Mass, quark-number, and sNN\sqrt{s_{NN}} dependence of the second and fourth flow harmonics in ultra-relativistic nucleus-nucleus collisions

preprint2007arXivOpen access

Abstract

We present STAR measurements of the azimuthal anisotropy parameter v2v_2 for pions, kaons, protons, ΛΛ, Λˉ\barΛ, Ξ+ΞˉΞ+\barΞ, and Ω+ΩˉΩ+ \barΩ, along with v4v_4 for pions, kaons, protons, and Λ+ΛˉΛ+ \barΛ at mid-rapidity for Au+Au collisions at sNN=62.4\sqrt{s_{_{NN}}}=62.4 and 200 GeV. The v2(pT)v_2(p_T) values for all hadron species at 62.4 GeV are similar to those observed in 130 and 200 GeV collisions. For observed kinematic ranges, v2v_2 values at 62.4, 130, and 200 GeV are as little as 10%--15% larger than those in Pb+Pb collisions at sNN=17.3\sqrt{s_{_{NN}}}=17.3 GeV. At intermediate transverse momentum (pTp_T from 1.5--5 GeV/c), the 62.4 GeV v2(pT)v_2(p_T) and v4(pT)v_4(p_T) values are consistent with the quark-number scaling first observed at 200 GeV. A four-particle cumulant analysis is used to assess the non-flow contributions to pions and protons and some indications are found for a smaller non-flow contribution to protons than pions. Baryon v2v_2 is larger than anti-baryon v2v_2 at 62.4 and 200 GeV perhaps indicating either that the initial spatial net-baryon distribution is anisotropic, that the mechanism leading to transport of baryon number from beam- to mid-rapidity enhances v2v_2, or that anti-baryon and baryon annihilation is larger in the in-plane direction.

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