New Analysis of p3H Capture at Low Energies

详细

Within the framework of the modified potential cluster model with classification of the orbital states of nuclear particles according to Young tableaux and isospin, calculations of the astrophysical S-factor of the radiative p³H capture reaction at energies from 1 keV to 10 MeV are performed and the possibility of describing the available experimental data in the energy range from 50 keV to 5 MeV is demonstrated.