Searching for $|V_{cd}|$ through the exclusive decay $D_s^+ \to K^0e^+\nu_e$ within QCD Sum Rules

TL;DR

This paper calculates the form factors and branching ratios for the semileptonic decay $D_s^+ o K^0 e^+ u_e$ using QCD sum rules, providing a new determination of $|V_{cd}|$ consistent with experimental data.

Contribution

It introduces a detailed QCD sum rules calculation of the transition form factor for $D_s^+ o K^0$, including NLO contributions and an extrapolation over the full $q^2$ range, to extract $|V_{cd}|$.

Findings

Calculated $f_+^{D_s^+ K^0}(0)=0.692_{-0.026}^{+0.027}$.

Predicted branching fractions $ imes 10^{-3}$: $3.379_{-0.275}^{+0.301}$ for $e$ channel, $3.351_{-0.273}^{+0.299}$ for $ u_ u$ channel.

Estimated $|V_{cd}|=0.221_{-0.010}^{+0.008}$.

Abstract

In this paper, we carry out an investigation into the semileptonic decays $D_s^+ \to K^0\ell^+\nu_\ell$ with $\ell=(e,\mu)$ by employing the QCD light-cone sum rules approach. The vector transition form factor (TFF) $f_+^{D_s^+ K^0}(q^2)$ for $D_s^+\to K^0$ decay is calculated while considering its next-to-leading order contribution. Subsequently, we briefly introduce the twist-2, 3 kaon distribution amplitudes, which are calculated by using QCD sum rules within the framework of the background field theory. At the large recoil point, the TFF has $f_+^{D_s^+ K^0}(0)=0.692_{-0.026}^{+0.027}$. Then, we extrapolate $f_+^{D_s^+ K^0}(q^2)$ to the whole physical $q^2$-region via the simplified $z(q^2,t)$-series expansion, and the behavior of TFF $f_+^{D_s^+ K^0}(q^2)$ is exhibited in the numerical results part, including the theoretical and experimental predictions for comparison. In addition, we compute the differential branching fraction $\mathcal{B}(D_s^+ \to K^0\ell^+\nu_\ell)$ with the electron and muon channels, which are expected to be $\mathcal{B}(D_s^+ \to K^0e^+\nu_e)=3.379_{-0.275}^{+0.301}\times 10^{-3}$ and $\mathcal{B}(D_s^+ \to K^0\mu^+\nu_\mu)=3.351_{-0.273}^{+0.299}\times 10^{-3}$ as well as contained other results for comparison. Our results show good agreement with the BESIII measurements and theoretical predictions. Furthermore, we present our prediction with respect to the CKM matrix element $|V_{cd}|$ by using the $\mathcal{B}(D_s^+ \to K^0e^+\nu_e)$ result from BESIII Collaboration, yielding $|V_{cd}|=0.221_{-0.010}^{+0.008}$. Finally, we provide the ratio between $D_s^+ \to K^0e^+\nu_e$ and $D_s^+ \to \eta e^+\nu_e$ channels, i.e. $\mathcal{R}_{K^0/\eta}^e=0.144_{-0.020}^{+0.028}$.