Next-to-leading-order QCD calculations of form factors with higher-twist corrections
arXiv:2504.13649 · doi:10.1103/k5qy-rc5j
Abstract
Applying the light-cone sum rules (LCSR) approach, the next-to-leading-order (NLO) corrections to form factors are calculated with the twist-two and twist-three meson light-cone distribution amplitudes (LCDAs) at leading power in . At one-loop level, the vacuum-to--meson correlation functions defined with interpolating currents for the -wave axial-vector meson are factorized into short-distance coefficients and the distribution amplitudes (DAs) of the meson, among which the hard coefficients for A0-type currents and dependent jet functions entering correlation functions , and are identical to the corresponding ones of in SCET. In addition, and coincide with the results of under the limit up to one-loop accuracy. Then the subleading power corrections to form factors are computed with the higher-twist meson LCDAs at tree level up to the twist-six accuracy. Furthermore, we predict the dependence of form factors via the Bourrely-Caprini-Lellouch (BCL) -series expanding parameterization to compute several physical observables including branching ratios of semileptonic and processes, transverse asymmetries, forward-backward asymmetries and lepton flavor universality observables employing the given mixing angles , , . We also compare our theory calculations with the results from other methods.
70 pages, 23 figures, 23 tables
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