On Production of Neutron-Rich Iron-Group Isotopes in Simple Models of Dense Thermonuclear Supernovae

Details On Production of Neutron-Rich Iron-Group Isotopes in Simple Models of Dense Thermonuclear Supernovae On Production of Neutron-Rich Iron-Group Isotopes in Simple Models of Dense Thermonuclear Supernovae

Mar 2012

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2012lpi....43.2293y&link_type=abstract

43rd Lunar and Planetary Science Conference, held March 19–23, 2012 at The Woodlands, Texas. LPI Contribution No. 1659, id.2293

Physics

Scientific paper

We presented a simple thermonuclear (Type Ia) supernovae model that
shows for high initial density (low entropy) most of the yield would be
neutron-rich iron-group isotopes. This may help to explain the excesses
and deficits correlation in FUN CAIs.

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