Higher Charmonia
Higher Charmonia
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.
S. Godfrey、E. S. Swanson、T. Barnes
Ottawa-Carleton Institute for Physics, Department of Physics, Carleton UniversityRudolph Peierls Centre for Theoretical Physics, Oxford UniversityDepartment of Physics and Astronomy, University of Tennessee
物理学
S. Godfrey,E. S. Swanson,T. Barnes.Higher Charmonia[EB/OL].(2005-04-29)[2025-08-02].https://arxiv.org/abs/hep-ph/0505002.点此复制
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