标题： 硼-10对质子的辐射俘获反应速率 显示英文标题

标题： Reaction rate of the radiative capture proton by 10B

摘要： 10B(p,{\gamma })11C反应在核天体物理学和受控热核聚变领域具有重要意义。 该反应是通过10B(p,{\gamma })11C(\b{eta}+{\nu })11B链产生11B的反应之一。 10B(p,{\gamma })11C反应（发生在第一代恒星内部）的速率对于今天在星际介质和地壳中观测到的10B和11B的数量可能非常重要。 在热核反应堆中，含有硼的结构元件可以用作中子吸收剂等。 因此，在这项工作中，基于修改后的势簇模型，并根据杨氏图分类轨道态，同时考虑允许和禁止状态，我们研究了描述总截面的可能性，这些截面是在高达1 MeV的能量下由p10B辐射俘获至11C核基态所形成的。 研究表明，仅基于从p10B散射态的E1和M1跃迁，考虑到11C核基态的第一个共振，就足以解释实验天体物理S因子的大小和形状。 本文给出了我们发现的11C核基态辐射p10B捕获的天体物理S因子与文献中的实验数据的比较。 基于得到的理论S因子，在0.01到1 T9的温度范围内计算了此反应的速率。 对速率的计算结果用一个简单表达式进行了近似，这简化了它们在应用热核和天体物理研究中的使用。 显示英文摘要

摘要： The 10B(p,{\gamma})11C reaction is of significant interest in nuclear astrophysics and in the field of controlled thermonuclear fusion. This reaction is one of the reactions of 11B production, which is carried out through the 10B(p,{\gamma})11C(\b{eta}+{\nu})11B chain. The rate of the 10B(p,{\gamma})11C reaction (occurring in the interiors of first-generation stars) can be of great importance for the amount of 10B and 11B observed today in the interstellar medium and in the Earth's crust. In thermonuclear reactors, structural elements containing boron can be used as neutron absorbers, etc. Therefore, in this work, within the framework of a modified potential cluster model with a classification of orbital states according to Young's diagrams and taking into account allowed and forbidden states, we examined the possibility of describing the available experimental data for the total cross sections of the radiative p10B capture to the ground state of the 11C nucleus at energies up to 1 MeV. It is shown that only on the basis of E1 and M1 transitions from the p10B scattering states, taking into account the first resonance for the ground state of the 11C nucleus, it is quite possible to explain the magnitude and shape of the experimental astrophysical S-factor. The work presents comparisons the astrophysical S-factors of the radiative p10B capture to the ground state of the 11C nucleus found by us with the experimental data available in the literature. Based on the obtained theoretical S-factor, the rate of this reaction was calculated in the temperature range from 0.01 to 1 T9. The calculated results for rates are approximated by a simple expression, which simplifies their use in applied thermonuclear and astrophysical research.