Asymptotic normalization coefficients for 11B + p → 12C from the 11B(10B, 9Be)12C reaction and the 11B(p, γ)12C astrophysical S-factor

The 11B(10B,9Be)12C reaction was studied at the energy of 41.3 MeV with transitions to the ground (0+) and low-lying excited 4.44 MeV (2+) and 9.64 MeV (3−) states of 12C nucleus. The analysis of the measured angular distributions was carried out using a modified distorted wave (MDWBA) method, assum...

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Bibliographic Details
Main Authors:	S.K. Sakhiyev, S.V. Artemov, N. Burtebayev, S.B. Sakuta, S.B. Igamov, Maulen Nassurlla, K. Rusek, M. Wolińska-Cichocka, N. Amangeldi, Marzhan Nassurlla, A. Trzcińska, G. Yergaliuly, F.Kh. Ergashev, O.R. Tojiboev, I.Ya. Son, A. Sabidolda, R. Khojayev, Y.B. Mukanov, D.A. Issayev
Format:	Article
Language:	English
Published:	Elsevier 2024-12-01
Series:	Results in Physics
Subjects:	Heavy ion beam peripheral proton transfer modified distorted wave Born approximation (MDWBA) asymptotic normalization coefficient (ANC) astrophysical S-factor
Online Access:	http://www.sciencedirect.com/science/article/pii/S2211379724007356
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Asymptotic normalization coefficients for 11B + p → 12C from the 11B(10B, 9Be)12C reaction and the 11B(p, γ)12C astrophysical S-factor

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