Abstract

We carry out a comprehensive analysis of the full set of {bar{B}}_q rightarrow D_q^{(*)} form factors for spectator quarks q=u,d,s within the framework of the Heavy-Quark expansion (HQE) to order {mathcal {O}}left( alpha _s, 1/m_b, 1/m_c^2right) . In addition to the available lattice QCD calculations we make use of two new sets of theoretical constraints: we produce for the first time numerical predictions for the full set of {bar{B}}_s rightarrow D_s^{(*)} form factors using Light-Cone sum rules with B_s-meson distribution amplitudes. Furthermore, we reassess the QCD three-point sum rule results for the Isgur-Wise functions entering all our form factors for both q=u,d and q=s spectator quarks. These additional constraints allow us to go beyond the commonly used assumption of SU(3)_F symmetry for the {{bar{B}}}_srightarrow D_s^{(*)} form factors, especially in the unitarity constraints which we impose throughout our analysis. We find the coefficients of the IW functions emerging at {mathcal {O}}left( 1/m_c^2right) to be consistent with the naive {mathcal {O}}left( 1right) expectation, indicating a good convergence of the HQE. While we do not find significant SU(3) breaking, the explicit treatment of q=s as compared to a simple symmetry assumption renders the unitarity constraints more effective. We find that the (pseudo)scalar bounds are saturated to a large degree, which affects our theory predictions. We analyze the phenomenological consequences of our improved form factors by extracting |V_{cb}| from {bar{B}}rightarrow D^{(*)}ell nu decays and producing theoretical predictions for the lepton-flavour universality ratios R(D), R(D^*), R(D_s) and R(D_s^*), as well as the tau - and D_q^* polarization fractions for the {bar{B}}_qrightarrow D_q^{(*)}tau nu modes.

Highlights

  • Semileptonic b → c transitions are of great phenomenological interest, both within the Standard Model (SM) and beyond

  • C: As scenario B, but we consider the impact of finite SU (3)F symmetry breaking in the form factors by amending our previous power counting: we count the expansion parameter εF for the symmetry breaking as εF ∼ ε ∼ εc

  • A first step to test the assumption of exact SU (3)F symmetry is taken by evaluating our nominal likelihood at the best-fit point obtained in Ref

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Summary

Introduction

Semileptonic b → c transitions are of great phenomenological interest, both within the Standard Model (SM) and beyond. These tensions motivate potential new physics (NP) contributions to b → c ν transitions with light leptons, which in turn require a determination of the corresponding form factors independent of the experimental input This situation, together with the recent appearance of several experimental analysis allowing for a model-independent interpretation of their results on B → D(∗) ν decays [5,6,7] sparked renewed interest in the relevant hadronic matrix elements [8,9,10,11,12,13,14,15,16,17,18]. In appendix B we provide the numerical inputs and results of our LCSR analysis

Notation and setup
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