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Next-to-Next-to-Leading-Order Corrections to the $B \to π$ Form Factors from Light-Cone Sum Rules

Published 21 Dec 2025 in hep-ph | (2512.18866v1)

Abstract: By incorporating the available leading-power results at $\mathcal{O}(αs)$ and next-to-leading-power corrections at tree level, we improve the precision of the theoretical predictions for $B\toπ$ form factors to the $\mathcal{O}(α_s2β_0)$ level in the large-recoil region using the light-cone sum rule approach with $B$-meson light-cone distribution amplitudes. We find that the QCD corrections at $\mathcal{O}(α_s2β_0)$ contribute approximately $+6.1\%$ compared to the tree-level result. Combining the light-cone sum rule predictions in the large-recoil region, lattice QCD results in the small-recoil region, we perform a combined fit for the $B\toπ$ form factors across the full kinematic range. Utilizing these form factors, we calculate the branching ratios, lepton-flavor-universality ratio $Rπ$, forward-backward asymmetry $\mathcal{A}{\rm FB}$, flat term $\mathcal{F}{\rm H}$ and polarization asymmetry $\mathcal{A}{\rm λ\ell}$ of $B\toπμ\barνμ$ and $B\toπτ\barντ$ decays. Using the experimentally measured $q2$-binned differential branching ratios of $B\toπμ\barνμ$ decay as input, employing the Bourrely-Caprini-Lellouch parametrization, we extract the Cabibbo-Kobayashi-Maskawa matrix element $|V{ub}| = 3.73(14) \times 10{-3}$.

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