The 8Li(d,p)9Li reaction and astrophysical 8B(p,γ)9C reaction rate

Details The 8Li(d,p)9Li reaction and astrophysical 8B(p,γ)9C reaction rate The 8Li(d,p)9Li reaction and astrophysical 8B(p,γ)9C reaction rate

Oct 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005nupha.761..162g&link_type=abstract

Nuclear Physics A, Volume 761, Issue 1-2, p. 162-172.

Physics

Nuclear Physics

13

Transfer Reactions, Spectroscopic Factors And Asymptotic Normalization Coefficients, Radiative Capture, Hydrostatic Stellar Nucleosynthesis

Scientific paper

Angular distribution of the Li8(d,p)Lig.s.9 reaction at E=7.8MeV was measured in inverse kinematics. The square of asymptotic normalization coefficient (ANC) for the virtual decay Li9→Li8+n was derived to be 1.33±0.33fm through distorted wave Born approximation (DWBA) analysis, for the first time. According to charge symmetry, (ANC)2 for C9→B8+p was then extracted to be 1.14±0.29fm. We have deduced the astrophysical S-factors and reaction rates for direct capture in B8(p,γ)C9 at energies of astrophysical relevance using the ANC for C9→B8+p extracted from the mirror system.

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