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Third harmonic flow of charged particles in Au plus Au collisions at root s(NN)=200 GeV
Adamczyk, L.1; Adkins, J. K.23; Agakishiev, G.21; Aggarwal, M. M.34; Ahammed, Z.53; Alakhverdyants, A. V.21; Alekseev, I.19; Alford, J.22; Anson, C. D.31; Arkhipkin, D.4
刊名PHYSICAL REVIEW C
2013-07-15
卷号88
ISSN号0556-2813
DOI10.1103/PhysRevC.88.014904
文献子类Article
英文摘要We report measurements of the third harmonic coefficient of the azimuthal anisotropy, upsilon(3), known as triangular flow. The analysis is for charged particles in Au + Au collisions at root s(NN) = 200 GeV, based on data from the STAR experiment at the BNL Relativistic Heavy Ion Collider. Two-particle correlations as a function of their pseudorapidity separation are fit with narrow and wide Gaussians. Measurements of triangular flow are extracted from the wide Gaussian, from two-particle cumulants with a pseudorapidity gap, and also from event plane analysis methods with a large pseudorapidity gap between the particles and the event plane. These results are reported as a function of transverse momentum and centrality. A large dependence on the pseudorapidity gap is found. Results are compared with other experiments and model calculations.
资助项目National Research Foundation[NRF-2012004024]
WOS关键词TIME PROJECTION CHAMBER ; MODEL ; STAR
WOS研究方向Physics
语种英语
出版者AMER PHYSICAL SOC
WOS记录号WOS:000321839300002
内容类型期刊论文
源URL[http://119.78.100.186/handle/113462/48409]  
专题中国科学院近代物理研究所
通讯作者Adamczyk, L.
作者单位1.AGH Univ Sci & Technol, Krakow, Poland
2.Argonne Natl Lab, Argonne, IL 60439 USA
3.Univ Birmingham, Birmingham, W Midlands, England
4.Brookhaven Natl Lab, Upton, NY 11973 USA
5.Univ Calif Berkeley, Berkeley, CA 94720 USA
6.Univ Calif Davis, Davis, CA 95616 USA
7.Univ Calif Los Angeles, Los Angeles, CA 90095 USA
8.Univ Estadual Campinas, Sao Paulo, Brazil
9.Cent China Normal Univ HZNU, Wuhan 430079, Peoples R China
10.Univ Illinois, Chicago, IL 60607 USA
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Adamczyk, L.,Adkins, J. K.,Agakishiev, G.,et al. Third harmonic flow of charged particles in Au plus Au collisions at root s(NN)=200 GeV[J]. PHYSICAL REVIEW C,2013,88.
APA Adamczyk, L..,Adkins, J. K..,Agakishiev, G..,Aggarwal, M. M..,Ahammed, Z..,...&STAR Collaboration.(2013).Third harmonic flow of charged particles in Au plus Au collisions at root s(NN)=200 GeV.PHYSICAL REVIEW C,88.
MLA Adamczyk, L.,et al."Third harmonic flow of charged particles in Au plus Au collisions at root s(NN)=200 GeV".PHYSICAL REVIEW C 88(2013).
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