Physics – Nuclear Physics
Scientific paper
May 1993
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993phrvc..47.2107k&link_type=abstract
Physical Review C (Nuclear Physics), Volume 47, Issue 5, May 1993, pp.2107-2112
Physics
Nuclear Physics
10
Inelastic Neutron Scattering, Stellar Structure, Interiors, Evolution, Nucleosynthesis, Ages, 20<=A<=38
Scientific paper
We have measured the 36Cl(n,p)36S cross section from thermal energy to approximately 800 keV. Parameters for eight resonances between 900 eV and 70 keV were determined in a multilevel fit to our data which also included information from published 36S(p,γ)37Cl measurements. The 36Cl(n,p)36S reaction can play a critical role in the production of the rare isotope 36S in explosive nucleosynthesis and s-process calculations. The astrophysical rate for this reaction was calculated from our measured cross sections and was found to be significantly smaller than the theoretical rate used in previous nucleosynthesis calculations. We discuss the impact of this result on the nucleosynthesis of 36S.
Gledenov Yu. M.
Graff S. M.
Koehler Paul E.
O'Brien H. A.
Popov Yu P.
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