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arXiv · 0808.1279

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

David Blaschke·Thomas Klaehn·Fridolin Weber
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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.

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David Blaschke, Thomas Klaehn, Fridolin Weber. 2008-08-10. Constraints on the High-Density Nuclear Equation of State from Neutron Star Observables. https://doi.org/10.1142/9789814304887_0003

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