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v 2 and v 4 centrality, p t and particle-type dependence in Au+Au collisions at RHIC Yuting Bai for the STAR Collaboration
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Yuting Bai2 Outline Introduction v 2 v 4 v 4 /v 2 2 Conclusion
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Yuting Bai3 Anisotropic Flow Anisotropic flow ≡ azimuthal correlation with the reaction plane established early, self- quenching, therefore sensitive to the early stage of the collisions
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Yuting Bai4 Charged particle v 2 as function of p t at 200GeV and 62GeV Charged particle v 2 from four particle cumulant are measured up to ~ 10 GeV at 200GeV. For Au+Au at 200 GeV still significant v 2 above 6 GeV/c -1.3 < < 1.3 Star Preliminary v 2 {4}: v 2 from 4-particle cumulant method.
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Yuting Bai5 The centrality dependence of v 2 changes from low-p t to intermediate p t. At intermediate p t the maximum v 2 is for the 30-40% centrality bin around 3 GeV/c. Charged particle v 2 as function of p t at 200GeV and 62GeV Star Preliminary
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Yuting Bai6 Charged particle v 2 as function of pseudorapidity at 200GeV and 62GeV Star Preliminary v 2 increases from 62 to 200 GeV
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Yuting Bai7 The increase in v 2 from 62 GeV to 200 GeV is larger at forward rapidity could be understood as a result of v 2 ~ dN/d v 2 {200}/v 2 {62} as function of pseudorapidity at 200GeV and 62GeV Star Preliminary
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Yuting Bai8 Charged particle v 2 as a function of -y beam at 200GeV and 62GeV Longitudinal scaling approximately holds Star Preliminary Only particles with positive are shown
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Yuting Bai9 Centrality dependence: (m T – m) scaling At low-p t m T -scaling: indicative for a common velocity for the different particles At intermediate p t meson- baryon grouping: indicative for coalescence mechanism m T -scaling and baryon meson grouping holds for all centralities! Star Preliminary event plane method
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Yuting Bai10 Centrality dependence: NQ scaling NQ scaling holds for all centralities. is systematically lower than other particles in central collisions. Star Preliminary
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Yuting Bai11 Star Preliminary NQ scaling at 62.4GeV At 62.4 and 200 GeV the same scaling is observed! minbias data (0-80%)
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Yuting Bai12 Higher Harmonics Higher harmonics are expected to be present. For smooth azimuthal distributions they will be small, v n ~ v 2 n/2 v 4 /v 2 2 a probe of ideal hydro behavior and related to degree of thermalization! Peter Kolb, PRC 68, 031902 R.S.Bhalerao et.al PLB 627,49; Borghini and Ollitrault, arXiv:nucl-th/0506045
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Yuting Bai13 Charged particle v 4 as function of p t at 200GeV and 62GeV Charged particle v 4 are measured up to ~ 7 GeV at 200GeV. Star Preliminary -1.3 < eta < 1.3 Relative to the 2nd order event plane
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Yuting Bai14 As for v 2, v 4 increases from 62 to 200 GeV Charge particle v 4 as function of pseudorapidity at 200GeV and 62GeV Star Preliminary
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Yuting Bai15 Same as v 2, for v 4 longitudinal scaling approximately holds Charged particle v 4 as function of -y beam at 200GeV and 62GeV Star Preliminary
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Yuting Bai16 v 4 systematic uncertainty estimate Uncertainties on are small, however they quickly become significant at larger p t
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Yuting Bai17 v 4 /v 2 2 for charged particles at 200GeV v 4 /v 2 2 a detailed probe of ideal hydro behavior and related to the degree of thermalization! Data points are above the model predictions, however due to the systematic uncertainty from non-flow we can not exclude the models yet Star Preliminary
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Yuting Bai18 Conclusions v 2 from four particle cumulant is measured up to 10 GeV/c Still significant v 2 observed above 6 GeV/c v 2 for identified particles shows m T scaling at low-p t and NQ scaling at intermediate p t For all centralities The energy dependence of v 2 and v 4 is approximately described by longitudinal scaling The observed ratio of v 4 /v 2 2 is above the ideal hydro predictions and close to AMPT, however the systematic uncertainties from non-flow do not allow us to contradict ideal hydrodynamics
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Yuting Bai19 v 4 /v 2 2 for charged particle as a function of p t at 200GeV and 62GeV Star Preliminary
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Yuting Bai20 v 4 /v 2 2 for charged particles as function of pseudorapidity at 200GeV and 62GeV Star Preliminary
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Yuting Bai21 Systematic errors are shown at mid-rapidity only. At forward rapidity, the non-flow effects are expected to be small. at mid-rapidity, the ratios are above 1, which is compatible with those at forward rapidity. v 4 /v 2 2 for charged particles as a function of pseudorapidity at 200GeV Star Preliminary
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Yuting Bai22 non-flow effect on v 4 /v 2 2 For v 4 /v 2 2 :
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