Properties of Dense Matter in Neutron Stars and Supernovae

Details Properties of Dense Matter in Neutron Stars and Supernovae Properties of Dense Matter in Neutron Stars and Supernovae

Aug 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010aipc.1269..219s&link_type=abstract

THE 10TH INTERNATIONAL SYMPOSIUM ON ORIGIN OF MATTER AND EVOLUTION OF GALAXIES: OMEG-2010. AIP Conference Proceedings, Volume 1

Physics

1

Neutron Stars, Interstellar Matter, Supernovae, Equations Of State, Neutron Stars, Interstellar Dust Grains, Diffuse Emission, Infrared Cirrus, Supernovae, Equations Of State Of Nuclear Matter

Scientific paper

We study the equation of state (EOS) of nuclear matter at finite temperature density with various proton fractions for use in supernova simulations. The properties of nuclear matter with both uniform and non-uniform distributions are studied consistently. We also discuss the EOS of neutron star matter at zero temperature in a wide density range including hyperons antikaons quarks. The EOS of neutron star matter could be softened by incorporating these new degrees of freedom.

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