https://doi.org/10.1140/epja/s10050-021-00652-z
Regular Article - Experimental Physics
Asymptotic normalization coefficient for 
from the 
reaction and the 
astrophysical S factor
1
Institute of Nuclear Physics, 100214, Tashkent, Uzbekistan
2
Institute of Nuclear Physics, 050032, Almaty, Kazakhstan
3
Al-Farabi Kazakh National University, 050040, Almaty, Kazakhstan
4
Branch of National Research Nuclear University MEPhI, 100214, Tashkent, Uzbekistan
5
L.N. Gumilyov Eurasian National University, 010008, Nur-Sultan, Kazakhstan
6
Heavy Ion Laboratory University of Warsaw, PL-20-093, Warsaw, Poland
7
National Research Center “Kurchatov Institute”, 123182, Moscow, Russia
8
Gulistan State University, 120100, Gulistan, Uzbekistan
9
Satbayev University, Institute of Physics and Technology, 050032, Almaty, Kazakhstan
Received:
26
May
2021
Accepted:
5
December
2021
Published online:
9
February
2022
This work is aimed at clarifying the contribution of the proton direct radiative capture to the reaction by specifying the value of the asymptotic normalization coefficient (ANC) for 
. In order to do this, the differential cross section of the proton transfer in the 
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 
cluster transfer contributions. The value of the ANC was derived to be 1.63±0.13 fm
, which was used in estimating the astrophysical S(E) factor and the reaction rate of the proton radiative capture by the 
nucleus at energies of astrophysical relevance.
© The Author(s), under exclusive licence to Società Italiana di Fisica and Springer-Verlag GmbH Germany, part of Springer Nature 2022
