Abstract

We present the first analytic mathcal{O}left({alpha}_sright) -computation at twist-1,2 of the {overline{B}}_{u,d,s} → γ form factors within the framework of sum rules on the light-cone. These form factors describe the charged decay {overline{B}}_uto gamma {mathrm{ell}}^{-}overline{v} , contribute to the flavour changing neutral currents {overline{B}}_{d,s}to gamma {mathrm{ell}}^{+}{mathrm{ell}}^{-} and serve as inputs to more complicated processes. We provide a fit in terms of a z-expansion with correlation matrix and extrapolate the form factors to the kinematic endpoint by using the gBB*γ couplings as a constraint. Analytic results are available in terms of multiple polylogarithms in the supplementary material. We give binned predictions for the {overline{B}}_uto gamma {mathrm{ell}}^{-}overline{v} branching ratio along with the associated correlation matrix. By comparing with three SCET-computations we extract the inverse moment B-meson distribution amplitude parameter λB = 360(110) MeV. The uncertainty thereof could be improved by a more dedicated analysis. In passing, we extend the photon distribution amplitude to include quark mass corrections with a prescription for the magnetic vacuum susceptibility, χq, compatible with the twist-expansion. The values χq = 3.21(15) GeV−2 and χs = 3.79(17) GeV−2 are obtained.

Highlights

  • In this work we provide the on-shell form factors contributing to semileptonic Bu → γ −νand flavour changing neutral decay (FCNC) Bd,s → γ + − with the method of light-cone sum rules (LCSR)

  • The dynamics, contrary to naive expectation, are more involved than for B → V (ρ, ω, K∗, φ) [1, 2]. This comes as the point-like photon, of leading twist-1, has no counterpart for the mesons and yet the photon is to be described by a photon distribution amplitude (DA)

  • Together with the fit-values given in table 4 of the previous section and the correlation matrix given in the supplementary material this constitutes the main practical results of our paper

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Summary

Introduction

In this work we provide the (photon) on-shell form factors contributing to semileptonic Bu → γ −νand flavour changing neutral decay (FCNC) Bd,s → γ + − with the method of light-cone sum rules (LCSR) This is the first complete next-to leading order (NLO) computation in αs including twist-1,2 and leading order (LO) twist-3 and partial twist-4. These form factors had been considered, in LCSR at LO [30], in [31] using aspects of heavy quark symmetry (with input from [32]), quark model computations [27, 33] and more recently in SCET [28] In this decay, the dipole operator mbqLσ·F b necessitates photon off-shell form factors. We provide the method-independent information on the B → γ form factors (FFs), such as the definition and the heavy quark scaling

Definition of the form factors
Form factor conventions in the literature
Heavy quark scaling of form factors
Definition of the correlation function appropriate for the sum rule
QED and axial Ward identity
The computation
Leading order
Next-to-leading order
Quark mass correction to the photon distribution amplitude
Comparison of form factor computation with the literature
Equations of motion as a test of the computation
Numerics
Equations of motion as constraints on sum rule parameters
Fit-ansatz
Results and plots
Comparison with the literature
Extraction of the inverse moment λB of the B-meson DA
Summary and discussions
A Conventions and additional plots
Borel transformation
Plots of scale dependence and twist-contributions
Leading order correlation functions We introduce the following shorthands
Full Text
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