Potential cluster calculations for the astrophysical S-factor and reaction rate of the radiative ³He(⁴He,γ)⁷Be capture

In the frame of a modified potential cluster model based on the classification of orbital states according to Young diagrams and revised interaction potential parameters for the bound states of ⁷Be in the ³He⁴He cluster model with forbidden states, the astrophysical S-factor for the radiative capture reaction ³He(⁴He,γ)⁷Be has been calculated from 10 keV. The result obtained, S(23 keV) = 0.561 keV·b, reproduces the latest experimental data at 23 keV. The calculated and parametrized reaction rate is compared with some known results in the range of temperatures from 0.05 to 5 T₉.