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Light nuclei collectivity from sNN=3 GeV Au+Au collisions at RHIC

  • 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
  • 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
  • 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
  • Indian Institute of Science Education and Research, Berhampur
  • Rice University
  • University of Tsukuba
  • University of Illinois at Chicago
  • Lehigh University
  • University of Calabria
  • Purdue University
  • Southern Connecticut State University
  • Technische Universität Darmstadt
  • Temple University
  • Valparaiso University
  • Indian Institute of Science Education and Research, Tirupati
  • CAS - Institute of Modern Physics
  • 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
  • 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
  • United States Naval Academy

Producción científica: Contribución a una revistaArtículorevisión exhaustiva

48 Citas (Scopus)

Resumen

In high-energy heavy-ion collisions, partonic collectivity is evidenced by the constituent quark number scaling of elliptic flow anisotropy for identified hadrons. A breaking of this scaling and dominance of baryonic interactions is found for identified hadron collective flow measurements in sNN = 3 GeV Au+Au collisions. In this paper, we report measurements of the first- and second-order azimuthal anisotropic parameters, v1 and v2, of light nuclei (d, t, 3He, 4He) produced in sNN = 3 GeV Au+Au collisions at the STAR experiment. An atomic mass number scaling is found in the measured v1 slopes of light nuclei at mid-rapidity. For the measured v2 magnitude, a strong rapidity dependence is observed. Unlike v2 at higher collision energies, the v2 values at mid-rapidity for all light nuclei are negative and no scaling is observed with the atomic mass number. Calculations by the Jet AA Microscopic Transport Model (JAM), with baryonic mean-field plus nucleon coalescence, are in good agreement with our observations, implying baryonic interactions dominate the collective dynamics in 3 GeV Au+Au collisions at RHIC.

Idioma originalInglés
Número de artículo136941
PublicaciónPhysics Letters, Section B: Nuclear, Elementary Particle and High-Energy Physics
Volumen827
DOI
EstadoPublicada - 10 abr 2022

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