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Observation of an alternative χc0(2P) candidate in e+e−→J/ψDD¯

  • (Belle Collaboration)
  • RAS - P.N. Lebedev Physics Institute
  • Moscow Engineering Physics Institute
  • The Graduate University for Advanced Studies
  • High Energy Accelerator Research Organization, Tsukuba
  • The University of Tokyo
  • King Abdulaziz University
  • University of Tabuk
  • Pacific Northwest National Laboratory
  • RAS - Budker Institute of Nuclear Physics
  • Novosibirsk State University
  • Tata Institute of Fundamental Research
  • King Abdulaziz City for Science and Technology
  • The University of Sydney
  • University of Melbourne
  • Indian Institute of Science Education and Research Mohali
  • Indian Institute of Technology Guwahati
  • Jožef Stefan Institute
  • H. Niewodniczanski Institute of Nuclear Physics
  • University of Maribor
  • University of Hawai'i at Mānoa
  • Charles University
  • Max Planck Institute for Physics (Werner Heisenberg Institute)
  • National Central University
  • Hanyang University
  • Korea Institute of Science and Technology Information
  • Sungkyunkwan University
  • Wayne State University
  • Indian Institute of Technology Bhubaneswar
  • German Electron Synchrotron
  • Virginia Polytechnic Institute and State University
  • Karlsruhe Institute of Technology
  • Niigata University
  • National Taiwan University

Research output: Contribution to journalArticlepeer-review

99 Scopus citations

Abstract

We perform a full amplitude analysis of the process e+e-→J/ψDD, where D refers to either D0 or D+. A new charmoniumlike state X∗(3860) that decays to DD is observed with a significance of 6.5σ. Its mass is (3862-32+26 -13+40) MeV/c2, and its width is (201-67+154 -82+88) MeV. The JPC=0++ hypothesis is favored over the 2++ hypothesis at the level of 2.5σ. The analysis is based on the 980 fb-1 data sample collected by the Belle detector at the asymmetric-energy e+e- collider KEKB.

Original languageEnglish
Article number112003
JournalPhysical Review D
Volume95
Issue number11
DOIs
StatePublished - 1 Jun 2017

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