Higher charmonia

被引:660
作者
Barnes, T [1 ]
Godfrey, S
Swanson, ES
机构
[1] Univ Tennessee, Dept Phys & Astron, Knoxville, TN 37996 USA
[2] Oak Ridge Natl Lab, Div Phys, Oak Ridge, TN 37831 USA
[3] Carleton Univ, Dept Phys, Ottawa Carleton Inst Phys, Ottawa, ON K1S 5B6, Canada
[4] Univ Oxford, Rudolph Peierls Ctr Theoret Phys, Oxford OX1 3NP, England
来源
PHYSICAL REVIEW D | 2005年 / 72卷 / 05期
基金
美国国家科学基金会;
关键词
D O I
10.1103/PhysRevD.72.054026
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
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 (c) over bar 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 wave functions, both in a nonrelativistic potential model and in the Godfrey-Isgur model. The open-flavor strong decay amplitudes are determined assuming harmonic oscillator wave functions and the P-3(0) 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.
引用
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页数:20
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