$B\to V\ell^+\ell^-$ in the Standard Model from Light-Cone Sum Rules
arXiv:1503.05534 · doi:10.1007/JHEP08(2016)098
Abstract
We present $B_q\toÏ$, $B_q\toÏ$, $B_q\to K^*$, $B_s\to K^*$ and $B_s\to Ï$ form factors from light-cone sum rules (LCSR) at $\mathcal{O}(α_s)$ for twist-2 and 3 and $\mathcal{O}(α_s^0)$ for twist-4 with updated hadronic input parameters. Three asymptotic light-cone distribution amplitudes of twist-$4$ (and $5$) are determined, necessary for the form factors to obey the equations of motion. It is argued that the latter constrain the uncertainty of tensor-to-vector form factor ratios thereby improving the prediction of zeros of helicity amplitudes of major importance for $B\to K^*\ell\ell$ angular observables. We provide easy-to-use fits to the LCSR results, including the full error correlation matrix, in all modes at low $q^2$ as well as combined fits to LCSR and lattice results covering the entire kinematic range for $B_q\to K^*$, $B_s\to K^*$ and $B_s\to Ï$. The error correlation matrix avoids the problem of overestimating the uncertainty in phenomenological applications. Using the new form factors and recent computations of non-factorisable contributions we provide Standard Model predictions for $B\to K^*γ$ as well as $B\to K^*\ell^+\ell^-$ and $B_s\toÏμ^+μ^-$ at low dilepton invariant mass. Employing our $B \to (Ï,Ï) $ form factor results we extract the CKM element $|V_\mathrm{ub}|$ from the semileptonic decays $B\to(Ï,Ï) \ellν$ and find good agreement with other exclusive determinations.
64 pages, 7 figures, 15 tables. v3: Minor clarifications, numerics unchanged. Matches version published in JHEP