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Study of the near-threshold ω mass enhancement in doubly OZI-suppressed J/ψ→γω decays

  • M. Ablikim
  • , M. N. Achasov
  • , O. Albayrak
  • , D. J. Ambrose
  • , F. F. An
  • , Q. An
  • , J. Z. Bai
  • , Y. Ban
  • , J. Becker
  • , J. V. Bennett
  • , M. Bertani
  • , J. M. Bian
  • , E. Boger
  • , O. Bondarenko
  • , I. Boyko
  • , R. A. Briere
  • , V. Bytev
  • , X. Cai
  • , O. Cakir
  • , A. Calcaterra
  • G. F. Cao, S. A. Cetin, J. F. Chang, G. Chelkov, G. Chen, H. S. Chen, J. C. Chen, M. L. Chen, S. J. Chen, X. Chen, Y. B. Chen, H. P. Cheng, Y. P. Chu, D. Cronin-Hennessy, H. L. Dai, J. P. Dai, D. Dedovich, Z. Y. Deng, A. Denig, I. Denysenko, M. Destefanis, W. M. Ding, Y. Ding, L. Y. Dong, M. Y. Dong, S. X. Du, J. Fang, S. S. Fang, H. Muramatsu, R. Poling, BESIII Collaboration

Research output: Contribution to journal › Article › peer-review

Abstract

A 2.25×108 J/ψ event sample accumulated with the BESIII detector is used to study the doubly Okubo-Zweig-Iizuka-suppressed decay modes J/ψ→γω, ω→π+π-π0, →K+K-. A strong deviation (>30σ) from three-body J/ψ→γω phase space is observed near the ω mass threshold that is consistent with a previous observation reported by the BESII experiment. A partial wave analysis with a tensor covariant amplitude that assumes that the enhancement is due to the presence of a resonance, the X(1810), is performed and confirms that the spin-parity of the X(1810) is 0 ++. The mass and width of the X(1810) are determined to be M=1795±7(stat)-5+13(syst)±19(mod) MeV/c2 and Γ= 95±10(stat)-34+21(syst)±75(mod) MeV/c2, respectively, and the product branching fraction is measured to be B(J/ψ→γX(1810)) ×B(X(1810)→ω)=(2.00±0.08(stat)-1.00+0.45(syst)±1. 30(mod))×10-4. These results are consistent within errors with those of the BESII experiment.

Original languageEnglish (US)
Article number032008
JournalPhysical Review D - Particles, Fields, Gravitation and Cosmology
Volume87
Issue number3
DOIs
StatePublished - Feb 22 2013

Bibliographical note

Publisher Copyright:
© 2013 American Physical Society.

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