Within the framework of the modified potential cluster model with the classification of orbital states according to Young diagrams, the astrophysical S-factor of the proton radiative capture on ¹¹C is calculated. The calculations take into account all resonances up to 3.5 MeV and are performed at energies up to 5 MeV. Based on the obtained total cross sections, the reaction rate in the temperature range of 0.01 to 10.0 $T_9$ is calculated and its simple parameterization is obtained. A comparative analysis of various model calculations of the ¹¹C($p,\gamma$)¹²N process is presented.

中文翻译：

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¹¹ C（p，γ）¹² N反应速率的聚类模型计算和比较概述

在根据杨氏图对轨道状态进行分类的改进的势簇模型的框架内，计算了¹¹ C上质子辐射俘获的天体S因子。该计算考虑了所有高达3.5 MeV的谐振，并且在高达5 MeV的能量下进行。基于获得的总横截面，反应速率在0.01到10.0的温度范围内${Ť}_9$计算并获得其简单的参数化。对¹¹ C（$p，\gamma$）提出了¹² N工艺。