Video URL

https://pirsa.org/11060014

Equation of State and Neutrino Opacity in Core Collapse Supernova

Shen, G. (2011). Equation of State and Neutrino Opacity in Core Collapse Supernova. Perimeter Institute for Theoretical Physics. https://pirsa.org/11060014

Shen, Gang. Equation of State and Neutrino Opacity in Core Collapse Supernova. Perimeter Institute for Theoretical Physics, Jun. 20, 2011, https://pirsa.org/11060014 

          @misc{ scivideos_PIRSA:11060014,
            doi = {10.48660/11060014},
            url = {https://pirsa.org/11060014},
            author = {Shen, Gang},
            keywords = {Particle Physics},
            language = {en},
            title = {Equation of State and Neutrino Opacity in Core Collapse Supernova},
            publisher = {Perimeter Institute for Theoretical Physics},
            year = {2011},
            month = {jun},
            note = {PIRSA:11060014 see, \url{https://scivideos.org/pirsa/11060014}}
          }

Gang Shen Los Alamos National Laboratory

DOI 10.48660/11060014
Source Repository PIRSA
Collection
Talk Type Conference
Subject

Abstract

We present new equations of state (EOS) of nuclear matter for a wide range of temperatures densities and proton fractions for use in supernova and neutron star merger simulations. We employ a full relativistic mean field (RMF) calculation for matter at intermediate density and high density and the Virial expansion of a nonideal gas for matter at low density. We tabulate the resulting EOS in the temperature range T = 0 - 80 MeV the density range nB = 10â