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New Results for Radiative 2H3H Capture at Astrophysical Energies

  • S. B. DubovichenkoEmail author
  • D. M. Zazulin
Article

Within the framework of the modified potential cluster model with forbidden states which follow from the classification of orbital states of the clusters according to the Young tableaux, we have calculated the total cross section, astrophysical S-factor, and reaction rate of 2H3H radiative capture at low energies. We have shown that the implemented model and methods of classification of cluster states according to the Young tableaux allow one overall to correctly describe the available experimental data for the total cross section and astrophysical S-factor of this process.

Keywords

nuclear astrophysics light atomic nuclei low and astrophysical energies elastic scattering 2H3H system potential description radiative capture total cross sections thermonuclear reactions potential cluster model forbidden states classification of orbital states according to the Young tableaux 

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© Springer Science+Business Media, LLC, part of Springer Nature 2019

Authors and Affiliations

  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 UniversityMinistry of Education and Science of the Republic of KazakhstanAlmatyKazakhstan

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