Abstract
Hadronic B decays containing an even-parity charmed meson in the final state are studied. Specifically we focus on the Cabibbo-allowed decays and where denotes generically a p-wave charmed meson. The transition form factors are studied in the improved version of the Isgur-Scora-Grinstein-Wise quark model. We apply heavy quark effective theory and chiral symmetry to study the strong decays of p-wave charmed mesons and determine the magnitude of the mixing angle (the superscript standing for the total angular momentum of the light quark). Except for the decay to the predictions of agree with experiment. The sign of the mixing angle is found to be positive in order to avoid a severe suppression of the production of The interference between color-allowed and color-suppressed tree amplitudes is expected to be destructive in the decay Hence, an observation of the ratio can be used to test the relative signs of various form factors as implied by heavy quark symmetry. Although the predicted at the level of exceeds the present upper limit, it leads to the ratio as expected from the factorization approach and from the ratio Therefore, it is crucial to have a measurement of this mode to test the factorization hypothesis. For decays, it is expected that as the decay constants of the multiplet become the same in the heavy quark limit. The preliminary Belle observation of fairly less abundant production of than is thus a surprise. What is the cause for the discrepancy between theory and experiment remains unclear. Meanwhile, it is also important to measure the B decay into to see if it is suppressed relative to to test the heavy quark symmetry relation Under the factorization hypothesis, the production of is prohibited as the tensor meson cannot be produced from the current. Nevertheless, it can be induced via final-state interactions or nonfactorizable contributions and hence an observation of could imply the importance of final-state rescattering effects.
- Received 15 July 2003
DOI:https://doi.org/10.1103/PhysRevD.68.094005
©2003 American Physical Society