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Bulk properties of the system formed in Au+Au collisions at sNN =14.5 GeV at the BNL STAR detector

  • STAR Collaboration
  • Brookhaven National Laboratory
  • AGH University of Krakow
  • Ohio State University
  • University of Kentucky
  • Kent State University
  • Joint Institute for Nuclear Research
  • Panjab University
  • Variable Energy Cyclotron Centre
  • Russian Research Centre Kurchatov Institute
  • Moscow Engineering Physics Institute
  • Texas A&M University
  • Central China Normal University
  • National Institute of Science Education and Research
  • University of California at Riverside
  • Stony Brook University
  • University of Houston
  • University of Jammu
  • Czech Technical University in Prague
  • Czech Academy of Sciences
  • Shandong University
  • Rice University
  • Yale University
  • University of California at Davis
  • University of California at Los Angeles
  • National Cheng Kung University
  • Fudan University
  • University of Science and Technology of China
  • Tsinghua University
  • Creighton University
  • University of California at Berkeley
  • Eötvös Loránd University
  • Abilene Christian University
  • Heidelberg University 
  • Institute for High Energy Physics
  • Lawrence Berkeley National Laboratory
  • Purdue University
  • Wayne State University
  • University of Tsukuba
  • Lehigh University
  • Southern Connecticut State University
  • Technische Universität Darmstadt
  • Valparaiso University
  • Indian Institute of Science Education and Research, Tirupati
  • American University in Cairo
  • Chinese Academy of Sciences
  • Pennsylvania State University
  • Indiana University Bloomington
  • Warsaw University of Technology
  • Goethe University Frankfurt
  • Argonne National Laboratory
  • Temple University
  • University of Texas at Austin
  • Rutgers - The State University of New Jersey, New Brunswick
  • Indian Institute of Science Education and Research, Berhampur
  • Max Planck Institute for Physics (Werner Heisenberg Institute)
  • Indian Institute of Technology Patna
  • Universidade de São Paulo
  • Huzhou University
  • Michigan State University
  • United States Naval Academy

Producción científica: Contribución a una revistaArtículorevisión exhaustiva

45 Citas (Scopus)

Resumen

We report systematic measurements of bulk properties of the system created in Au+Au collisions at sNN=14.5 GeV recorded by the STAR detector at the Relativistic Heavy Ion Collider (RHIC). The transverse momentum spectra of π±, K±, and p(p) are studied at midrapidity (|y|<0.1) for nine centrality intervals. The centrality, transverse momentum (pT), and pseudorapidity (η) dependence of inclusive charged particle elliptic flow (v2), and rapidity-odd charged particles directed flow (v1) results near midrapidity are also presented. These measurements are compared with the published results from Au+Au collisions at other energies, and from Pb+Pb collisions at sNN=2.76 TeV. The results at sNN=14.5 GeV show similar behavior as established at other energies and fit well in the energy dependence trend. These results are important as the 14.5-GeV energy fills the gap in μB, which is of the order of 100 MeV, between sNN=11.5 and 19.6 GeV. Comparisons of the data with UrQMD and AMPT models show poor agreement in general.

Idioma originalInglés
Número de artículo024905
PublicaciónPhysical Review C
Volumen101
N.º2
DOI
EstadoPublicada - feb. 2020
Publicado de forma externa

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