QCD analysis of $B \to \pi\pi$ form factors and the $\vert V_{ub} \vert$ extraction from $B_{l4}$ decays

TL;DR

This paper presents a novel QCD analysis of $B o ho ho$ form factors using light-cone sum rules, deriving twist-three two-pion distribution amplitudes, and extracting $|V_{ub}|$ from $B_{l4}$ decays with improved precision.

Contribution

It introduces the first systematic calculation of higher-power corrections to $B o ho ho$ form factors via explicit twist-three two-pion DAs derived from conformal symmetry.

Findings

Extracted $|V_{ub}|$ with reduced uncertainties from $B_{l4}$ decays.

Clarified the impact of finite width and nonresonant effects on $|V_{ub}|$ from $B o ho l u$.

Provided new insights into $ ho$ resonance effects in semileptonic B decays.

Abstract

The $B_{l4}$ decays offer an independent method for determining the Cabibbo-Kobayashi-Maskawa matrix element $\vert V_{ub} \vert$, with a QCD analysis of the underlying $B \to \pi\pi$ form factors serving as a crucial component. We present a comprehensive QCD analysis of the $B \to \pi\pi$ form factors within the framework of light-cone sum rules, employing two-pion light-cone distribution amplitudes. For the first time, we derive the twist-three $2\pi$DAs explicitly by exploiting the conformal symmetry of massless QCD. This breakthrough enables the first systematic calculation of higher-power corrections to the $B \to \pi\pi$-type transitions. Leveraging the recently measured partial decay fractions of $B^+ \to \pi^+\pi^- l^+ \nu_l$ by the Belle detector, we obtain $\vert V_{ub} \vert = \left( 4.27 \pm 0.49\vert_{\rm data} \pm 0.55\vert_{\rm LCSRs} \right) \times 10^{-3}$ within the dominant region of the $\rho$ resonance. We clarify that the relatively small value of $\vert V_{ub} \vert$ extracted from $B \to \rho l \nu$, when compared to the golden channel $B \to \pi l\nu$, arises due to the finite width and nonresonant effects. We anticipate future measurements of purely isovector and isoscalar $B_{l4}$ decays, which will aid in reducing uncertainties by enhancing our understanding of the $\pi\pi$ phase shifts in the two-pion distribution amplitudes through heavy flavor decays.