Nucleosynthesis of neutron-rich heavy nuclei during explosive helium burning in a 15 solar-mass supernova

Details Nucleosynthesis of neutron-rich heavy nuclei during explosive helium burning in a 15 solar-mass supernova Nucleosynthesis of neutron-rich heavy nuclei during explosive helium burning in a 15 solar-mass supernova

Oct 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980icrc....2....7b&link_type=abstract

In: International Cosmic Ray Conference, 16th, Kyoto, Japan, August 6-18, 1979, Conference Papers. Volume 2. (A81-12386 02-93) T

Computer Science

Gas Explosions, Heavy Nuclei, Helium, Neutrons, Nuclear Fusion, Supernovae, Abundance, Actinide Series, Combustion, Solar System, Stellar Mass Ejection, Stellar Models

Scientific paper

The production of heavy nuclei during explosive helium burning has been calculated using the Weaver and Woosley self-consistent model of a complete 15 solar-mass star and the n-process code of Blake and Schramm. It was found that the resulting neutron-rich heavy nuclei are not produced in the relative abundances of solar-system r-process material (such as a Pt peak) nor are any actinides produced. Basically insufficient neutrons are available.

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