Asymptotic normalization constants in nuclear astrophysics Academic Article

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.

authors

• Gagliardi, Carl

published proceedings

• CZECHOSLOVAK JOURNAL OF PHYSICS

author list (cited authors)

• Kroha, V., Bem, P., Burjan, V., Novak, J., Piskor, S., Simeckova, E., ... Carstoiu, F.

citation count

• 2

complete list of authors

• Kroha, V||Bem, P||Burjan, V||Novak, J||Piskor, S||Simeckova, E||Vincour, J||Azhari, A||Gagliardi, CA||Mukhamedzhanov, AM||Tang, X||Trache, L||Tribble, RE||Carstoiu, F

publication date

• May 2001

publisher

• Springer Nature  Publisher

keywords

• Direct Nuclear Reactions
• Dwba Analysis
• Nuclear Astrophysics

Digital Object Identifier (DOI)

• 10.1023/A:1017504100371

start page

• 471

end page

• 489

volume

• 51

issue

• 5

URL

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