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Measurement of In-Medium Jet Modification Using Direct Photon+Jet and π0+Jet Correlations in p+p and Central Au+Au Collisions at sNN =200 GeV

  • STAR Collaboration
  • Texas A&M University
  • Czech Technical University in Prague
  • AGH University of Krakow
  • Panjab University
  • Variable Energy Cyclotron Centre India
  • Brookhaven National Laboratory
  • Indian Institute of Technology Patna
  • Abilene Christian University
  • Universidad de Tarapacá
  • Shandong University
  • University of California at Riverside
  • Indian Institute of Science Education and Research, Tirupati
  • University of Houston
  • University of Jammu
  • Stony Brook University
  • Czech Academy of Sciences
  • Ohio State University
  • Chinese Academy of Sciences
  • Yale University
  • University of California at Davis
  • Lawrence Berkeley National Laboratory
  • University of California at Los Angeles
  • Indiana University Bloomington
  • National Institute of Technology, Durgapur
  • Fudan University
  • Guangxi Normal University
  • Tsinghua University
  • University of California at Berkeley
  • Eötvös Loránd University
  • University of Illinois at Chicago

Research output: Contribution to journalArticlepeer-review

3 Scopus citations

Abstract

The STAR Collaboration presents measurements of the semi-inclusive distribution of charged-particle jets recoiling from energetic direct-photon (γdir) and neutral-pion (π0) triggers in p+p and central Au+Au collisions at sNN=200 GeV over a broad kinematic range, for jet resolution parameters R=0.2 and 0.5. Medium-induced jet yield suppression is observed to be larger for R=0.2 than for 0.5, reflecting the angular range of jet energy redistribution due to quenching. The predictions of model calculations incorporating jet quenching are not fully consistent with the observations. These results provide new insight into the physical origins of jet quenching.

Original languageEnglish
Article number232301
JournalPhysical Review Letters
Volume134
Issue number23
DOIs
StatePublished - Jun 13 2025

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