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First measurement of coherent ρ0 photoproduction in ultra-peripheral Xe–Xe collisions at sNN=5.44 TeV

  • ALICE Collaboration
  • Variable Energy Cyclotron Centre India
  • Czech Academy of Sciences
  • Goethe University Frankfurt
  • Lund University
  • CERN
  • National Institute for Nuclear Physics
  • Aligarh Muslim University
  • Korea Institute of Science and Technology Information
  • Indonesian Institute of Sciences
  • Russian Research Centre Kurchatov Institute
  • GSI Helmholtz Centre for Heavy Ion Research
  • Universidade Estadual de Campinas
  • Central China Normal University
  • Universidad Nacional Autónoma de México
  • COMSATS University Islamabad
  • University of Houston
  • University of Bergen
  • St. Petersburg State University
  • Horia Hulubei National Institute of Physics and Nuclear Engineering
  • National Institute for Subatomic Physics
  • University of Münster
  • Heidelberg University 
  • Ruder Boskovic Institute
  • Lawrence Berkeley National Laboratory
  • Nantes Université
  • University of Oslo
  • Yale University
  • Laboratoire de Physique des 2 Infinis Irène Joliot-Curie

Research output: Contribution to journalJournal articlepeer-review

Abstract

The first measurement of the coherent photoproduction of ρ0 vector mesons in ultra-peripheral Xe–Xe collisions at sNN=5.44 TeV is presented. This result, together with previous HERA γp data and γ–Pb measurements from ALICE, describes the atomic number (A) dependence of this process, which is particularly sensitive to nuclear shadowing effects and to the approach to the black-disc limit of QCD at a semi-hard scale. The cross section of the Xe+Xe→ρ0+Xe+Xe process, measured at midrapidity through the decay channel ρ0→π+π, is found to be dσ/dy=131.5±5.6(stat.)−16.9+17.5(syst.) mb. The ratio of the continuum to resonant contributions for the production of pion pairs is also measured. In addition, the fraction of events accompanied by electromagnetic dissociation of either one or both colliding nuclei is reported. The dependence on A of cross section for the coherent ρ0 photoproduction at a centre-of-mass energy per nucleon of the γA system of WγA,n=65 GeV is found to be consistent with a power-law behaviour σ(γA→ρ0A)∝Aα with a slope α=0.96±0.02(syst.). This slope signals important shadowing effects, but it is still far from the behaviour expected in the black-disc limit.

Original languageEnglish
Article number136481
JournalPhysics Letters, Section B: Nuclear, Elementary Particle and High-Energy Physics
Volume820
DOIs
StatePublished - 2021.09.10

Quacquarelli Symonds(QS) Subject Topics

  • Physics & Astronomy

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