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Wan-Bing Luo

Publications and source records attributed to Wan-Bing Luo.

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Vector mesons leading-twist longitudinal distribution amplitudes and related semi-leptonic decays within QCD sum rules

In this work, we focus on the light vector meson leading-twist longitudinal distribution amplitudes (DAs) $\phi^\parallel_{2;V}(x,\mu)$ with $V = \rho, K^\ast, \phi$. In order to obtain their accurate behaviors, a new scheme of QCD sum rule research with respect to DA suggested in 2021 by us is adopted. With an improved sum rule formula, the $\xi$-moments $\langle\xi^n\rangle_{2;V}^\parallel$ up to tenth order are calculated. In which, $\langle\xi^2\rangle^\parallel_{2;\rho}=0.225^{+0.013}_{-0.012}$, $\langle\xi^1\rangle^\parallel_{2;K^\ast}=-0.0228^{+0.0042}_{-0.0040}$, $\langle\xi^2\rangle^\parallel_{2;K^\ast}=0.217^{+0.007}_{-0.007}$, $\langle\xi^2\rangle^\parallel_{2;\phi}=0.209^{+0.020}_{-0.020}$, and the corresponding Gegenbauer moments $a^{2;\parallel}_{2;\rho}=0.074^{+0.039}_{-0.036}$, $a^{1;\parallel}_{2;K^\ast}=-0.038^{+0.007}_{-0.007}$, $a^{2;\parallel}_{2;K^\ast}=0.050^{+0.020}_{-0.019}$, $a^{2;\parallel}_{2;\phi}=0.027^{+0.058}_{-0.058}$ at the scale $\mu = 1~{\rm GeV}$, respectively. By fitting those $\langle\xi^n\rangle^\parallel_{2;V}(n = 1,2,\cdots,10)$ with the least squares method, the behaviors of leading-twist longitudinal DAs for $\rho, K^\ast, \phi$ are determined. Further, we recalculate the transition form factors and branching ratio of the $D\to(\rho,K^\ast)$, $D_s\to\phi$ semi-leptonic decay processes.

hep-ph

Status of the $D_s^+\to\phi\ell^+\nu_\ell$ decay with a chiral-odd $\phi$-meson light-cone distribution amplitude

The twist-2 distribution amplitude of the $\phi$-meson has attracted considerable interest due to its unique properties. In this work, we construct the transverse leading-twist light-cone distribution amplitude $\phi_{2;\phi}^\bot(x,\mu_0)$ of the $\phi$-meson using the light-cone harmonic oscillator model, in which a parameter $B_{2;\phi}^\bot$ dominantly control its longitudinal distribution. To explicitly isolate different twist contributions, we employ the right-handed chiral correlator for the QCD light-cone sum rules calculation of $D_s^+\to\phi$ decays, and further, we get the branching fraction, $\mathcal{B}(D_s^+ \to \phi e^+\nu_e )= (2.271_{-0.243}^{+0.291})\times 10^{-2}$ and $\mathcal{B}(D_s^+ \to \phi \mu^+\nu_\mu )=(2.250_{-0.240}^{+0.287})\times 10^{-2}$, where errors are squared average of the mentioned error sources. Furthermore, we have extracted the Cabbibo-Kobayashi-Maskawa (CKM) matrix element $|V_{cs}|=0.975_{-0.066}^{+0.067}$ with improved precision through the analysis. Finally, we calculated the polarization parameter and asymmetry parameter for the $D_s^+\to\phi$ decays.

hep-ph

Probing $D_s^*$-meson longitudinal twist-2 LCDA

In this paper, we carry on an investigation of the semileptonic decays $B_s\to D_s^*\ell \bar\nu_{\ell}$. Firstly, we derive the moments of the $D_s^*$-meson longitudinal leading-twist light-cone distribution amplitude (LCDA) based on QCD sum rules within background field theory framework. Considering the contributions of the vacuum condensates up to dimension-six, its first ten non-zero $\xi$-moments are given. Meanwhile, we construct the $D_s^*$-meson longitudinal leading-twist LCDA by using the light-cone harmonic oscillator model. Then, using those moments, we fix the model parameters $\alpha_{2;D_s^*}$ and $B_1^{2;D_s^*}$ by the least square method and apply them to calculate $B_s \to D_s^*$ transition form factors $A_1(q^2), A_2(q^2)$ and $V(q^2)$ that are derived by using the QCD light-cone sum rules. At the large recoil region, we obtain $A_1(0) =0.632_{-0.135}^{+0.228}, A_2(0) =0.706_{-0.092}^{+0.109}$ and $V(0) =0.647_{-0.069}^{+0.076}$. Those form factors are then extrapolated to the allowed whole physical $q^2$-region through the simplified series expansion. Finally, we obtain the branching fractions for the two decay channels $B_s\to D_s^*\ell\bar\nu_\ell$, $\it i.e.$ ${\cal B}(B_s^0 \to D_s^{*+}e^-\bar\nu_e)=(5.45_{-1.57}^{+2.15})\times 10^{-2}$, ${\cal B}(B_s^0 \to D_s^{*+}\mu^-\bar\nu_\mu)=(5.43_{-1.57}^{+2.14})\times 10^{-2}$.

hep-ph