Azimuthal anisotropy in Au plus Au collisions at √SNN=200 GeV -: art. no. 014904

被引:565
作者
Adams, J
Aggarwal, MM
Ahammed, Z
Amonett, J
Anderson, BD
Arkhipkin, D
Averichev, GS
Badyal, SK
Bai, Y
Balewski, J
Barannikova, O
Barnby, LS
Baudot, J
Bekele, S
Belaga, VV
Bellwied, R
Berger, J
Bezverkhny, BI
Bharadwaj, S
Bhasin, A
Bhati, AK
Bhatia, VS
Bichsel, H
Bielcik, J
Bielcikova, J
Billmeier, A
Bland, LC
Blyth, CO
Bonner, BE
Botje, M
Boucham, A
Brandin, AV
Bravar, A
Bystersky, M
Cadman, RV
Cai, XZ
Caines, H
Sánchez, MCD
Castillo, J
Catu, O
Cebra, D
Chajecki, Z
Chaloupka, P
Chattopadhyay, S
Chen, HF
Chen, Y
Cheng, J
Cherney, M
Chikanian, A
Christie, W
机构
[1] Argonne Natl Lab, Argonne, IL 60439 USA
[2] Univ Bern, CH-3012 Bern, Switzerland
[3] Univ Birmingham, Birmingham, W Midlands, England
[4] Brookhaven Natl Lab, Upton, NY 11973 USA
[5] CALTECH, Pasadena, CA 91125 USA
[6] Univ Calif Berkeley, Berkeley, CA 94720 USA
[7] Univ Calif Davis, Davis, CA 95616 USA
[8] Univ Calif Los Angeles, Los Angeles, CA 90095 USA
[9] Carnegie Mellon Univ, Pittsburgh, PA 15213 USA
[10] Creighton Univ, Omaha, NE 68178 USA
[11] AS CR, Inst Nucl Phys, CR-25068 Prague, Czech Republic
[12] JINR, Lab High Energy, Dubna, Russia
[13] JINR, Particle Phys Lab, Dubna, Russia
[14] Goethe Univ Frankfurt, D-6000 Frankfurt, Germany
[15] Inst Phys, Bhubaneswar 751005, Orissa, India
[16] Indian Inst Technol, Bombay 400076, Maharashtra, India
[17] Indiana Univ, Bloomington, IN 47408 USA
[18] Inst Rech Subatom, Strasbourg, France
[19] Univ Jammu, Jammu 180001, India
[20] Kent State Univ, Kent, OH 44242 USA
[21] Lawrence Berkeley Natl Lab, Berkeley, CA 94720 USA
[22] MIT, Cambridge, MA 02139 USA
[23] Max Planck Inst Phys & Astrophys, D-80805 Munich, Germany
[24] Michigan State Univ, E Lansing, MI 48824 USA
[25] Moscow Engn Phys Inst, Moscow, Russia
[26] CUNY City Coll, New York, NY 10031 USA
[27] NIKHEF, Amsterdam, Netherlands
[28] Ohio State Univ, Columbus, OH 43210 USA
[29] Panjab Univ, Chandigarh 160014, India
[30] Penn State Univ, University Pk, PA 16802 USA
[31] Inst High Energy Phys, Protvino, Russia
[32] Purdue Univ, W Lafayette, IN 47907 USA
[33] Univ Rajasthan, Jaipur 302004, Rajasthan, India
[34] Rice Univ, Houston, TX 77251 USA
[35] Univ Sao Paulo, Sao Paulo, Brazil
[36] Univ Sci & Technol China, Anhui 230027, Peoples R China
[37] Shanghai Inst Appl Phys, Shanghai 201800, Peoples R China
[38] SUBATECH, Nantes, France
[39] Texas A&M Univ, College Stn, TX 77843 USA
[40] Univ Texas, Austin, TX 78712 USA
[41] Tsinghua Univ, Beijing 100084, Peoples R China
[42] Valparaiso Univ, Valparaiso, IN 46383 USA
[43] Ctr Variable Energy Cyclotron, Kolkata 700064, W Bengal, India
[44] Warsaw Univ Technol, Warsaw, Poland
[45] Univ Washington, Seattle, WA 98195 USA
[46] Wayne State Univ, Detroit, MI 48201 USA
[47] CCNU HZNU, Inst Particle Phys, Wuhan 430079, Peoples R China
[48] Yale Univ, New Haven, CT 06520 USA
[49] Univ Zagreb, HR-10002 Zagreb, Croatia
来源
PHYSICAL REVIEW C | 2005年 / 72卷 / 01期
关键词
D O I
10.1103/PhysRevC.72.014904
中图分类号
O57 [原子核物理学、高能物理学];
学科分类号
070202 ;
摘要
The results from the STAR Collaboration on directed flow (v(1)), elliptic flow (v(2)), and the fourth harmonic (v(4)) in the anisotropic azimuthal distribution of particles from Au+Au collisions at root s(NN) = 200 GeV are summarized and compared with results from other experiments and theoretical models. Results for identified particles are presented and fit with a blast-wave model. Different anisotropic flow analysis methods are compared and nonflow effects are extracted from the data. For v(2), scaling with the number of constituent quarks and parton coalescence are discussed. For v(4), scaling with v(2)(2) and quark coalescence are discussed.
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