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The astrophysical S-factor of proton radiative capture on triton
New Astronomy ( IF 1.9 ) Pub Date : 2021-02-02 , DOI: 10.1016/j.newast.2021.101572 H. Khalili , M. Mohammadzade
中文翻译:
Triton上质子辐射俘获的天体S因子
更新日期:2021-02-10
New Astronomy ( IF 1.9 ) Pub Date : 2021-02-02 , DOI: 10.1016/j.newast.2021.101572 H. Khalili , M. Mohammadzade
The proton capture on H is important to understand various physical and astrophysical processes. In this study, the cross section and astrophysical S-factor of the proton radiative capture on triton were taken into account at low energies. The H(p,He reaction was studied using the E1 transition. The gamma-ray transition is dominated by the E1 multipolarity and by incoming -waves. The non-resonant astrophysical S-factors for the E1 transition were calculated using the potential model. The results were satisfactorily in good agreement with the corresponding experimental data.
中文翻译:
Triton上质子辐射俘获的天体S因子
质子捕获 H对于理解各种物理和天体过程很重要。在这项研究中,在低能量条件下考虑了质子辐射俘获tri的截面和天体S因子。这生命值,使用E1跃迁研究了他的反应。伽马射线跃迁主要由E1多极性和入射-波浪。使用电位模型计算E1跃迁的非共振天体S因子。结果令人满意地与相应的实验数据吻合。