Radiative capture reaction 7(p,γ)8B at low energies

Details Radiative capture reaction 7(p,γ)8B at low energies Radiative capture reaction 7(p,γ)8B at low energies

Jan 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987phrvc..35..363k&link_type=abstract

Physical Review C (Nuclear Physics), Volume 35, Issue 1, January 1987, pp.363-366

Physics

Nuclear Physics

90

Nuclear Reaction Models And Methods, Radiative Capture

Scientific paper

We calculated the differential cross sections as well as the total cross sections for the 7Be(p,γ)8B at low energies in the radiative direct capture model including the E1, M1, and E2 transitions. The astrophysical S factor at the solar temperature of 20 keV is found to be 0.024 keV which agrees well with a recent measurement by Filippone et al. We show that the d-wave capture plays an important role in determining the magnitude and shape of S(E) at low energies of astrophysical interest.

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