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K∗0 production in Au+Au collisions at sNN =7.7, 11.5, 14.5, 19.6, 27, and 39 GeV from the RHIC beam energy scan

  • STAR Collaboration
  • American University in Cairo
  • Texas A&M University
  • Czech Technical University in Prague
  • AGH University of Krakow
  • Ohio State University
  • University of Kentucky
  • Panjab University
  • Variable Energy Cyclotron Centre India
  • Brookhaven National Laboratory
  • Abilene Christian University
  • Universidad de Tarapacá
  • University of California at Riverside
  • University of Houston
  • University of Jammu
  • Stony Brook University
  • 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
  • Indiana University Bloomington
  • Warsaw University of Technology
  • Shandong University
  • Fudan University
  • University of Science and Technology of China
  • Tsinghua University
  • University of California at Berkeley
  • Eötvös Loránd University
  • University of Illinois at Chicago
  • Heidelberg University 

Research output: Contribution to journalArticlepeer-review

13 Scopus citations

Abstract

We report the measurement of K∗0 meson at midrapidity (|y|< 1.0) in Au+Au collisions at sNN=7.7, 11.5, 14.5, 19.6, 27, and 39 GeV collected by the STAR experiment during the Relativistic Heavy Ion Collider (RHIC) beam energy scan program. The transverse momentum spectra, yield, and average transverse momentum of K∗0 are presented as functions of collision centrality and beam energy. The K∗0/K yield ratios are presented for different collision centrality intervals and beam energies. The K∗0/K ratio in heavy-ion collisions are observed to be smaller than that in small-system collisions (e+e and p+p). The K∗0/K ratio follows a similar centrality dependence to that observed in previous RHIC and Large Hadron Collider measurements. The data favor the scenario of the dominance of hadronic rescattering over regeneration for K∗0 production in the hadronic phase of the medium.

Original languageEnglish
Article number034907
JournalPhysical Review C
Volume107
Issue number3
DOIs
StatePublished - Mar 2023

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