Usai Dipartimento di Fisica dell’Università and Sezione INFN, Cagliari, Italy
M. Vajzer Faculty of Nuclear Sciences and Physical Engineering, Czech Technical University in Prague, Prague, Czech Republic Nuclear Physics Institute, Academy of Sciences of the Czech Republic, Řež u Prahy, Czech Republic
M. Vala Institute of Experimental Physics, Slovak Academy of Sciences, Košice, Slovakia Joint Institute for Nuclear Research (JINR), Dubna, Russia
L. Valencia Palomo Institut de Physique Nucléaire d’Orsay (IPNO), Université Paris-Sud, CNRS-IN2P3, Orsay, France
S. Vallero Dipartimento di Fisica dell’Università and Sezione INFN, Turin, Italy
P. Vande Vyvre European Organization for Nuclear Research (CERN), Geneva, Switzerland
J. W. Van Hoorne European Organization for Nuclear Research (CERN), Geneva, Switzerland
M. van Leeuwen Nikhef, National Institute for Subatomic Physics and Institute for Subatomic Physics of Utrecht University, Utrecht, Netherlands
L. Vannucci Laboratori Nazionali di Legnaro, INFN, Legnaro, Italy
A. Vargas Benemérita Universidad Autónoma de Puebla, Puebla, Mexico
R. Varma Indian Institute of Technology Bombay (IIT), Mumbai, India
M. Vasileiou Physics Department, University of Athens, Athens, Greece
A. Vasiliev Russian Research Centre Kurchatov Institute, Moscow, Russia
V. Vechernin V. Fock Institute for Physics, St. Petersburg State University, St. Petersburg, Russia
M. Veldhoen Nikhef, National Institute for Subatomic Physics and Institute for Subatomic Physics of Utrecht University, Utrecht, Netherlands
M. Venaruzzo Dipartimento di Fisica dell’Università and Sezione INFN, Trieste, Italy
E. Vercellin Dipartimento di Fisica dell’Università and Sezione INFN, Turin, Italy
S. Vergara Benemérita Universidad Autónoma de Puebla, Puebla, Mexico
R. Vernet Centre de Calcul de l’IN2P3, Villeurbanne, France
M. Verweij Nikhef, National Institute for Subatomic Physics and Institute for Subatomic Physics of Utrecht University, Utrecht, Netherlands
L. Vickovic Technical University of Split FESB, Split, Croatia
G. Viesti Dipartimento di Fisica e Astronomia dell’Università and Sezione INFN, Padova, Italy
J. Viinikainen Helsinki Institute of Physics (HIP) and University of Jyväskylä, Jyväskylä, Finland
Z. Vilakazi Physics Department, University of Cape Town and iThemba LABS, National Research Foundation, Somerset West, South Africa
O. Villalobos Baillie School of Physics and Astronomy, University of Birmingham, Birmingham, United Kingdom
Y. Vinogradov Russian Federal Nuclear Center (VNIIEF), Sarov, Russia
L. Vinogradov V. Fock Institute for Physics, St. Petersburg State University, St. Petersburg, Russia
A. Vinogradov Russian Research Centre Kurchatov Institute, Moscow, Russia
T. Virgili Dipartimento di Fisica ‘E.R. Caianiello’ dell’Università and Gruppo Collegato INFN, Salerno, Italy
Y. P. Viyogi Variable Energy Cyclotron Centre, Kolkata, India
A. Vodopyanov Joint Institute for Nuclear Research (JINR), Dubna, Russia
M. A. Völkl Physikalisches Institut, Ruprecht-Karls-Universität Heidelberg, Heidelberg, Germany
S. Voloshin Wayne State University, Detroit, Michigan United States
K. Voloshin Institute for Theoretical and Experimental Physics, Moscow, Russia
G. Volpe European Organization for Nuclear Research (CERN), Geneva, Switzerland
B. von Haller European Organization for Nuclear Research (CERN), Geneva, Switzerland
I. Vorobyev V. Fock Institute for Physics, St. Petersburg State University, St. Petersburg, Russia
D. Vranic European Organization for Nuclear Research (CERN), Geneva, Switzerland Research Division and ExtreMe Matter Institute EMMI, GSI Helmholtzzentrum für Schwerionenforschung, Darmstadt, Germany
J. Vrláková Faculty of Science, P.J. Šafárik University, Košice, Slovakia
B. Vulpescu Laboratoire de Physique Corpusculaire (LPC), Clermont Université, Université Blaise Pascal, CNRS–IN2P3, Clermont-Ferrand, France
A. Vyushin Russian Federal Nuclear Center (VNIIEF), Sarov, Russia
V. Wagner Faculty of Nuclear Sciences and Physical Engineering, Czech Technical University in Prague, Prague, Czech Republic
B. Wagner Department of Physics and Technology, University of Bergen, Bergen, Norway
R. Wan Central China Normal University, Wuhan, China
