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

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 3 He 4 He, 3 H 4 He, and 2 H 4 He cluster channels of the nuclei 7 Be, 7 Li, and 6 Li, astrophysical S-factors of processes of radiative 3 He 4 He capture from 20 keV, 3 H 4 Hе capture from 10 keV, and 2 Н 4 Не 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 T 9 and a comparison with the results of other authors is carried out.