Constraints on the High-Density Nuclear Equation of State from Neutron Star Observables

Details Constraints on the High-Density Nuclear Equation of State from Neutron Star Observables Constraints on the High-Density Nuclear Equation of State from Neutron Star Observables

2008-08-08

arxiv.org/abs/0808.1279v2

Astronomy and Relativistic Astrophysics: New Phenomena and New States of Matter in the Universe}, Word Scientific (2010), p. 3

Astronomy and Astrophysics

Astrophysics

16 pages, 11 figures, Contribution to Proceedings of the 3rd International Workshop on Astronomy and Relativistic Astrophysics

Scientific paper

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.

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