Uncertainties of the $B\to D$ transition form factor from the $D$-Meson Leading-Twist Distribution Amplitude

TL;DR

This paper investigates the $D$-meson leading-twist distribution amplitude's uncertainties and their impact on the $B o D$ transition form factor, providing new sum rules, a refined model, and results consistent with experimental data.

Contribution

It introduces new sum rules for the $D$-meson DA moments and constructs a better model to evaluate the $B o D$ transition form factor with quantified uncertainties.

Findings

Calculated the first four moments of the $D$-meson DA.

Provided a refined model for the $D$-meson DA.

Estimated the impact of DA uncertainties on the $B o D$ form factor and branching ratio.

Abstract

The $B\to D$ transition form factor (TFF) $f^{B\to D}_+(q^2)$ is determined mainly by the $D$-meson leading-twist distribution amplitude (DA) , $\phi_{2;D}$, if the proper chiral current correlation function is adopted within the light-cone QCD sum rules. It is therefore significant to make a comprehensive study of DA $\phi_{2;D}$ and its impact on $f^{B\to D}_+(q^2)$. In this paper, we calculate the moments of $\phi_{2;D}$ with the QCD sum rules under the framework of the background field theory. New sum rules for the leading-twist DA moments $\left<\xi^n\right>_D$ up to fourth order and up to dimension-six condensates are presented. At the scale $\mu = 2 \rm GeV$, the values of the first four moments are: $\left<\xi^1\right>_D = -0.418^{+0.021}_{-0.022}$, $\left<\xi^2\right>_D = 0.289^{+0.023}_{-0.022}$, $\left<\xi^3\right>_D = -0.178 \pm 0.010$ and $\left<\xi^4\right>_D = 0.142^{+0.013}_{-0.012}$. Basing on the values of $\left<\xi^n\right>_D(n=1,2,3,4)$, a better model of $\phi_{2;D}$ is constructed. Applying this model for the TFF $f^{B\to D}_+(q^2)$ under the light cone sum rules, we obtain $f^{B\to D}_+(0) = 0.673^{+0.038}_{-0.041}$ and $f^{B\to D}_+(q^2_{\rm max}) = 1.124^{+0.053}_{-0.058}$. The uncertainty of $f^{B\to D}_+(q^2)$ from $\phi_{2;D}$ is estimated and we find its impact should be taken into account, especially in low and central energy region. The branching ratio $\mathcal{B}(B\to Dl\bar{\nu}_l)$ is calculated, which is consistent with experimental data.