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Measurements of Proton High-Order Cumulants in sNN =3 GeV Au+Au Collisions and Implications for the QCD Critical Point

  • (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 India
  • Russian Research Centre Kurchatov Institute
  • National Research Nuclear 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
  • 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

Research output: Contribution to journalArticlepeer-review

75 Scopus citations

Abstract

We report cumulants of the proton multiplicity distribution from dedicated fixed-target Au+Au collisions at sNN=3.0 GeV, measured by the STAR experiment in the kinematic acceptance of rapidity (y) and transverse momentum (pT) within -0.5<y<0 and 0.4<pT<2.0 GeV/c. In the most central 0%-5% collisions, a proton cumulant ratio is measured to be C4/C2=-0.85±0.09 (stat)±0.82 (syst), which is 2σ below the Poisson baseline with respect to both the statistical and systematic uncertainties. The hadronic transport UrQMD model reproduces our C4/C2 in the measured acceptance. Compared to higher energy results and the transport model calculations, the suppression in C4/C2 is consistent with fluctuations driven by baryon number conservation and indicates an energy regime dominated by hadronic interactions. These data imply that the QCD critical region, if created in heavy-ion collisions, could only exist at energies higher than 3 GeV.

Original languageEnglish
Article number202303
JournalPhysical Review Letters
Volume128
Issue number20
DOIs
StatePublished - May 20 2022

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