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The Ground state of matter at high densities: Equation of state and stellar models

Gordon Baym, +2 more
- 01 Jan 1971 - 
- Vol. 170, pp 299-317
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This article is published in The Astrophysical Journal.The article was published on 1971-01-01. It has received 1314 citations till now. The article focuses on the topics: Ground state & Equation of state.

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Neutrino emissivity in the quark-hadron mixed phase of neutron stars

TL;DR: In this article, the effect of a quark-hadron mixed phase on the neutrino emissivity from the core of a neutron star was investigated, using the relativistic mean-field approximation to model hadronic matter and a nonlocal extension of the three-flavor Nambu-Jona-Lasinio model for quark matter.
Journal ArticleDOI

Maximum mass and universal relations of rotating relativistic hybrid hadron-quark stars

TL;DR: In this paper, the authors construct equilibrium models of uniformly and differentially rotating hybrid hadron-quark stars using equations of state (EOSs) with a first-order phase transition that gives rise to a third family of compact objects.
Journal ArticleDOI

Nuclear Statistical Equilibrium equation of state for core collapse

TL;DR: In this article, the authors presented extensive calculations of properties of supernova matter using the extended Nuclear Statistical Equilibrium model of Ref. [1] based on a statistical distribution of Wigner-Seitz cells modeled using realistic nuclear mass and level density tables, complemented with a non-relativistic Skyrme functional for unbound particles and beyond drip-line nuclei.
Journal ArticleDOI

Maximum mass of a hot neutron star with a quark core

TL;DR: In this article, the authors considered a hot neutron star with a quark core, a mixed phase of quark-hadron matter, and a hadronic matter crust and determined the equation of state of the hadronic phase and the quark phase.
Journal ArticleDOI

Cooling of neutron stars in "nuclear medium cooling scenario" with stiff equation of state including hyperons

TL;DR: In this article, the authors demonstrate that the existing neutron-star cooling data can be appropriately described within the nuclear medium cooling scenario including hyperons under the assumption that different compact-star sources have different masses.
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