共变约束夸克模型中的辐射衰变 \bm{$D^*_{(s)}\to D_{(s)}\gamma$}

C. Tran, Mikhail A. Ivanov, Pietro Santorelli, Quang-Chau Vo
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摘要

根据textit{BABAR}和BESIII合作的新实验数据,我们重新审视了辐射衰变$D^*_{(s)}\to D_{(s)}\gamma$。我们在自己建立的协变约束夸克模型框架内计算了编码非微扰 QCD 效应的辐射耦合 $g_{D^*D\gamma}$。我们将我们的结果与其他理论研究和实验数据进行了比较。耦合(单位:$\textrm{GeV}^{-1}$)$|g_{D^{*+}D^+\gamma}| = 0.45(9)$和$|g_{D^{*0}D^0\gamma}| = 1.72(34)$与实验数据|g_{D^{*+}D^+\gamma}|=0.47(7)$和|g_{D^{*0}D^0\gamma}|=1.77(16)$一致。最有趣的情况是衰变$D^*_s\to D_s\gamma$,对于这个衰变,最近基于次先导阶光锥和规则的预测结果$|g_{D^*_s D_s\gamma}|=0.60(19)$ 与第一个(也是迄今为止唯一的)晶格QCD结果$|g_{D^*_s D_s\gamma}|=0.11(2)$ 存在近$3\sigma$的偏差。我们的计算结果为 $|g_{D^*_s D_s\gamma}|=0.29(6)$,介于上述两个结果之间,但比其他使用夸克模型或 QCD 和规则的研究预测的结果要大。本文内容可根据知识共享署名 3.0 许可条款使用。对本作品的任何进一步传播都必须注明作者、作品名称、期刊引文和 DOI。文章由 SCOAP3 资助,由中国物理学会、中国科学院高能物理研究所、中国科学院近代物理研究所和 IOP Publishing Ltd. 授权出版。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Radiative decays \bm{$D^*_{(s)}\to D_{(s)}\gamma$} in covariant confined quark model
Radiative decays $D^*_{(s)}\to D_{(s)}\gamma$ are revisited in light of new experimental data from \textit{BABAR} and BESIII collaborations. The radiative couplings $g_{D^*D\gamma}$ encoding nonperturbative QCD effects are calculated in the framework of the covariant confined quark model developed by us. We compare our results with other theoretical studies and experimental data. The couplings (in $\textrm{GeV}^{-1}$) $|g_{D^{*+}D^+\gamma}| = 0.45(9)$ and $|g_{D^{*0}D^0\gamma}| = 1.72(34)$ calculated in our model agree with the experimental data $|g_{D^{*+}D^+\gamma}|=0.47(7)$ and $|g_{D^{*0}D^0\gamma}|=1.77(16)$. The most interesting case is the decay $D^*_s\to D_s\gamma$, for which the recent prediction based on light-cone sum rules at next-to-leading order $|g_{D^*_s D_s\gamma}|=0.60(19)$ deviates from the first (and so far the only) lattice QCD result $|g_{D^*_s D_s\gamma}|=0.11(2)$ at nearly $3\sigma$. Our calculation yields $|g_{D^*_s D_s\gamma}|=0.29(6)$, which falls somehow between the two mentioned results, but is larger than those predicted in other studies using quark models or QCD sum rules. Content from this work may be used under the terms of the Creative Commons Attribution 3.0 licence. Any further distribution of this work must maintain attribution to the author(s) and the title of the work, journal citation and DOI. Article funded by SCOAP3 and published under licence by Chinese Physical Society and the Institute of High Energy Physics of the Chinese Academy of Science and the Institute of Modern Physics of the Chinese Academy of Sciences and IOP Publishing Ltd.
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