New Results for Astrophysical S-Factors of Radiative 3Не4Не, 3Н4Не, and 2Н4Не Capture

详细

Within the framework of the modified potential cluster model with classification of orbital states according to the Young tableaux and revised potential parameters for the ³He⁴He, ³H⁴He, and ²H⁴He cluster channels of the nuclei ⁷Be, ⁷Li, and ⁶Li, astrophysical S-factors of processes of radiative ³He⁴He capture from 20 keV, ³H⁴Hе capture from 10 keV, and ²Н⁴Не capture from 5 keV are considered. On the basis of the obtained results, the rates of all of the considered reactions are calculated in the temperature range from 0.05 to 5 T₉ and a comparison with the results of other authors is carried out.