Investigating the ratio of CKM matrix elements $|V_{ub}|/|V_{cb}|$ from semileptonic decay $B_s^0\to K^-\mu^+\nu_\mu$ and kaon twist-2 distribution amplitude

TL;DR

This study calculates the ratio of CKM matrix elements $|V_{ub}|/|V_{cb}|$ from the semileptonic decay $B_s^0 o K^-\mu^+ u_$ using QCD sum rules and a new kaon distribution amplitude model, providing a precise determination of the ratio.

Contribution

The paper introduces a new model for the kaon leading-twist distribution amplitude and applies it to improve the precision of the $B_s o K$ transition form factor calculation within QCD light-cone sum rules.

Findings

Calculated $|V_{ub}|/|V_{cb}| = 0.072 1.005

Obtained $f^{B_s o K}_+(0) = 0.270^{+0.022}_{-0.030}$

Derived a decay width of $5.626^{+1.271}_{-0.864} imes 10^{-12}$ GeV.

Abstract

In this paper, we calculate the ratio of Cabibbo-Kobayashi-Maskawa matrix elements, $|V_{ub}|/|V_{cb}|$, based on the semileptonic decay $B_s^0\to K^-\mu^+\nu_\mu$. Its key component, the $B_s\to K$ transition form factor $f^{B_s\to K}_+(q^2)$, is studied within the QCD light-cone sum rules approach by using a chiral correlator. The derived $f^{B_s\to K}_+(q^2)$ is dominated by the leading-twist part, and to improve its precision, we construct a new model for the kaon leading-twist distribution amplitude $\phi_{2;K}(x,\mu)$, whose parameters are fixed by using the least squares method with the help of the moments calculated by using the QCD sum rules within the background field theory. The first four moments at the initial scale $\mu_0 = 1~{\rm GeV}$ are, $\langle \xi^1\rangle _{2;K} = -0.0438^{+0.0053}_{-0.0075}$, $\langle \xi^2\rangle _{2;K} = 0.262 \pm 0.010$, $\langle \xi^3\rangle _{2;K} = -0.0210^{+0.0024}_{-0.0035}$ and $\langle \xi^4\rangle _{2;K} = 0.132 \pm 0.006$, respectively. And their corresponding Gegenbauer moments are, $a^{2;K}_1 = -0.0731^{+0.0089}_{-0.0124}$, $a^{2;K}_2 = 0.182^{+0.029}_{-0.030}$, $a^{2;K}_3 = -0.0114^{+0.0008}_{-0.0016}$ and $a^{2;K}_4 = 0.041^{-0.003}_{+0.005}$, respectively. At the large recoil region, we obtain $f^{B_s\to K} _+ (0) = 0.270^{+0.022}_{-0.030}$. By extrapolating $f^{B_s\to K}_+(q^2)$ to all the physical allowable region, we obtain a $|V_{ub}|$-independent decay width for the semileptonic decay $B_s^0\to K^-\mu^+\nu_\mu$, $5.626^{+1.271}_{-0.864} \times 10^{-12}\ {\rm GeV}$, which then leads to $|V_{ub}|/|V_{cb}| = 0.072\pm0.005$.