ASTROPHYSICAL S-FACTOR FOR p12C→13Nγ RADIATIVE CAPTURE
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作者:
Dubovichenko, S. B.
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Kazakhstan Sci Ctr Space Res & Technol, VG Fesenkov Astrophys Inst, Alma Ata, KazakhstanKazakhstan Sci Ctr Space Res & Technol, VG Fesenkov Astrophys Inst, Alma Ata, Kazakhstan
Dubovichenko, S. B.
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Dzhazairov-Kakhramanov, A. V.
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Kazakhstan Sci Ctr Space Res & Technol, VG Fesenkov Astrophys Inst, Alma Ata, KazakhstanKazakhstan Sci Ctr Space Res & Technol, VG Fesenkov Astrophys Inst, Alma Ata, Kazakhstan
Dzhazairov-Kakhramanov, A. V.
[1
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机构:
[1] Kazakhstan Sci Ctr Space Res & Technol, VG Fesenkov Astrophys Inst, Alma Ata, Kazakhstan
Within the framework of the potential cluster model with forbidden states the feasibility of description of experimental data on the astrophysical S-factors for p(12)C radiative capture is studied at energies from 0.03 to 1.0 MeV.