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NSR database version of May 8, 2024.

Search: Author = B.Beisenov

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2021DU02      Nucl.Phys. A1007, 122135 (2021)

S.B.Dubovichenko, N.A.Burkova, A.V.Dzhazairov-Kakhramanov, B.Beisenov

Cluster model calculations of the ¹¹C(p, γ)¹²N reaction rate and comparative overview

NUCLEAR REACTIONS ¹¹C(p, γ), E=1-1000 MeV; calculated S-factor, astrophysical reaction rates within the framework of the modified potential cluster model with the classification of orbital states according to Young diagrams. Comparison with available data.

doi: 10.1016/j.nuclphysa.2020.122135
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2020DU14      Phys.Rev. C 102, 045805 (2020)

S.B.Dubovichenko, R.Ya.Kezerashvili, N.A.Burkova, A.V.Dzhazairov-Kakhramanov, B.Beisenov

Reanalysis of the ¹³N(p, γ)¹⁴O reaction and its role in the stellar CNO cycle

NUCLEAR REACTIONS ¹³N(p, γ)¹⁴O, E(cm)=0.030-7 MeV; analyzed astrophysical S factor of the proton radiative capture through the experimentally known levels and resonances up to 9.76 MeV; calculated reaction rates at temperatures of 0.01 to 10 GK; deduced parameters of the analytical parametrization, and compared with NACRE II values. Modified potential cluster model (MPCM) of light atomic nuclei. Relevance to conversion of the carbon-nitrogen-oxygen (CNO) cycle to the hot CNO cycle.

doi: 10.1103/PhysRevC.102.045805
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