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Astrophysical S-Factor of Radiative р 14C Capture at Low Energies

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Russian Physics Journal Aims and scope

The possibility of describing the available experimental data on the astrophysical S-factor for the reaction of p14C capture to the ground state of 15N at astrophysical energies within the framework of the modified potential cluster model is considered.

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Authors and Affiliations

  1. V. G. Fessenkov Astrophysical Institute of the National Center for Space Research and Technology of the National Space Agency of the Aviation and Space Complex of the Ministry of Research and Development of the Republic of Kazakhstan, Almaty, Kazakhstan

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

  2. Institute of Nuclear Physics of the Atomic Energy Commission of the Ministry of Industry and New Technologies of the Republic of Kazakhstan, Almaty, Kazakhstan

    S. B. Dubovichenko, N. Burtebaev & A. V. Dzhazairov-Kakhramanov

  3. Al-Farabi Kazakh National University, Almaty, Kazakhstan

    D. K. Alimov

Authors
  1. S. B. Dubovichenko
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  2. N. Burtebaev
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  3. A. V. Dzhazairov-Kakhramanov
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  4. D. K. Alimov
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Translated from Izvestiya Vysshikh Uchebnykh Zavedenii, Fizika, No. 12, pp. 147–154, December, 2015.

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Dubovichenko, S.B., Burtebaev, N., Dzhazairov-Kakhramanov, A.V. et al. Astrophysical S-Factor of Radiative р 14C Capture at Low Energies. Russ Phys J 58, 1834–1842 (2016). https://doi.org/10.1007/s11182-016-0724-9

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  • DOI: https://doi.org/10.1007/s11182-016-0724-9

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