REVIEW 1 cited by
Thermal Evolution of Compact Stars
Not yet reviewed by Pith; the record is open.
This paper has not been read by Pith yet. Machine review is queued; the pith claim, tier, and objections will appear here once it completes.
SPECIMEN: schema-true, not a live event
T0 review · schema-true
One-sentence machine reading of the paper's core claim.
pith:XXXXXXXX · record.json · timestamp
Signed reviews
read the original 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.
Forward citations
Cited by 1 Pith paper
-
Unified QMF equation of state for neutron star matter: Static and dynamic properties
The quark mean-field model predicts larger crust clusters and a slower direct-Urca cooling phase than the relativistic mean-field model, while both reproduce the observed crustal cooling of the transient KS 1731-260.
Discussion (0). Continue with ORCID to comment.