Astrophysical S-factors from asymptotic normalization coefficients View Full Text


Ontology type: schema:ScholarlyArticle     


Article Info

DATE

1999-09

AUTHORS

RE Tribble, A Azhari, HL Clark, CA Gagliardi, Y-W Lui, AM Mukhamedzhanov, A Sattaroy, X Tang, L Trache, V Burjan, J Cejpek, V Kroha, S Piskor, J Vincour, F Carstoiu

ABSTRACT

S-factors for direct capture reactions can be found at astrophysical energies from asymptotic normalization coefficients which provide the normalization of the tail of the overlap function. For example the overlap for 8B → 7Be+p defines the S-factor for 7Be (p, γ)8B. Peripheral transfer reactions offer a technique to determine these asymptotic normalization coefficients. As a test of the technique, the 16O(3He, d)17F reaction has been used to determine asymptotic normalization coefficients 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 asymptotic normalization coefficients 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 to measure the asymptotic normalization coefficient for 7Be(p, γ)8B. This result provides an indirect determination of S17(0). More... »

PAGES

585-594

Identifiers

URI

http://scigraph.springernature.com/pub.10.1007/s12043-999-0035-6

DOI

http://dx.doi.org/10.1007/s12043-999-0035-6

DIMENSIONS

https://app.dimensions.ai/details/publication/pub.1011336000


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