Abstract
An exploratory study of charmless 3-body decays of mesons is presented using a simple model based on the framework of the factorization approach. The nonresonant contributions arising from transitions are evaluated using heavy meson chiral perturbation theory (HMChPT). The momentum dependence of nonresonant amplitudes is assumed to be in the exponential form so that the HMChPT results are recovered in the soft meson limit . In addition, we have identified another large source of the nonresonant signal in the matrix elements of scalar densities, e.g. , which can be constrained from the decay or . The intermediate vector-meson contributions to 3-body decays are identified through the vector current, while the scalar meson resonances are mainly associated with the scalar density. Their effects are described in terms of the Breit-Wigner formalism. Our main results are: (i) All modes are dominated by the nonresonant background. The predicted branching ratios of , and modes are consistent with the data within errors. (ii) Although the penguin-dominated decay is subject to a potentially significant tree pollution, its effective is very similar to that of the mode. However, direct asymmetry of the former, being of order , is more prominent than the latter. (iii) For decays, we found sizable nonresonant contributions in and modes, in agreement with the Belle measurements but larger than the BABAR result. (iv) Time-dependent asymmetries in , a purely -even state, and , an admixture of -even and -odd components, are studied. (v) The mode is found to have a rate larger than even though the former involves a in the final state. They are both dominated by resonant contributions. (vi) We have computed the resonant contributions to 3-body decays and determined the rates for the quasi-two-body decays and . The predicted , and rates are in agreement with the data, while the calculated , , and are in general too small compared to experiment. (vii) Sizable direct asymmetry is found in and modes.
- Received 10 April 2007
DOI:https://doi.org/10.1103/PhysRevD.76.094006
©2007 American Physical Society