Y. Wang Central China Normal University, Wuhan, China
Y. Wang Physikalisches Institut, Ruprecht-Karls-Universität Heidelberg, Heidelberg, Germany
M. Wang Central China Normal University, Wuhan, China
K. Watanabe University of Tsukuba, Tsukuba, Japan
M. Weber University of Houston, Houston, Texas United States
J. P. Wessels European Organization for Nuclear Research (CERN), Geneva, Switzerland Institut für Kernphysik, Westfälische Wilhelms-Universität Münster, Münster, Germany
U. Westerhoff Institut für Kernphysik, Westfälische Wilhelms-Universität Münster, Münster, Germany
J. Wiechula Eberhard Karls Universität Tübingen, Tübingen, Germany
J. Wikne Department of Physics, University of Oslo, Oslo, Norway
M. Wilde Institut für Kernphysik, Westfälische Wilhelms-Universität Münster, Münster, Germany
G. Wilk National Centre for Nuclear Studies, Warsaw, Poland
M. C. S. Williams Sezione INFN, Bologna, Italy
B. Windelband Physikalisches Institut, Ruprecht-Karls-Universität Heidelberg, Heidelberg, Germany
C. G. Yaldo Wayne State University, Detroit, Michigan United States
Y. Yamaguchi University of Tokyo, Tokyo, Japan
S. Yang Department of Physics and Technology, University of Bergen, Bergen, Norway
P. Yang Central China Normal University, Wuhan, China
H. Yang Commissariat à l’Energie Atomique, IRFU, Saclay, France Nikhef, National Institute for Subatomic Physics and Institute for Subatomic Physics of Utrecht University, Utrecht, Netherlands
S. Yasnopolskiy Russian Research Centre Kurchatov Institute, Moscow, Russia
J. Yi Pusan National University, Pusan, South Korea
Z. Yin Central China Normal University, Wuhan, China
I.-K. Yoo Pusan National University, Pusan, South Korea
J. Yoon Yonsei University, Seoul, South Korea
X. Yuan Central China Normal University, Wuhan, China
I. Yushmanov Russian Research Centre Kurchatov Institute, Moscow, Russia
V. Zaccolo Niels Bohr Institute, University of Copenhagen, Copenhagen, Denmark
C. Zach Faculty of Nuclear Sciences and Physical Engineering, Czech Technical University in Prague, Prague, Czech Republic
C. Zampolli Sezione INFN, Bologna, Italy
S. Zaporozhets Joint Institute for Nuclear Research (JINR), Dubna, Russia
A. Zarochentsev V. Fock Institute for Physics, St. Petersburg State University, St. Petersburg, Russia
P. Závada Institute of Physics, Academy of Sciences of the Czech Republic, Prague, Czech Republic
N. Zaviyalov Russian Federal Nuclear Center (VNIIEF), Sarov, Russia
H. Zbroszczyk Warsaw University of Technology, Warsaw, Poland
P. Zelnicek Institut für Informatik, Johann Wolfgang Goethe-Universität Frankfurt, Frankfurt, Germany
I. S. Zgura Institute of Space Sciences (ISS), Bucharest, Romania
M. Zhalov Petersburg Nuclear Physics Institute, Gatchina, Russia
Y. Zhang Central China Normal University, Wuhan, China
H. Zhang Central China Normal University, Wuhan, China
X. Zhang Central China Normal University, Wuhan, China Laboratoire de Physique Corpusculaire (LPC), Clermont Université, Université Blaise Pascal, CNRS–IN2P3, Clermont-Ferrand, France Lawrence Berkeley National Laboratory, Berkeley, California United States
D. Zhou Central China Normal University, Wuhan, China
Y. Zhou Nikhef, National Institute for Subatomic Physics and Institute for Subatomic Physics of Utrecht University, Utrecht, Netherlands
F. Zhou Central China Normal University, Wuhan, China
H. Zhu Central China Normal University, Wuhan, China
J. Zhu Central China Normal University, Wuhan, China
X. Zhu Central China Normal University, Wuhan, China
J. Zhu Central China Normal University, Wuhan, China
A. Zichichi Centro Fermi - Museo Storico della Fisica e Centro Studi e Ricerche “Enrico Fermi”, Rome, Italy Dipartimento di Fisica e Astronomia dell’Università and Sezione INFN, Bologna, Italy
A. Zimmermann Physikalisches Institut, Ruprecht-Karls-Universität Heidelberg, Heidelberg, Germany
G. Zinovjev Bogolyubov Institute for Theoretical Physics, Kiev, Ukraine
Y. Zoccarato Université de Lyon, Université Lyon 1, CNRS/IN2P3, IPN-Lyon, Villeurbanne, France
M. Zynovyev Bogolyubov Institute for Theoretical Physics, Kiev, Ukraine
M. Zyzak Institut für Kernphysik, Johann Wolfgang Goethe-Universität Frankfurt, Frankfurt, Germany

