Indirect methods of determination of the asymptotic normalization coefficients and their application for nuclear astrophysics

Abstract

The basic methods of the determination of asymptotic normalization coefficient for A + a → B of astrophysical interest are briefly presented. The results of the application of the specific asymptotic normalization coefficients derived within these methods for the extrapolation of the astrophysical S factors to experimentally inaccessible energy regions (E ≤ 25 keV) for the some specific radiative capture A(a, γ)B reactions of the pp-chain and the CNO cycle are presented.