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arXiv 1912.06375hep-phhep-exhep-lat
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$N(1535) \rightarrow N$引力跃迁形状因子

Gravitational transition form factors of $N(1535) \rightarrow N$

U. Özdem, K. Azizi

摘要:

我们利用对称能量动量张量流的夸克部分,利用光锥QCD求和规则计算了$N(1535) \rightarrow N$的跃迁引力形状因子.在数值分析中,我们采用了$ N(1535) $重子分布振幅的两组不同的形状参数和核子内插流的一般形式。可以看出,动量平方依赖的引力形状因子可以很好地描述的p极拟合函数。用两组参数得到的结果有很大的不同,并且$N(1535) \rightarrow N$跃迁引力形状因子高度依赖于表征夸克相对轨道角动量的$N(1535)$态分布振幅的形状参数.

英文摘要:

We employ the quark part of the symmetric energy-momentum tensor current to calculate the transition gravitational form factors of the $N(1535) \rightarrow N$ by means of the light cone QCD sum rule formalism. In numerical analysis, we use two different sets of the shape parameters in the distribution amplitudes of the $ N(1535) $ baryon and the general form of the nucleon's interpolating current. It is seen that the momentum squared dependence of the gravitational form factors can be well described by the p-pole fit function. The results obtained by using two sets of parameters are found to be quite different from each other and the $N(1535) \rightarrow N$ transition gravitational form factors depend highly on the shape parameters of the distribution amplitudes of the $N(1535)$ state that parametrize relative orbital angular momentum of the constituent quarks.

机构、总结、中文摘要均由AI分析而来,可能存在错误,请以论文正文为准。

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