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J/ψ elliptic flow in Pb-Pb collisions at √(s(NN))=2.76 TeV

We report on the first measurement of inclusive J/ψ elliptic flow v2 in heavy-ion collisions at the LHC. The measurement is performed with the ALICE detector in Pb-Pb collisions at √(s(NN))=2.76 TeV in the rapidity range 2.5<y<4.0. The dependence of the J/ψ v2 on the collision centrality and on the J/ψ transverse momentum is studied in the range 0≤p(T)<10 GeV/c. For semicentral Pb-Pb collisions at √(s(NN))=2.76 TeV, an indication of nonzero v2 is observed with a largest measured value of v2=0.116±0.046(stat)±0.029(syst) for J/ψ in the transverse momentum range 2≤p(T)<4 GeV/c. The elliptic flow measurement complements the previously reported ALICE results on the inclusive J/ψ nuclear modification factor and favors the scenario of a significant fraction of J/ψ production from charm quarks in a deconfined partonic phase.

D meson elliptic flow in noncentral Pb-Pb collisions at sqrt[sNN]=2.76 Tev

Azimuthally anisotropic distributions of D0, D+, and D*+ mesons were studied in the central rapidity region (|y|<0.8) in Pb-Pb collisions at a center-of-mass energy sqrt[sNN]=2.76  TeV per nucleon-nucleon collision, with the ALICE detector at the LHC. The second Fourier coefficient v2 (commonly denoted elliptic flow) was measured in the centrality class 30%-50% as a function of the D meson transverse momentum pT, in the range 2-16  GeV/c. The measured v2 of D mesons is comparable in magnitude to that of light-flavor hadrons. It is positive in the range 2<pT<6  GeV/c with 5.7σ significance, based on the combination of statistical and systematic uncertainties.

Medium modification of jet fragmentation in Au+Au collisions at √[s(NN)]=200 GeV measured in direct photon-hadron correlations

The jet fragmentation function is measured with direct photon-hadron correlations in p+p and Au+Au collisions at √[s(NN)]=200 GeV. The p(T) of the photon is an excellent approximation to the initial p(T) of the jet and the ratio z(T)=p(T)(h)/p(T)(γ) is used as a proxy for the jet fragmentation function. A statistical subtraction is used to extract the direct photon-hadron yields in Au+Au collisions while a photon isolation cut is applied in p+p. I(AA), the ratio of hadron yield opposite the photon in Au+Au to that in p+p, indicates modification of the jet fragmentation function. Suppression, most likely due to energy loss in the medium, is seen at high z(T). The associated hadron yield at low z(T) is enhanced at large angles. Such a trend is expected from redistribution of the lost energy into increased production of low-momentum particles.