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Russian Physics Journal

, Volume 61, Issue 9, pp 1613–1619 | Cite as

Radiative p14N Capture to the Third Excited State of the 15O Nucleus at 6.17 MeV

  • S. B. DubovichenkoEmail author
  • N. A. Burkova
  • A. V. Dzhazairov-Kakhramanov
  • Ch. T. Omarov
Article
  • 5 Downloads

Within the framework of the modified potential cluster model, results of a description of available experimental data in terms of the astrophysical S-factor for the reaction of p14N capture to the third excited state of the 15O nucleus at 6.17 MeV with J = 3/2– for proton energies up to 1 MeV are presented. Under the assumption that this excited state is a P3/2 level and the two resonances at 260 and 987 keV are D scattering waves, we have on the whole successfully reproduced the experimental data for the astrophysical S-factor.

Keywords

nuclear astrophysics light atomic nuclei low and astrophysical energies elastic scattering p14N system potential description radiative capture total cross sections thermonuclear reactions potential cluster model forbidden states classification of orbital states according to Young tableaux 

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Copyright information

© Springer Science+Business Media, LLC, part of Springer Nature 2018

Authors and Affiliations

  • S. B. Dubovichenko
    • 1
    • 2
    Email author
  • N. A. Burkova
    • 2
  • A. V. Dzhazairov-Kakhramanov
    • 1
  • Ch. T. Omarov
    • 1
  1. 1.Fesenkov Astrophysical Institute of the National Center for Space Research and Technology of the Aerospace Agency of the Ministry of Defense and the Aerospace Industry of the Republic of KazakhstanAlmatyKazakhstan
  2. 2.Al Farabi Kazakh National University, Ministry of Education and Science of the Republic of KazakhstanAlmatyKazakhstan

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