Energy and system size dependence of elliptic flow: using rapidity gaps to suppress non-flow contribution

Details Energy and system size dependence of elliptic flow: using rapidity gaps to suppress non-flow contribution Energy and system size dependence of elliptic flow: using rapidity gaps to suppress non-flow contribution

2006-10-25

arxiv.org/abs/nucl-ex/0610038v1

AIPConf.Proc.870:691-694,2006

Physics

Nuclear Physics

Nuclear Experiment

4 pages. Talk at CIPANP 2006, 9th Conference on the Intersections of Particle and Nuclear Physics, May 30-June 3, 2006, Rio Gr

Scientific paper

10.1063/1.2402731

In this talk I present new STAR results on measurements of integrated elliptic flow at midrapidity in Au+Au and Cu+Cu collisions at $\sqrt{s_{NN}}=$200 and 62 GeV energies. These results have been obtained from azimuthal correlations between particles in the main STAR TPC and two forward TPCs, and are to a large extent free from so-called non-flow correlations. These results along with the previously reported values of ``participant'' eccentricity taking into account eccentricity fluctuations are used for testing the $v_2/\eps$ scaling, which is found to hold relatively well.

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