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Particle-Type Dependence of Azimuthal Anisotropy and Nuclear Modification of Particle Production in Au + Au Collisions at √SNN= 200 GeV

  • STAR Collaboration
  • University of Birmingham
  • Goethe University Frankfurt
  • Panjab University
  • Variable Energy Cyclotron Centre India
  • Kent State University
  • University of California at Davis
  • Joint Institute for Nuclear Research
  • University of Jammu
  • Indiana University Bloomington
  • Purdue University
  • Institut de Recherches Subatomiques
  • Ohio State University
  • Wayne State University
  • Yale University
  • University of Rajasthan
  • University of Washington
  • Brookhaven National Laboratory
  • Rice University
  • National Institute for Subatomic Physics
  • SUBATECH
  • Moscow Engineering Physics Institute
  • Argonne National Laboratory
  • Academia Sinica - Shanghai Institute of Nuclear Research
  • Lawrence Berkeley National Laboratory
  • Czech Academy of Sciences
  • University of Science and Technology of China
  • University of California at Los Angeles
  • Creighton University
  • University of Texas at Austin

Research output: Contribution to journalArticlepeer-review

577 Scopus citations

Abstract

We present STAR measurements of the azimuthal anisotropy parameter ν2 and the binary-collision scaled centrality ratio RCP for kaons and lambdas (Λ + Λ) at midrapidity in Au + Au collisions at √sNN = 200 GeV. In combination, the ν2 and RCP particle-type dependencies contradict expectations from partonic energy loss followed by standard fragmentation in vacuum We establish pT ≈ 5 GeV/c as the value where the centrality dependent baryon enhancement ends. The K0 and Λ + Λ¯ ν2 values are consistent with expectations of constituent-quark-number scaling from models of hadron formation by parton coalescence or recombination.

Original languageEnglish
Article number052302
Pages (from-to)523021-523026
Number of pages6
JournalPhysical Review Letters
Volume92
Issue number5
DOIs
StatePublished - Feb 6 2004

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