Radiative hc/b decays to η or η

Ruilin Zhu and Jian-Ping Dai
Phys. Rev. D 94, 094034 – Published 28 November 2016

Abstract

Motivated by recent measurements of the radiative decay rates of the P-wave spin singlet charmonium hc to the light meson η or η by the BESIII Collaboration, we investigate the decay rates of these channels at order ααs4. The photon is radiated mainly from charm quark pairs in the lowest-order Feynman diagrams, because the diagrams where a photon radiated from light quarks are suppressed by αs or the relative charm quark velocity v, due to charge-parity conservation. The form factors of two gluons to η or η, which are the major mechanism for η and η production, are employed. η(η) is treated as a light-cone object when we consider that the parent charmonium mass is much heavier than that of the final light meson. We obtain the branching ratio B(hcγη)=(1.940.51+0.70)×103 in the nonrelativistic QCD approach, which is in agreement with the BESIII measurement. The prediction of the branching ratio of hcγη is also within the range of experimental error after including the larger uncertainty of the total decay width Γhc. The applications of these formulas to the radiative decays to η(η) of the P-wave spin singlet bottomonium hb(nP) are presented. These studies will shed some light on the ηη mixing effects, the flavor SU(3) symmetry breaking, and the nonperturbative dynamics of charmonium and bottomonium.

  • Figure
  • Figure
  • Received 4 October 2016

DOI:https://doi.org/10.1103/PhysRevD.94.094034

© 2016 American Physical Society

Physics Subject Headings (PhySH)

Particles & Fields

Authors & Affiliations

Ruilin Zhu*

  • Department of Physics and Institute of Theoretical Physics, Nanjing Normal University, Nanjing, Jiangsu 210023, China

Jian-Ping Dai

  • INPAC, Shanghai Key Laboratory for Particle Physics and Cosmology, Department of Physics and Astronomy, Shanghai Jiao-Tong University, Shanghai 200240, China

  • *rlzhu@njnu.edu.cn
  • daijianping@ihep.ac.cn

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Issue

Vol. 94, Iss. 9 — 1 November 2016

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