Thermal Evolution of Compact Stars

Details Thermal Evolution of Compact Stars Thermal Evolution of Compact Stars

1996-03-27

arxiv.org/abs/astro-ph/9603142v2

Nucl.Phys. A605 (1996) 531

Astronomy and Astrophysics

Astrophysics

41 pages, revised version

Scientific paper

10.1016/0375-9474(96)00164-9

A collection of modern, field-theoretical equations of state is applied to the investigation of cooling properties of compact stars. These comprise neutron stars as well as hypothetical strange matter stars, made up of absolutely stable 3-flavor strange quark matter. Various uncertainties in the behavior of matter at supernuclear densities, e.g., hyperonic degrees of freedom, behavior of coupling strengths in matter, pion and meson condensation, superfluidity, transition to quark matter, absolute stability of strange quark matter, and last but not least the many-body technique itself are tested against the body of observed cooling data.

Affiliated with

Also associated with

No associations

Rating

Thermal Evolution of Compact Stars 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 Thermal Evolution of Compact Stars, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Thermal Evolution of Compact Stars will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-697133