Production of Nitrogen-15 in Explosive Helium Burning and Supernova Presolar Grains

Details Production of Nitrogen-15 in Explosive Helium Burning and Supernova Presolar Grains Production of Nitrogen-15 in Explosive Helium Burning and Supernova Presolar Grains

Mar 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011lpi....42.2376m&link_type=abstract

42nd Lunar and Planetary Science Conference, held March 7–11, 2011 at The Woodlands, Texas. LPI Contribution No. 1608, p.2376

Physics

Scientific paper

Production of nitrogen-15 in explosive helium burning occurs by
sequences of alpha and neutron capture reactions. Shocks stronger than
in current supernova models increase the rates for these reactions and
may help explain the N isotopes in presolar-grain SiC-X grains.

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