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Probing strangeness canonical ensemble with K, ϕ(1020) and Ξ production in Au+Au collisions at sNN=3 GeV

  • STAR Collaboration
  • American University in Cairo
  • Texas A&M University
  • Brookhaven National Laboratory
  • AGH University of Krakow
  • Ohio State University
  • University of Kentucky
  • Joint Institute for Nuclear Research
  • Panjab University
  • Variable Energy Cyclotron Centre India
  • Alikhanov Institute for Theoretical and Experimental Physics
  • Moscow Engineering Physics Institute
  • Central China Normal University
  • Kent State University
  • Universidad de Tarapacá
  • University of California at Riverside
  • University of Houston
  • Stony Brook University
  • University of Jammu
  • Czech Technical University in Prague
  • Czech Academy of Sciences
  • Rice University
  • Chinese Academy of Sciences
  • Yale University
  • University of California at Davis
  • Lawrence Berkeley National Laboratory
  • University of California at Los Angeles
  • National Cheng Kung University
  • Shandong University
  • Fudan University

Research output: Contribution to journalArticlepeer-review

21 Scopus citations

Abstract

We report the first multi-differential measurements of strange hadrons of K, ϕ and Ξ yields as well as the ratios of ϕ/K and ϕ/Ξ in Au+Au collisions at sNN=3 GeV with the STAR experiment fixed target configuration at RHIC. The ϕ mesons and Ξ hyperons are measured through hadronic decay channels, ϕ→K+K and Ξ→Λπ. Collision centrality and rapidity dependence of the transverse momentum spectra for these strange hadrons are presented. The 4π yields and ratios are compared to thermal model and hadronic transport model predictions. At this collision energy, thermal model with grand canonical ensemble (GCE) under-predicts the ϕ/K and ϕ/Ξ ratios while the result of canonical ensemble (CE) calculations reproduce ϕ/K, with the correlation length rc∼2.7 fm, and ϕ/Ξ, rc∼4.2 fm, for the 0-10% central collisions. Hadronic transport models including high mass resonance decays could also describe the ratios. While thermal calculations with GCE work well for strangeness production in high energy collisions, the change to CE at 3 GeV implies a rather different medium property at high baryon density.

Original languageEnglish
Article number137152
JournalPhysics Letters, Section B: Nuclear, Elementary Particle and High-Energy Physics
Volume831
DOIs
StatePublished - Aug 10 2022

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