Abstract

We study the contributions of the resonant states {K}_0^{ast } (1430) and {K}_0^{ast } (1950) in the three-body decays B → Kπh (with h = π, K) in the perturbative QCD approach. The crucial nonperturbative input FKπ(s) in the distribution amplitudes of the S-wave Kπ system is derived from the matrix element of vacuum to Kπ pair. The C P averaged branching fraction of the quasi-two-body decay process B → {K}_0^{ast } (1950) h → Kπh is about one order smaller than that of the corresponding decay B → {K}_0^{ast } (1430)h → Kπh. In view of the important contribution from the S-wave Kπ system for the B → Kπh decays, it is not appropriate to neglect the {K}_0^{ast } (1950) in the theoretical or experimental studies for the relevant three-body B meson decays. The predictions in this work for the relevant decays are consistent with the existing experimental data.

Highlights

  • The kaon-pion scattering has been extensively studied in refs. [74,75,76,77,78,79,80] in recent years

  • We study the contributions of the resonant states K0∗(1430) and K0∗(1950) in the three-body decays B → Kπh in the perturbative QCD approach

  • We will focus on the contributions of the resonant state K0∗(1430) in the B → Kπh decay processes in the PQCD approach based on the kT factorization theorem [107,108,109,110]

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Summary

Framework

The light spectator quark comes from B meson and goes into intermediate state in the hadronization of. = m2K0∗ − is the full width for resonant state K0∗. The twist-2 light-cone distribution amplitude has the form [113, 138, 142]. For the twist-3 light-cone distribution amplitudes in this work, we take the asymptotic forms as φs(z, s) = F√Kπ(s) , 2 2Nc φt(z, s) = F√Kπ(s) (1 − 2z) . The distribution amplitudes for B meson and the bachelor final state h in this work are the same as those widely employed in the studies of the hadronic B meson decays in the PQCD approach, one can find their expressions and parameters in the appendix

Results and discussions
Conclusion
A Decay amplitudes
B PQCD functions
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