Physics
Scientific paper
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.
Shen Hao
Wang Nun-Yii
Wen Wei
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