S-D mixing and production in annihilation and B decay and its radiative transitions
arXiv:hep-ph/0405126 · doi:10.1103/PhysRevD.70.094001
Abstract
The large decay rate observed by Belle for , which is comparable to , might indicate either an unexpectedly large S-D mixing angle or the leading role of the color-octet mechanism in D-wave charmonium production in B decay. By calculating the production rate of in the continuum annihilation at GeV with these two possible approaches (i.e. the large S-D mixing and the color-octet mechanism), we show that the measurement for this process at Belle and BaBar may provide a clear cut clarification for the two approaches. In addition, the radiative E1 transition ratio may dramatically change from 0.04 (for ) to 200 (for ) due to the large S-D interference effect, thus the E1 transition measurement of at BES and CLEO-c will also be very useful in clarifying this issue.
arXiv commentfinal version to appear in Phys.Rev.D, discussion on uncertainties associated with the color-octet matrix elements is added, 16 pages, 2 figures
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Cited by in corpus (8)
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- The mass spectrum and wave functions of the system
- Modeling Charmonium- Decays of Higher Charmonia
- Possible large branching fraction of psi(3770) decays to charmless final states
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