Directed Flow of Identified Particles in Au+Au Collisions at SNN=200GeV at RHIC

L. Adamczyk et al. (STAR Collaboration)
Phys. Rev. Lett. 108, 202301 – Published 15 May 2012

Abstract

STAR’s measurements of directed flow (v1) around midrapidity for π±, K±, KS0, p, and p¯ in Au+Au collisions at sNN=200GeV are presented. A negative v1(y) slope is observed for most of produced particles (π±, K±, KS0, and p¯). In 5%–30% central collisions, a sizable difference is present between the v1(y) slope of protons and antiprotons, with the former being consistent with zero within errors. The v1 excitation function is presented. Comparisons to model calculations (RQMD, UrQMD, AMPT, QGSM with parton recombination, and a hydrodynamics model with a tilted source) are made. For those models which have calculations of v1 for both pions and protons, none of them can describe v1(y) for pions and protons simultaneously. The hydrodynamics model with a tilted source as currently implemented cannot explain the centrality dependence of the difference between the v1(y) slopes of protons and antiprotons.

  • Figure
  • Figure
  • Figure
  • Figure
  • Received 16 December 2011

DOI:https://doi.org/10.1103/PhysRevLett.108.202301

© 2012 American Physical Society

Authors & Affiliations

Click to Expand

Article Text (Subscription Required)

Click to Expand

References (Subscription Required)

Click to Expand
Issue

Vol. 108, Iss. 20 — 18 May 2012

Reuse & Permissions
Access Options
CHORUS

Article Available via CHORUS

Download Accepted Manuscript
Author publication services for translation and copyediting assistance advertisement

Authorization Required


×
×

Images

×

Sign up to receive regular email alerts from Physical Review Letters

Log In

Cancel
×

Search


Article Lookup

Paste a citation or DOI

Enter a citation
×