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New Analysis of p 3H Capture at Low Energies

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...

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Bibliographic Details
Published in:Russian physics journal 2017-05, Vol.60 (1), p.63-72
Main Author: Dubovichenko, S. B.
Format: Article
Language:English
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Summary: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.
ISSN:1064-8887
1573-9228
DOI:10.1007/s11182-017-1043-5