Azimuthal anisotropy in Au+Au collisions at sqrtsNN = 200 GeV
STAR Collaboration
TL;DR
The paper presents comprehensive measurements of azimuthal anisotropy in Au+Au collisions at $\sqrt{s_{NN}}=200$ GeV, focusing on directed, elliptic, and higher harmonic flows. Using multiple analysis methods (event-plane, cumulants, and mixed-harmonics), it addresses nonflow and fluctuations while comparing to hydrodynamic, transport, and Blast Wave models. Key findings include in-plane $v_2$ with mass ordering at low $p_T$, constituent-quark-number scaling for identified hadrons at intermediate $p_T$, and $v_4$ that scales with $v_2^2$ but exceeds simple coalescence expectations, challenging some model assumptions. Blast Wave fits provide a coherent framework to systematize the data across centralities, suggesting significant but nuanced collective behavior and partial early thermalization in the produced medium, with ongoing tension between hydrodynamic descriptions and high-$p_T$ phenomena.
Abstract
The results from the STAR Collaboration on directed flow (v_1), elliptic flow (v_2), and the fourth harmonic (v_4) in the anisotropic azimuthal distribution of particles from Au+Au collisions at sqrtsNN = 200 GeV are summarized and compared with results from other experiments and theoretical models. Results for identified particles are presented and fit with a Blast Wave model. Different anisotropic flow analysis methods are compared and nonflow effects are extracted from the data. For v_2, scaling with the number of constituent quarks and parton coalescence is discussed. For v_4, scaling with v_2^2 and quark coalescence is discussed.
