RADIATIVE PROTON CAPTURE ON 3 H AT ASTROPHYSICAL ENERGIES AND ITS ROLE IN THE INITIAL STAGE OF STAR FORMATION

A. V. Dzhazairov-Kakhramanov, L.T. Karipbayeva

2019

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DOI 10.32014/2019.2518-1726.19
Data confidence 70 medium
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Abstract

Calculations of the astrophysical S-factor of the proton radiative capture on 3 H at energies from 1 keV to 10 MeV in the frame of the Modified Potential Cluster Model (MPCM) with classification of orbital states of nuclear particles according to Young tableaux and isospin were carried out.The explanation of the used phenomenological model MPCM was done.The classification of the p 3 H states according to Young tableaux was given.The p 3 H interaction potentials and phase shifts of the p 3 H elastic scattering were found.