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Photoproduction of the $B_c$ meson at the future $e^+e^-$ colliders

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arxiv 2211.09003 v1 pith:VKLS7JUG submitted 2022-11-16 hep-ph

classification hep-ph
keywords photoproductioncollidersfuturegammarightarrowmesonphotonresolved
verification ladder T0 review T1 audit T2 compute T3 formal
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abstract

In the present paper, we study the photoproduction of various $S$-wave $B_c$ states, i.e. $B_c(1{}^1S_0)$, $B_c^*(1{}^1S_0)$, $B_c(2{}^1S_0)$ and $B^*_c(2{}^3S_1)$, at future $e^+e^-$ colliders within the framework of non-relativistic QCD. Two sources of the initial photons can be realized in the production, i.e., the LBS photon and the WWA photon. In addition to the direct photoproduction via the sub-process, $\gamma + \gamma \rightarrow B_c + b + \bar{c}$, we also calculate the resolved photoproduction via the sub-processes, $\gamma + g \rightarrow B_c + b + \bar{c}$ and $q + \bar{q} \rightarrow B_c + b + \bar{c}$ with $q=u,d,s,g$, respectively. Numerical results indicate that the contributions from the single resolved photoproduction are significant and even dominant at certain collision configuration. At the future high-energy and high-luminosity $e^+e^-$ colliders, the $B_c$ meson generated via the photoproduction mechanism is promisingly observable and can be well studied.

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  1. Rare $W \to B_c + \gamma$ decay up to the NNLO and NLL accuracy in QCD

    hep-ph 2025-02 conditional novelty 6.0 of 10

    The rare decay W to Bc plus photon gets NNLO QCD corrections that reduce the width by 31 percent, giving a branching fraction of 1.522 times 10 to the minus 10 after NLL resummation.

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