Title

Inclusive (2P) production in (3S) decay

Authors

R. Morrison, University of California, Santa Barbara
D. Schmidt, University of California, Santa Barbara
M. Procario, University of California, Santa Barbara
D. R. Johnson, University of California, Santa Barbara
K. Lingel, University of California, Santa Barbara
P. Rankin, University of California, Santa Barbara
J. G. Smith, University of California, Santa Barbara
J. Alexander, University of California, Santa Barbara
M. Artuso, University of California, Santa Barbara
C. Bebek, University of California, Santa Barbara
K. Berkelman, University of California, Santa Barbara
D. Besson, University of California, Santa Barbara
T. E. Browder, University of California, Santa Barbara
D. G. Cassel, University of California, Santa Barbara
E. Cheu, University of California, Santa Barbara
D. M. Coffman, University of California, Santa Barbara
P. S. Drell, University of California, Santa Barbara
R. Ehrlich, University of California, Santa Barbara
R. S. Galik, University of California, Santa Barbara
M. Garcia-Sciveres, University of California, Santa Barbara
B. Geiser, University of California, Santa Barbara
B. Gittelman, University of California, Santa Barbara
S. W. Gray, University of California, Santa Barbara
D. L. Hartill, University of California, Santa Barbara
B. K. Heltsley, University of California, Santa Barbara
K. Honscheid, University of California, Santa Barbara
J. Kandaswamy, University of California, Santa Barbara
N. Katayama, University of California, Santa Barbara
D. L. Kreinick, University of California, Santa Barbara
J. D. Lewis, University of California, Santa Barbara
G. S. Ludwig, University of California, Santa Barbara

Document Type

Article

Publication Date

1-1-1991

Abstract

Using the CsI calorimeter of the CLEO II detector, the spin triplet b(2P) states are observed in (3S) radiative decays with much higher statistics than seen in previous experiments. The observed mass splittings are not described well by theoretical models, while the relative branching ratios agree with predictions that include relativistic corrections to the radiative transition rates. © 1991 The American Physical Society.

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