Персона: Игамов, Сайрамбай Бадамбаевич
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Сайрамбай Бадамбаевич
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- ПубликацияТолько метаданныеAsymptotic normalization coefficient for C-12 + p -> N-13 from the C-12(B-10, Be-9)N-13 reaction and the C-12(p, gamma) N-13 astrophysical S factor(2022) Artemov, S. V.; Yarmukhamedov, R.; Burtebayev, N.; Karakozov, B. K.; Igamov, S. B.; Игамов, Сайрамбай БадамбаевичThis work is aimed at clarifying the contribution of the proton direct radiative capture to the C-12(p, gamma) N-13 reaction by specifying the value of the asymptotic normal- ization coefficient (ANC) for C-12 + p -> N-13(g.s). In order to do this, the differential cross section of the proton transfer in the C-12(B-10, Be-9) N-13 reaction at an energy of 41.3 MeV has been measured and analyzed through the modified distorted wave Born approximation (MDWBA) method taking into account the reaction channel coupling and He-3 cluster transfer contributions. The value of the ANC was derived to be 1.63 +/- 0.13 fm(-1/2), which was used in estimating the astrophysical S(E) factor and the reaction rate of the proton radiative capture by the C-12 nucleus at energies of astrophysical relevance.