Constraints on the High-Density Nuclear Equation of State from Neutron Star Observables
classification
🌌 astro-ph
hep-phnucl-th
keywords
matterconstraintsequationhigh-densityneutronnuclearphasesstate
read the original abstract
Depending on the density reached in the cores of neutron stars, such objects may contain stable phases of novel matter found nowhere else in the Universe. This article gives a brief overview of these phases of matter and discusses astrophysical constraints on the high-density equation of state associated with ultra-dense nuclear matter.
This paper has not been read by Pith yet.
discussion (0)
Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.