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Journal ArticleDOI

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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Proceedings ArticleDOI

Delineating the properties of matter in cold, dense QCD

TL;DR: The properties of dense QCD matter are delineated through the construction of equations of state which should be consistent with QCD calculations in the low and high density limits, nuclear laboratory experiments, and the neutron star observations as mentioned in this paper.
Journal ArticleDOI

Crystallization of the outer crust of a non-accreting neutron star

TL;DR: In this paper, the authors study the cooling and equilibrium composition of the outer layers of a neutron star down to crystallization, and show that the presence of impurities in the outer crust of a supernova core is not a trivial issue and may have a sizeable impact on transport properties.
Journal ArticleDOI

Comparison of perturbative and non-perturbative methods in f(R) gravity

TL;DR: In this paper , the structure and properties of neutron stars in the background of f ( R ) gravity were investigated using two approaches, viz: the perturbative and non-perturbative methods.
Journal ArticleDOI

Self-consistently thermodynamic treatment for strange quark matter in the effective mass bag model

TL;DR: In this paper, the thermodynamic treatment for strange quark matter (SQM) self-consistently overcomes the inconsistencies in the thermodynamical properties of the system.
Journal ArticleDOI

Holographic equations of state and astrophysical compact objects

TL;DR: In this paper, the authors solved the Tolman-Oppenheimer-Volkoff equation using an equation of state (EoS) calculated in holographic QCD and showed that the EoS from the D4/D8/\textoverline {D8} model may not support any stable compact stars or may support one whose radius is very large.
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