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Probing parton dynamics of QCD matter with Ω and φ production

  • STAR Collaboration
  • AGH University of Krakow
  • University of Kentucky
  • Joint Institute for Nuclear Research
  • Panjab University
  • Kent State University
  • Brookhaven National Laboratory
  • Variable Energy Cyclotron Centre
  • Alikhanov Institute for Theoretical and Experimental Physics
  • Central China Normal University
  • National Institute of Science Education and Research
  • University of Houston
  • University of Jammu
  • University of Texas at Austin
  • Czech Technical University in Prague
  • Czech Academy of Sciences
  • Rice University
  • Moscow Engineering Physics Institute
  • Yale University
  • University of California at Davis
  • Ohio State University
  • Texas A&M University
  • Chinese Academy of Sciences
  • CAS - Institute of Modern Physics
  • Tsinghua University
  • Creighton University
  • Lawrence Berkeley National Laboratory
  • University of California at Berkeley
  • Institute of Physics Bhubaneswar
  • Shandong University
  • Institute for High Energy Physics
  • Pennsylvania State University
  • Valparaiso University
  • University of California at Los Angeles
  • University of Illinois at Chicago
  • Purdue University
  • Warsaw University of Technology
  • Temple University
  • University of Science and Technology of China
  • National Cheng Kung University
  • Indiana University Bloomington
  • Korea Institute of Science and Technology Information
  • Wayne State University
  • Goethe University Frankfurt
  • Argonne National Laboratory
  • Stony Brook University
  • Indian Institute of Technology Bombay
  • Michigan State University
  • Pusan National University
  • Institute of Nuclear Physics PAN
  • University of Rajasthan
  • Max Planck Institute for Physics (Werner Heisenberg Institute)
  • World Laboratory for Cosmology and Particle Physics (WLCAPP)
  • United States Naval Academy

Producción científica: Contribución a una revistaArtículorevisión exhaustiva

65 Citas (Scopus)

Resumen

We present measurements of Ω and φ production at midrapidity from Au+Au collisions at nucleon-nucleon center-of-mass energies sNN=7.7, 11.5, 19.6, 27, and 39 GeV by the STAR experiment at the BNL Relativistic Heavy Ion Collider (RHIC). Motivated by the coalescence formation mechanism for these strange hadrons, we study the ratios of N(Ω-+Ω#x0002B;)/[2N(φ)]. These ratios as a function of transverse momentum pT fall on a consistent trend at high collision energies, but start to show deviations in peripheral collisions at sNN=19.6, 27, and 39 GeV, and in central collisions at 11.5 GeV in the intermediate pT region of 2.4-3.6 GeV/c. We further evaluate empirically the strange quark pT distributions at hadronization by studying the Ω/φ ratios scaled by the number of constituent quarks (NCQ). The NCQ-scaled Ω/φ ratios show a suppression of strange quark production in central collisions at 11.5 GeV compared to sNN≥19.6 GeV. The shapes of the presumably thermal strange quark distributions in 0-60% most central collisions at 7.7 GeV show significant deviations from those in 0-10% most central collisions at higher energies. These features suggest that there is likely a change of the underlying strange quark dynamics in the transition from quark matter to hadronic matter at collision energies below 19.6 GeV.

Idioma originalInglés
Número de artículo021903
PublicaciónPhysical Review C
Volumen93
N.º2
DOI
EstadoPublicada - 24 feb 2016
Publicado de forma externa

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