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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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On the Sound Speed in Neutron Stars

TL;DR: In this paper , the authors constructed more than 107 equations of state (EOSs) with continuous sound speed and built more than 108 nonrotating stellar models consistent with nuclear theory and perturbative QCD, but also with astronomical observations.
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Bayesian Inference of the Symmetry Energy of Super-Dense Neutron-Rich Matter from Future Radius Measurements of Massive Neutron Stars

TL;DR: Using an explicitly isospin-dependent parametric Equation of State (EOS) for the core of neutron stars (NSs) within the Bayesian statistical approach, the authors infer the EOS parameters of super-dense neutron-rich nuclear matter from three sets of imagined mass-radius correlation data representing typical predictions by various nuclear many-body theories.
Journal ArticleDOI

Accretion of a massive magnetized torus on a rotating black hole

TL;DR: In this paper, numerical simulations of the axisymmetric accretion of a massive magnetized plasma torus on a rotating black hole were presented, and the authors used a realistic equation of state, which took into account neutrino cooling and energy loss due to nucleus dissociations.
Journal ArticleDOI

Structure of the Electrospheres of Bare Strange Stars

TL;DR: In this article, the authors considered a thin layer of electrons (the electrosphere) at the quark surface of a bare star, taking into account the surface effects at the boundary with the vacuum.
Journal ArticleDOI

Quark mass effects on the stability of hybrid stars

TL;DR: In this paper, it was shown that the constituent mass of the nonstrange quarks in vacuum is a very important parameter that controls the beginning of the hadron-quark phase transition.
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