@article{A.V. Dzhazairov-Kakhramanov_L.T. Karipbayeva_2019, title={RADIATIVE PROTON CAPTURE ON 3H AT ASTROPHYSICAL ENERGIES AND ITS ROLE IN THE INITIAL STAGE OF STAR FORMATION}, url={https://journals.nauka-nanrk.kz/physics-mathematics/article/view/1575}, abstractNote={<p>Calculations of the astrophysical S-factor of the proton radiative capture on 3H at energies from 1<br>keV to 10 MeV in the frame of the Modified Potential Cluster Model (MPCM) with classification of orbital states of<br>nuclear particles according to Young tableaux and isospin were carried out. The explanation of the used<br>phenomenological model MPCM was done. The classification of the p3H states according to Young tableaux was<br>given. The p3H interaction potentials and phase shifts of the p3H elastic scattering were found.</p>}, number={3}, journal={Известия НАН РК. Серия физико-математическая}, author={A.V. Dzhazairov-Kakhramanov and L.T. Karipbayeva}, year={2019}, month={июн.}, pages={13–21} }