Power Corrections in Charmless Nonleptonic B-Decays: Annihilation is Factorizable and Real
Christian M. Arnesen, Zoltan Ligeti, Ira Z. Rothstein, Iain W. Stewart
TL;DR
This paper uses soft-collinear effective theory (SCET) to classify LambdaQCD/mb power corrections in charmless nonleptonic B decays and to show that leading annihilation amplitudes are real, with complex strong phases arising only at higher orders. It provides a complete factorization framework for both local and chirally enhanced annihilation, including a full basis of SCET$_{II}$ operators and a real, convergent convolution structure with twist-2 and twist-3 meson distributions. The authors show that nonperturbative strong phases are suppressed unless the intermediate scale is poorly behaved, and they quantify annihilation’s small but non-negligible role in penguin amplitudes for modes like B→Kπ and B→KK. Simple numerical modeling within this framework yields annihilation contributions at the 10–15% level of the penguin amplitude, consistent with power-counting expectations and offering constraints on prior phenomenological approaches. Overall, the work provides a rigorous, scale-separated description of annihilation effects and their weak-phase content, aiding interpretation of CP asymmetries and guiding future fits to data.
Abstract
We classify LambdaQCD/mb power corrections to nonleptonic B-> M1 M2 decays, where M1 and M2 are charmless non-isosinglet mesons. Using recent developments in soft-collinear effective theory, we prove that the leading contributions to annihilation amplitudes of O[alphas(mb) LambdaQCD/mb] are real. The leading annihilation amplitudes depend on twist-2 and twist-3 three parton distributions. A complex nonperturbative parameter from annihilation first appears at O[alphas^2(sqrt{Lambda mb}) LambdaQCD/mb]. ``Chirally enhanced'' contributions are also factorizable and real at lowest order. Thus, incalculable strong phases are suppressed in annihilation amplitudes, unless the alphas(sqrt{Lambda mb}) expansion breaks down. Modeling the distribution functions, we find that (11 +- 9)% and (15 +- 11)% of the absolute value of the measured B-> K- pi+ and B-> K- K0 penguin amplitudes come from annihilation. This is consistent with the expected size of power corrections.
