Higher Charmonia

By T.Barnes, S.Godfrey, E. D. O. Physics, Astronomy, U. Tennessee, P. Division, Oak Ridge National Laboratory, Ottawa-Carleton Institute for Physics, D. Physics, Carleton University and 3 more. 2005

476 citations recorded by the source corpus.

This paper gives results for the spectrum, all allowed E1 radiative partial widths (and some important M1 widths) and all open-charm strong decay amplitudes of all 40 c-cbar states expected up to the mass of the 4S multiplet, just above 4.4 GeV. The spectrum and radiative widths are evaluated using two models, the relativized Godfrey-Isgur model and a nonrelativistic potential model. The electromagnetic transitions are evaluated using Coulomb plus linear plus smeared hyperfine wavefunctions, both in a nonrelativistic potential model and in the Godfrey-Isgur model. The open-flavor strong decay amplitudes are determined assuming harmonic oscillator wavefunctions and the 3P0 decay model. This work is intended to motivate future experimental studies of higher-mass charmonia, and may be useful for the analysis of high-statistics data sets to be accumulated by the BES, CLEO and GSI facilities.

Subfields: Nuclear and High Energy Physics

View Paper: https://www.semanticscholar.org/paper/02d7a93c6858a7ed0e8c4810f38018464e5b5103

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In Nuclear and High Energy Physics

  1. S. Olsen
  2. Xiang Liu
  3. T. Skwarnicki
  4. S. Godfrey
  5. E. Swanson
  6. R. Mitchell
  7. Shi-Lin Zhu
  8. Alessandro Pilloni

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