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Register a new userBeam Energy Dependence of the Third Harmonic of Azimuthal Correlations in Au+Au Collisions at RHIC
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We present results from a harmonic decomposition of two-particle azimuthal correlations measured with the STAR detector in Au+Au collisions for energies ranging from $sqrt{s_{NN}}=7.7$ GeV to 200 GeV. The third harmonic $v_3^2{2}=langle cos3(phi_1-phi_2)rangle$, where $phi_1-phi_2$ is the angular difference in azimuth, is studied as a function of the pseudorapidity difference between particle pairs $Deltaeta = eta_1-eta_2$. Non-zero {vthree} is directly related to the previously observed large-$Deltaeta$ narrow-$Deltaphi$ ridge correlations and has been shown in models to be sensitive to the existence of a low viscosity Quark Gluon Plasma (QGP) phase. For sufficiently central collisions, $v_3^2{2}$ persist down to an energy of 7.7 GeV suggesting that QGP may be created even in these low energy collisions. In peripheral collisions at these low energies however, $v_3^2{2}$ is consistent with zero. When scaled by pseudorapidity density of charged particle multiplicity per participating nucleon pair, $v_3^2{2}$ for central collisions shows a minimum near {snn}$=20$ GeV.
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The two-particle angular correlation functions, $R_2$, of pions, kaons, and protons in Au+Au collisions at $sqrt{s_{NN}}=$ 7.7, 11.5, 14.5, 19.6, 27, 39, 62.4, and 200 GeV were measured by the STAR experiment at RHIC. These correlations were measured for both like-sign and unlike-sign charge combinations and versus the centrality. The correlations of pions and kaons show the expected near-side ({it i.e.}, at small relative angles) peak resulting from short-range mechanisms. The amplitudes of these short-range correlations decrease with increasing beam energy. However, the proton correlation functions exhibit strong anticorrelations in the near-side region. This behavior is observed for the first time in an A+A collision system. The observed anticorrelation is $p_{T}$-independent and decreases with increasing beam energy and centrality. The experimental results are also compared to the Monte Carlo models UrQMD, Hijing, and AMPT.
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