An extended equation of state for simulations of stellar collapse

Details An extended equation of state for simulations of stellar collapse An extended equation of state for simulations of stellar collapse

Dec 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010sf2a.conf..185o&link_type=abstract

SF2A-2010: Proceedings of the Annual meeting of the French Society of Astronomy and Astrophysics. Eds.: S. Boissier, M. Heydari-

Astronomy and Astrophysics

Astrophysics

1

Core Collapse, Equation Of State, Dense Matter

Scientific paper

In core-collapse events matter is heated and compressed to densities above nuclear matter saturation density. For progenitors with masses above about 25 solar masses, which eventually form a black hole, the temperatures and densities reached during the collapse are so high that a traditional description in terms of electrons, nuclei, and nucleons is no longer adequate. We will present here an improved equation of state which contains in addition pions and hyperons. They become abundant in the high temperature and density regime, and we will discuss the effect on the thermodynamic properties.

Affiliated with

Also associated with

No associations

Rating

An extended equation of state for simulations of stellar collapse does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with An extended equation of state for simulations of stellar collapse, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and An extended equation of state for simulations of stellar collapse will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1311376