Next-to-leading-order QCD calculations of B A form factors with higher-twist corrections
Abstract
Applying the light-cone sum rules (LCSR) approach, the next-to-leading-order (NLO) corrections to B A form factors are calculated with the twist-two and twist-three B meson light-cone distribution amplitudes (LCDAs) at leading power in / mb. At one-loop level, the vacuum-to-B-meson correlation functions defined with interpolating currents for the p-wave axial-vector meson are factorized into short-distance coefficients and the distribution amplitudes (DAs) of the B meson, among which the hard coefficients for A0-type currents and μ dependent jet functions entering correlation functions μ,\|(T+T), δμ,(V-A) and δμ,(T+T) are identical to the corresponding ones of B V in SCET. In addition, μ,\|(V-A) and μ,\|(T+T) coincide with the results of B π,K under the limit mq 0 up to one-loop accuracy. Then the subleading power corrections to B A form factors are computed with the higher-twist B meson LCDAs at tree level up to the twist-six accuracy. Furthermore, we predict the q2 dependence of B A form factors via the Bourrely-Caprini-Lellouch (BCL) z-series expanding parameterization to compute several physical observables including branching ratios of semileptonic B A and B A processes, transverse asymmetries, forward-backward asymmetries and lepton flavor universality observables employing the given mixing angles θK=-34, θ1P1=28, θ3P1=23. We also compare our theory calculations with the results from other methods.
Turn this paper into a full lesson
ArcXiv compiles a staged curriculum from this paper: 8-12 lessons across beginner → advanced, synthesised section guides, visuals, flashcards, a quiz, exercises, and on-demand deep dives per section. Grounded in the abstract, never invented.