$B\to D_0^*$ and $B_s\to D_{s0}^*$ form factors from QCD light-cone sum rules

TL;DR

This paper calculates form factors for B to D0* and Bs to Ds0* transitions using QCD light-cone sum rules, considering different resonance scenarios, and compares predictions with experimental data and HQET predictions.

Contribution

First application of QCD light-cone sum rules with B-meson distribution amplitudes to these form factors, including multiple resonance scenarios and detailed theoretical considerations.

Findings

Predicted semileptonic decay branching ratios.

Calculated decay constants for D0* and Ds0* mesons.

Predicted lepton flavor universality ratios R(D0*) and R(Ds0*).

Abstract

We present the first application of QCD light-cone sum rules (LCSRs) with $B_{(s)}$-meson distribution amplitudes to the $B_{(s)}\!\to\! D_{(s)0}^*$ form factors, where $D_{(s)0}^*$ is a charmed scalar meson. We consider two scenarios for the $D_0^*$ spectrum. In the first one, we follow the Particle Data Group and consider a single broad resonance $D_0^*(2300)$. In the second one, we assume the existence of two scalar resonances, $D_0^*(2105)$ and $D_0^*(2451)$, as follows from a recent theoretically motivated analysis of $B\to D\pi\pi$ decays. The $B\!\to\! D_0^*$ form factors are calculated in both scenarios, also taking into account the large total width of $D_0^*(2300)$. Furthermore, we calculate the $B_s\!\to\! D_{s0}^*$ form factors, considering in this case only the one-resonance scenario with $D_{s0}(2317)$. In this LCSRs calculation, the $c$-quark mass is kept finite and the $s$-quark mass is taken into account. We also include contributions of the two- and three-particle distribution amplitudes up to twist-four. Our predictions for semileptonic $B\!\to\! D_0^*\ell\nu_\ell$ and $B_s\!\to\! D_{s0}^*\ell\nu_\ell$ branching ratios are compared with the available data and HQET-based predictions. As a byproduct, we also obtain the $D_0^*$- and $D_{s0}^*$-meson decay constants and predict the lepton flavour universality ratios $R(D_0^*)$ and $R(D_{s0}^*)$.