Equation of State and Neutrino Opacity of Dense Stellar Matter

Details Equation of State and Neutrino Opacity of Dense Stellar Matter Equation of State and Neutrino Opacity of Dense Stellar Matter

Sep 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004rpao.conf...89r&link_type=abstract

THE r-PROCESS The Astrophysical Origin of the Heavy Elements and Related Rare Isotope Accelerator Physics. Proceedings of the Fi

Physics

Nuclear Physics

Nuclear Theory

Scientific paper

The properties of matter at densities similar to nuclear density plays an important role in core collapse supernova. In this talk I discuss aspects of the equation of state and weak interactions at high density. I highlight its relation to the temporal and spectral features of the neutrino emission from the newly born neutron star born in the aftermath of a core-collapse supernova. I will briefly comment on how this will impact r-process nucleosynthesis.

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