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Beam-Energy Dependence of Directed Flow of Λ, Λ , K±, Ks0, and φ in Au+Au Collisions

  • STAR Collaboration
  • AGH University of Krakow
  • Ohio State University
  • University of Kentucky
  • Joint Institute for Nuclear Research
  • Panjab University
  • Variable Energy Cyclotron Centre India
  • Stony Brook University
  • Alikhanov Institute for Theoretical and Experimental Physics
  • Moscow Engineering Physics Institute
  • Texas A&M University
  • University of Tsukuba
  • Brookhaven National Laboratory
  • Tsinghua University
  • Central China Normal University
  • National Institute of Science Education and Research
  • University of California at Riverside
  • University of Houston
  • University of Jammu
  • University of Texas at Austin
  • Czech Technical University in Prague
  • Czech Academy of Sciences
  • Kent State University
  • Rice University
  • Lehigh University
  • Yale University
  • University of California at Davis
  • Shandong University
  • University of Science and Technology of China
  • Chinese Academy of Sciences
  • CAS - Institute of Modern Physics

Research output: Contribution to journalArticlepeer-review

114 Scopus citations

Abstract

Rapidity-odd directed-flow measurements at midrapidity are presented for Λ, Λ, K±, Ks0, and φ at sNN=7.7, 11.5, 14.5, 19.6, 27, 39, 62.4, and 200 GeV in Au+Au collisions recorded by the Solenoidal Tracker detector at the Relativistic Heavy Ion Collider. These measurements greatly expand the scope of data available to constrain models with differing prescriptions for the equation of state of quantum chromodynamics. Results show good sensitivity for testing a picture where flow is assumed to be imposed before hadron formation and the observed particles are assumed to form via coalescence of constituent quarks. The pattern of departure from a coalescence-inspired sum rule can be a valuable new tool for probing the collision dynamics.

Original languageEnglish
Article number062301
JournalPhysical Review Letters
Volume120
Issue number6
DOIs
StatePublished - Feb 6 2018

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