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  • Open Access

Precision calculations of B→K* form factors from SCET sum rules beyond leading-power contributions

Jing Gao1, Ulf-G. Meißner1,2,3, Yue-Long Shen4, and Dong-Hao Li5,*

  • 1Helmholtz-Institut für Strahlen- und Kernphysik and Bethe Center for Theoretical Physics, Universität Bonn, D-53115 Bonn, Germany
  • 2Institute for Advanced Simulation, Forschungszentrum Jülich, D-52425 Jülich, Germany
  • 3Peng Huanwu Collaborative Center for Research and Education, International Institute for Interdisciplinary and Frontiers, Beihang University, Beijing 100191, China
  • 4College of Physics and Photoelectric Engineering, Ocean University of China, Qingdao 266100, China
  • 5MOE Frontiers Science Center for Rare Isotopes, and School of Nuclear Science and Technology, Lanzhou University, Lanzhou 730000, China

  • *Contact author: lidh@lzu.edu.cn

Phys. Rev. D 112, 014032 – Published 21 July, 2025

DOI: https://doi.org/10.1103/yvjd-2ymn

Abstract

We construct light cone sum rules (LCSR) for the B→K* form factors in the large recoil region using vacuum-to-B-meson correlation functions, and systematically calculate subleading-power corrections to these form factors at tree level, including next-to-leading power contributions from the hard-collinear propagator, the subleading effective current q¯Γ[iD⊥/(2mb)]hv, and twist-five/six four-particle higher-twist effects. By incorporating the available leading-power results at O(αs) and the corrections to higher-twist B-meson light cone distribution amplitudes from our previous work, we improve the precision of theoretical predictions for B→K* form factors and find that the subleading-power contributions amount to 30% of the corresponding leading-power results. Employing the Bourrely-Caprini-Lellouch parametrization, we determine the numerical results for B→K* form factors across the full kinematic range through a combined fit of LCSR predictions in the large recoil region and lattice QCD results in the small recoil region. Using the newly obtained B→K* form factors, we compute the branching fractions for the rare decays B→K*νℓν¯ℓ in the Standard Model, obtaining BR(B¯0→K¯*0νℓν¯ℓ)=8.09(96)×10−6 and BR(B¯+→K¯*+νℓν¯ℓ)=9.95(1.05)×10−6. Additionally, we predict that the longitudinal K* polarization fraction is FL=0.44(4).

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