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Astrophysical S-factor for р 12С→13Nγ radiative capture

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Russian Physics Journal Aims and scope

Within the framework of the potential cluster model with forbidden states the feasibility of description of experimental data on the astrophysical S-factors for р 12С radiative capture is studied at energies from 0.03 to 1.0 MeV.

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Authors and Affiliations

  1. V. G. Fesenkov Astrophysical Institute of Kazakhstan Scientific Center of Space Research and Technology, Almaty, Kazakhstan

    S. B. Dubovichenko & A. V. Dzhazairov-Kakhramanov

Authors
  1. S. B. Dubovichenko
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  2. A. V. Dzhazairov-Kakhramanov
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Corresponding author

Correspondence to S. B. Dubovichenko.

Additional information

Translated from Izvestiya Vysshikh Uchebnykh Zavedenii, Fizika, No. 8, pp. 58–64, August, 2009.

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Dubovichenko, S.B., Dzhazairov-Kakhramanov, A.V. Astrophysical S-factor for р 12С→13Nγ radiative capture. Russ Phys J 52, 833–840 (2009). https://doi.org/10.1007/s11182-010-9308-2

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  • DOI: https://doi.org/10.1007/s11182-010-9308-2

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