Capture Gamma Reaction Rates at Stellar Energies by the Asymptotic Normalization Coefficient Method

Details Capture Gamma Reaction Rates at Stellar Energies by the Asymptotic Normalization Coefficient Method Capture Gamma Reaction Rates at Stellar Energies by the Asymptotic Normalization Coefficient Method

Jun 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003cgrs.conf..298t&link_type=abstract

CAPTURE GAMMA-RAY SPECTROSCOPY AND RELATED TOPICS. Proceedings of the Eleventh International Symposium. Held 2-6 September 2002

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Peripheral transfer reactions can be used to determine asymptotic normalization coefficients (ANCs). These coefficients, which provide the normalization of the tail of the overlap function for a proton bound to a nucleus, determine S factors for direct capture reactions at astrophysical energies. A variety of proton transfer reactions have been used to measure ANCs using both stable and radioactive beams. The technique of utilizing ANCs to predict astrophysical S factors has been tested for 9Be(p, γ)10B, 16O(p, γ)17F and recently 13C(p, γ)14N using ANCs from transfer reaction measurements. Recent applications include measurements of ANCs appropriate for determining stellar reaction rates for 7Be(p, γ)8B, 11C(p, γ)12N and 14N(p, γ)15O.

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