Astrophysical S-Factors from Asymptotic Normalization Coefficients View Full Text


Ontology type: schema:Chapter     


Chapter Info

DATE

2001

AUTHORS

R. E. Tribble , A. Azhari , P. Bem , V. Burjan , F. Carstoiu , J. Cejpek , H. L. Clark , C. A. Gagliardi , V. Kroha , Y.-W. Lui , A. M. Mukhamedzhanov , J. Novak , S. Piskor , A. Sattarov , E. Simeckova , X. Tang , L. Trache , J. Vincour

ABSTRACT

Peripheral transfer reactions can be used to determine asymptotic normalization coefficients (ANC). These coefficients, which provide the normalization of the tail of the overlap function, determine S-factors for direct capture reactions at astrophysical energies. A variety of proton transfer reactions have been used to measure ANCs. As a test of the technique, the 16O(3He,d)17F reaction has been used to determine ANCs for transitions to the ground and first excited states of 17F. The S-factors for 16O(p,γ)17F calculated from these 17F → 16O +p ANCs are found to be in very good agreement with recent measurements. Following the same technique, the 10B(7Be,8B)9Be and 14N(7Be,8B)13C reactions have been used, along with optical model parameters for the radioactive beams that were obtained from a study of elastic scattering of loosely bound p-shell nuclei, to measure the ANC appropriate for determining 7Be(p,γ)8B. The results from the two transfer reactions provide an indirect determination of S17(0). Recent measurements have been completed on the 14N(11C, 12N)13C reaction which will allow us to define the astrophysical S-factor for the 11C(p,γ)12N reaction. More... »

PAGES

317-328

Identifiers

URI

http://scigraph.springernature.com/pub.10.1007/978-94-010-0708-5_27

DOI

http://dx.doi.org/10.1007/978-94-010-0708-5_27

DIMENSIONS

https://app.dimensions.ai/details/publication/pub.1014373520


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