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Covariant Spectator Theory of heavy–light and heavy mesons and the predictive power of covariant interaction kernels

机译:重轻介子和重介子的协变旁观者理论和协变相互作用核的预测能力

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摘要

The Covariant Spectator Theory (CST) is used to calculate the mass spectrum and vertex functions of heavy–light and heavy mesons in Minkowski space. The covariant kernel contains Lorentz scalar, pseudoscalar, and vector contributions. The numerical calculations are performed in momentum space, where special care is taken to treat the strong singularities present in the confining kernel. The observed meson spectrum is very well reproduced after fitting a small number of model parameters. Remarkably, a fit to a few pseudoscalar meson states only, which are insensitive to spin–orbit and tensor forces and do not allow to separate the spin–spin from the central interaction, leads to essentially the same model parameters as a more general fit. This demonstrates that the covariance of the chosen interaction kernel is responsible for the very accurate prediction of the spin-dependent quark–antiquark interactions.
机译:协方差理论(CST)用于计算Minkowski空间中重轻介子和重介子的质谱和顶点函数。协变核包含Lorentz标量,伪标量和向量贡献。数值计算是在动量空间中进行的,在动量空间中要特别注意处理约束核中存在的强奇点。拟合少量模型参数后,观察到的介子谱可以很好地重现。值得注意的是,仅对几个伪标量子介子状态的拟合对旋转轨道和张量力不敏感,并且不允许将旋转自旋与中心相互作用分开,从而导致与更一般的拟合基本相同的模型参数。这表明所选相互作用核的协方差可非常精确地预测自旋相关的夸克-反夸克相互作用。

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