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Flow and interferometry results from Au+Au collisions at sNN =4.5 GeV

  • STAR Collaboration
  • American University in Cairo
  • Brookhaven National Laboratory
  • AGH University of Krakow
  • Ohio State University
  • University of Kentucky
  • 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
  • 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
  • University of Science and Technology of China
  • Tsinghua University
  • University of California at Berkeley
  • Eötvös Loránd University
  • Abilene Christian University
  • Heidelberg University 
  • Institute for High Energy Physics
  • Wayne State University
  • University of Tsukuba
  • University of Illinois at Chicago
  • Lehigh University
  • Purdue University
  • Southern Connecticut State University
  • Technische Universität Darmstadt
  • Temple University
  • Valparaiso University
  • Indian Institute of Science Education and Research, Tirupati
  • Pennsylvania State University
  • Indiana University Bloomington
  • Warsaw University of Technology
  • Goethe University Frankfurt
  • National Institute of Science Education and Research
  • University of Texas at Austin
  • Rutgers - The State University of New Jersey, New Brunswick
  • Indian Institute of Science Education and Research, Berhampur
  • Institute of Nuclear Physics PAN
  • Max Planck Institute for Physics (Werner Heisenberg Institute)
  • Creighton University
  • Indian Institute of Technology Patna
  • Argonne National Laboratory
  • Universidade de São Paulo
  • Huzhou University
  • Michigan State University

Producción científica: Contribución a una revistaArtículorevisión exhaustiva

47 Citas (Scopus)

Resumen

The beam energy scan (BES) program at the BNL Relativistic Heavy Ion Collider (RHIC) was extended to energies below sNN=7.7 GeV in 2015 by successful implementation of the fixed-target mode of operation in the STAR (Solenoidal Tracker At RHIC) experiment. In this mode, ions circulate in one ring of the collider and interact with a stationary target at the entrance of the STAR time projection chamber. The first results for Au+Au collisions at sNN=4.5 GeV are presented, demonstrating good performance of all the relevant detector subsystems in fixed-target mode. Results presented here include directed and elliptic flow of identified hadrons, and radii from pion femtoscopy. The latter, together with recent HADES results, reveal a long-sought peak structure that may be caused by the system evolving through a first-order phase transition from quark-gluon plasma to the hadronic phase. Directed and elliptic flow for pions are presented for the first time at this beam energy. Pion and proton elliptic flow show behavior which hints at constituent quark scaling, and demonstrate that a definitive conclusion will be achievable using the full statistics of the ongoing second phase of BES (BES-II). In particular, BES-II to date has recorded fixed-target data sets with two orders of magnitude more events at each of nine energies between sNN=3.0 and 7.7 GeV.

Idioma originalInglés
PublicaciónPhysical Review C
Volumen103
N.º3
DOI
EstadoPublicada - mar. 2021

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