Triangular Flow of Identified Hadrons in Au+Au Collisions at √s NN = 39 & 200 GeV Xu Sun (1,2) for the STAR Collaboration TPC ToFToF 33 1)Harbin Institute.

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Triangular Flow of Identified Hadrons in Au+Au Collisions at √s NN = 39 & 200 GeV Xu Sun (1,2) for the STAR Collaboration TPC ToFToF 33 1)Harbin Institute of Technology, Harbin, China 2)Lawrence Berkeley National Laboratory, Berkeley, USA Initial Condition and Collectivity in high-energy nuclear collisions

Particle Identification and p T Dependence 5/24/14Xu Sun – QM Flash Talk 39 GeV STAR Preliminary Au+Au, 200 GeV,00-80% 2 Mass ordering of v 3 for 200 and 39 GeV  radial flow The collectivity is stronger in 200GeV collisions Au+Au, 39 GeV,00-80%

Number-of-Constituent Quark Scaling 5/24/14Xu Sun – QM Flash Talk3 STAR Preliminary Au+Au 200 GeV R. Lacey, J. Phys. G: Nucl. Part. Phys. 38 (2011) AMPT: PRC 84, (2011) Harri Niemi, QM14, Friday STAR Preliminary 200 GeV 39 GeV Collective behavior for v 3 at 39 and 200 GeV Mass ordering at low p T, similar to v 2 v 2 /v 3 > 1: v 2 geometry +fluctuation v 3 fluctuation More energies (19.6, 27,…) and particle species (K 0 s,Λ,…) coming soon Collective behavior for v 3 at 39 and 200 GeV Mass ordering at low p T, similar to v 2 v 2 /v 3 > 1: v 2 geometry +fluctuation v 3 fluctuation More energies (19.6, 27,…) and particle species (K 0 s,Λ,…) coming soon