The total cross sections of the radiative proton capture on ⁸Li at astrophysical energies are considered in the framework of the modified potential cluster model with forbidden states with the classification of the orbital cluster states according to Young diagrams. The data obtained from the ⁹Be(γ, $p_0$)⁸Li photodisintegration process according to the detailed balancing principle are used for the experimental data of the ⁸Li(p, γ)⁹Be capture. It is possible to reproduce the available data on cross sections at the energies up to 7.0 MeV. Astrophysical S-factors and reaction rates $〈\sigma \nu 〉$ are calculated at the temperature range of 0.01 to 10 $T_9$. It is shown that the reaction rate is significantly affected by the resonances in the $p^8$Li scattering channel, and, especially by the first $1/2^{-}$ resonance at 87 keV. The analytical parametrization is performed for the calculated reaction rate $〈\sigma \nu 〉$.

在修正的势态簇模型的框架中考虑了天体能量在⁸ Li上的辐射质子捕获的总截面，并根据杨图对轨道簇状态进行了分类。从⁹ Be（γ，$p_0$）根据详细的平衡原理，对⁸ Li（p，γ）⁹ Be捕获的实验数据采用了⁸ Li光分解过程。可以在能量高达7.0 MeV的情况下在横截面上再现可用数据。天体S因子和反应速率$〈\sigma \nu 〉$ 在0.01至10的温度范围内计算 ${Ť}_9$。结果表明，反应速率显着受共振的影响。$p^8$锂的散射通道，尤其是通过第一 $\mathrm{1个}/2^{-}$在87 keV时产生共振。对计算出的反应速率进行分析参数化$〈\sigma \nu 〉$。