Asymptotic normalization coefficients in nuclear astrophysics and structure View Full Text


Ontology type: schema:Chapter     


Chapter Info

DATE

2003

AUTHORS

C. A. Gagliardi , A. Azhari , V. Burjan , F. Carstoiu , V. Kroha , A. M. Mukhamedzhanov , A. Sattarov , X. Tang , L. Trache , R. E. Tribble

ABSTRACT

The asymptotic normalization coefficient (ANC) for a nuclear system specifies the normalization of the tail of the nuclear overlap function. ANCs may be determined experimentally by measuring peripheral nuclear reactions. They may be used to calculate the astrophysical S-factors for radiative capture reactions at stellar energies and to determine the halo structure of loosely bound nuclei. A brief introduction to ANCs is given and applications to the 7Be(p,γ)8B and 11C(p,γ)12N reactions and the halo structure of 8B are described. More... »

PAGES

109-113

Identifiers

URI

http://scigraph.springernature.com/pub.10.1007/978-3-642-55560-2_34

DOI

http://dx.doi.org/10.1007/978-3-642-55560-2_34

DIMENSIONS

https://app.dimensions.ai/details/publication/pub.1020098314


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