Astrophysical S factor for the B11(d,n)C12 reaction below 135 keV

Details Astrophysical S factor for the B11(d,n)C12 reaction below 135 keV Astrophysical S factor for the B11(d,n)C12 reaction below 135 keV

Jul 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006phrvc..74a5804p&link_type=abstract

Physical Review C, vol. 74, Issue 1, id. 015804

Astronomy and Astrophysics

Astrophysics

1

Spectroscopic Factors And Asymptotic Normalization Coefficients, Optical And Diffraction Models, Transfer Reactions

Scientific paper

The B11(d,n)C12 reaction was studied using deuteron beams of 120 160 keV to determine the absolute astrophysical S factors and cross sections for the n0 and n1 neutron groups. The slopes of the S factors are consistent with zero for both the n0 and n1 cases. The measured S factor for the sum of both neutron groups at c.m. energies below 135 keV is S=3180±480 keV b. A DWBA calculation is able to reproduce the ratio of the S factors found here to those obtained in a recent study of the Li7(d,n0,1)Be8 reaction.

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