Nucleosynthesis in Neutrino-Driven Supernovae

Details Nucleosynthesis in Neutrino-Driven Supernovae Nucleosynthesis in Neutrino-Driven Supernovae

2005-11-18

arxiv.org/abs/astro-ph/0511584v1

New Astron.Rev.50:496-499,2006

Astronomy and Astrophysics

Astrophysics

7 pages, 2 figures, in proceedings of Astronomy with Radioactivities V, Clemson University, September 5-9, 2005, to appear in

Scientific paper

10.1016/j.newar.2006.06.003

Core collapse supernovae are the leading actor in the story of the cosmic origin of the chemical elements. Existing models, which generally assume spherical symmetry and parameterize the explosion, have been able to broadly replicate the observed elemental pattern. However, inclusion of neutrino interactions produces noticeable improvement in the composition of the ejecta when compared to observations. Neutrino interactions may also provide a supernova source for light p-process nuclei.

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