Behaviour of radiative-capture reactions near zero energy

Details Behaviour of radiative-capture reactions near zero energy Behaviour of radiative-capture reactions near zero energy

Jul 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005nupha.758..114b&link_type=abstract

Nuclear Physics A, Vol. 758, p.114-117

Physics

Nuclear Physics

1

Scientific paper

The Taylor expansion of the astrophysical S factor for radiative-capture reactions between charged particles is calculated in a direct way near zero energy in the potential and R matrix models. The 14N(p,γ)15O reaction is treated as an example. A similar expansion derived for neutron capture provides simple low-energy parametrizations of the 12C(n,γ)13C cross sections.

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