Nuclei in the Cosmos 2000 , Aarhus , Denmark , June 27 - July 1 , 2000

Abstract

The most detailed calculations of the p-process call for its development in the O/Ne layers of Type II supernovae. In spite of their overall success in reproducing the solar system content of p-nuclides, they suggest a significant underproduction of the light Mo and Ru isotopes. On grounds of a model for the explosion of a 25 M star with solar metallicity… (More)

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