Revisiting $D$-meson twist-2, 3 distribution amplitudes

TL;DR

This paper refines the understanding of D-meson distribution amplitudes by developing new sum rules and improved models, aiming to reduce theoretical uncertainties in semileptonic B decay predictions.

Contribution

It introduces new sum rules for D-meson twist-2, 3 distribution amplitudes and improves their light-cone harmonic oscillator models for better accuracy.

Findings

Derived new sum rules for $\xi$-moments of D-meson DAs.

Constructed improved light-cone harmonic oscillator models.

Determined model parameters through least squares fitting.

Abstract

Due to the significant difference between the experimental measurements and the theoretical predictions of standard model (SM) for the value of $\mathcal{R}(D)$ of the semileptonic decay $B\to D\ell\bar{\nu}_{\ell}$, people speculate that it may be the evidence of new physics beyond the SM. Usually, the $D$-meson twist-2, 3 distribution amplitudes (DAs) $\phi_{2;D}(x,\mu)$, $\phi_{3;D}^p(x,\mu)$ and $\phi_{3;D}^\sigma(x,\mu)$ are the main error sources when using perturbative QCD factorization and light-cone QCD sum rules to study $B\to D\ell\bar{\nu}_{\ell}$. Therefore, it is important to get more reasonable and accurate behaviors for those DAs. Motivated by our previous work [Phys. Rev. D 104, no.1, 016021 (2021)] on pionic leading-twist DA, we revisit $D$-meson twist-2, 3 DAs $\phi_{2;D}(x,\mu)$, $\phi_{3;D}^p(x,\mu)$ and $\phi_{3;D}^\sigma(x,\mu)$. New sum rules formulae for the $\xi$-moments of these three DAs are suggested to obtain more accurate values. The light-cone harmonic oscillator models for those DAs are improved, and whose model parameters are determined by fitting the values of $\xi$-moments with the least squares method.