Asymptotic Normalization Coefficients of ^10B → ^9Be + p and the astrophysical factor for direct capture ^9Be(p,γ)^10B

Details Asymptotic Normalization Coefficients of ^10B → ^9Be + p and the astrophysical factor for direct capture ^9Be(p,γ)^10B Asymptotic Normalization Coefficients of ^10B → ^9Be + p and the astrophysical factor for direct capture ^9Be(p,γ)^10B

Oct 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997aps..dnp..cd06m&link_type=abstract

American Physical Society, Division of Nuclear Physics Meeting, October 5-8, 1997, abstract #CD.06

Physics

Nuclear Physics

Scientific paper

In previous work we have found the asymptotic normalization coefficients (ANC) for the virtual decays of the ground and first three excited states of ^10B to ^9Be + p from analysis of the proton transfer reaction ^9Be(^10B,^9Be)^10B. These ANC's are used to calculate the rate for the direct radiative capture ^9Be + p → ^10B + γ which turns out to be higher than previously reported. Using the calculated rate we fit the experimental astrophysical S-factor at low energies which includes the contribution from the resonance and direct captures using the standard resonance parameters. Comparison with the previously reported fit will be given.

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