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$W$ radiative decay to heavy-light mesons in HQET factorization through ${\cal O}(\alpha_s)$

High Energy Physics - Phenomenology 2019-10-02 v2 High Energy Physics - Experiment

Abstract

Analogous to NRQCD factorization for heavy quarkonium exclusive production, in this work we propose to employ the heavy-quark-effective-theory (HQET) factorization, which has been predominantly applied to account for exclusive BB decays, to study the exclusive production of the heavy-flavored mesons. We take WB(Ds)+γW\to B(D_s)+\gamma as a prototype process. The validity of the HQET factorization rests upon the presumed scale hierarchy: mWmbΛQCDm_W\sim m_b\gg \Lambda_{\rm QCD}. Through an explicit analysis at next-to-leading order in αs\alpha_s yet at leading order in 1/mb1/m_b, we verify that the decay form factors can indeed be expressed as the convolution between perturbatively calculable hard-scattering kernel and the BB meson light-cone distribution amplitude (LCDA) defined in HQET. It is observed that the factorization scale dependence becomes reduced after incorporating the NLO perturbative correction. An interesting future investigation is to identify and resum large collinear logarithms of mW/mbm_W/m_b that arise ubiquitously in the fixed-order expressions of the hard-scattering kernel in HQET factorization.

Keywords

Cite

@article{arxiv.1903.12627,
  title  = {$W$ radiative decay to heavy-light mesons in HQET factorization through ${\cal O}(\alpha_s)$},
  author = {Saadi Ishaq and Yu Jia and Xiaonu Xiong and De-Shan Yang},
  journal= {arXiv preprint arXiv:1903.12627},
  year   = {2019}
}

Comments

22 pages, 8 figures, 1 table. Text expanded and improved, two more figures and one table added, references added