35Cl(n,p)35S cross section from 25 meV to 100 keV

Details 35Cl(n,p)35S cross section from 25 meV to 100 keV 35Cl(n,p)35S cross section from 25 meV to 100 keV

Oct 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991phrvc..44.1675k&link_type=abstract

Physical Review C (Nuclear Physics), Volume 44, Issue 4, October 1991, pp.1675-1678

Physics

Nuclear Physics

8

Inelastic Neutron Scattering, Stellar Structure, Interiors, Evolution, Nucleosynthesis, Ages, 20<=A<=38

Scientific paper

We have measured the 35Cl(n,p)35S cross section from 25 meV to 100 keV. Strengths were determined for the resonances at En=398, 4249, 16340, 27316, and 57700 eV. The proton width for the J π=2+ state just below threshold was calculated using previously known resonance parameters and the thermal cross section. The cross section calculated from the parameters for this state was found to be in good agreement with our data to approximately 100 eV. The astrophysical reaction rate, NA<σv>, was calculated from the resonance strengths determined in our measurements, plus the thermal cross section. The role of this reaction in the nucleosynthesis of light elements in the s process as well as in explosive nucleosynthesis is discussed.

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