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arXiv:astro-ph/9603142 (astro-ph)
[Submitted on 27 Mar 1996 (v1), last revised 9 Apr 1996 (this version, v2)]

Title:Thermal Evolution of Compact Stars

Authors:Ch. Schaab, F. Weber, M.K. Weigel, N.K. Glendenning
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Abstract: 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.
Comments: 41 pages, revised version
Subjects: Astrophysics (astro-ph); Nuclear Theory (nucl-th)
Cite as: arXiv:astro-ph/9603142
  (or arXiv:astro-ph/9603142v2 for this version)
  https://doi.org/10.48550/arXiv.astro-ph/9603142
Journal reference: Nucl.Phys. A605 (1996) 531
Related DOI: https://doi.org/10.1016/0375-9474%2896%2900164-9

Submission history

From: Christoph Schaab [view email]
[v1] Wed, 27 Mar 1996 15:49:50 UTC (161 KB)
[v2] Tue, 9 Apr 1996 13:20:22 UTC (181 KB)
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