14N(n,p)14C cross section from 61 meV to 34.6 keV and its astrophysical implications

Details 14N(n,p)14C cross section from 61 meV to 34.6 keV and its astrophysical implications 14N(n,p)14C cross section from 61 meV to 34.6 keV and its astrophysical implications

Apr 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989phrvc..39.1655k&link_type=abstract

Physical Review C (Nuclear Physics), Volume 39, Issue 4, April 1989, pp.1655-1657

Physics

Nuclear Physics

34

Inelastic Neutron Scattering, 20<=A<=38, Origin, Formation, And Abundances Of The Elements

Scientific paper

We have measured the 14N(n,p)14C cross section from 61 meV to 34.6 keV. Our data are in agreement with previous measurements made via the inverse reaction, but are approximately a factor of 2.5 larger than a recent direct measurement. As a result, our data support the astrophysical reaction rate used in most previous nucleosynthesis calculations over the recently recommended three-fold reduction in this rate. Astrophysical implications of our new measurements are discussed.

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