  The results are presented on the total cross sections, astrophysical
S-factor, reaction rate of the deuteron radiative capture on 3He at the
temperatures from 0.03 up to 3 T9 calculated in the framework of the potential
cluster model with the forbidden states coming from the classification of the
orbital states by the Young diagrams. Within the used model and exploited Young
diagram classification made it possible to reproduce the general features of
the available experimental data on the cross section and reconstructed
astrophysical S-factor in the energy range from 200 keV up to 1.4 MeV. The
parametrization of the obtained reaction rate has been found and been compared
with some other actual reactions with light clusters.
