Asymptotic normalization coefficients and astrophysical radiative capture reactions

Details Asymptotic normalization coefficients and astrophysical radiative capture reactions Asymptotic normalization coefficients and astrophysical radiative capture reactions

Mar 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998nupha.631..788m&link_type=abstract

Nuclear Physics A, Volume 631, Issue 1-4, p. 788-792.

Physics

Nuclear Physics

Scientific paper

The differential cross sections for the reactions 9Be(10B, 9Be)10B at an incident 10B energy of 100MeV and 16O(3He,d)17F*(0.495MeV, 1/2+) at an incident 3He energy of 29.75MeV were measured. By normalizing the theoretical DWBA proton exchange cross sections to the experimental ones, the asymptotic normalization coefficients (ANC's) for the virtual decays 10B-->9Be+p and 17F*(0.495MeV)-->16O+p have been found. These ANC's are used to calculate the S(0)-factors for the direct radiative captures 9Be+p-->10B+γ and 16O+p-->17F*(0.495MeV)+γ.

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