Asymptotic Normalization Constants in Nuclear Astrophysics View Full Text


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Article Info

DATE

2001-05

AUTHORS

V. Kroha, P. Bém, V. Burjan, J. Novák, Š. Piskoř, E. Šimečková, J. Vincour, A. Azhari, C.A. Gagliardi, A.M. Mukhamedzhanov, X. Tang, L. Trache, R.E. Tribble, F. Carstoiu

ABSTRACT

The indirect method of determining astrophysical nuclear reaction rates is discussed. The overall normalization of the astrophysical S-factor for such reactions may be determined from one quantity, the asymptotic normalization coefficient of the overlap function of the bound state wave functions for the initial and final channels. These coefficients can be found also from peripheral transfer reactions whose amplitudes are determined by the same overlap function as the amplitudes of the corresponding astrophysical radiative capture processes. The experimental test of this approach and the last results of S17 measurements are presented. More... »

PAGES

471-489

Identifiers

URI

http://scigraph.springernature.com/pub.10.1023/a:1017504100371

DOI

http://dx.doi.org/10.1023/a:1017504100371

DIMENSIONS

https://app.dimensions.ai/details/publication/pub.1046967249


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