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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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Equation of state of dense matter and the minimum mass of cold neutron stars

TL;DR: In this article, the equilibrium congurations of cold neutron stars near the minimum mass are studied, using the recent equation of state SLy model, which describes in a unied, physically consistent manner, both the solid crust and the liquid core of neutron stars.
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Impact of the nuclear equation of state on the last orbits of binary neutron stars

TL;DR: In this article, the authors presented quasi-equilibrium sequences of irrotational binary neutron stars based on realistic equations of state (EOS) for the whole neutron star interior.
Journal ArticleDOI

Kaon condensation in the quark-meson coupling model and compact stars

TL;DR: In this paper, the properties of neutron stars, consisting of a crust of hadrons and an internal part of hadron and kaon condensate, are calculated within the quark-meson-coupling model.
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Hyperon-mixed neutron star with universal many-body repulsion

TL;DR: In this paper, a multi-pomeron exchange potential (MPP) was introduced as a model for the universal many-body repulsion in baryonic systems on the basis of the Extended Soft Core (ESC) baryon-baryon interaction.
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New Neutron Star Equation of State with Quark-Hadron Crossover

TL;DR: In this paper, Togashi et al. presented a much improved equation of state for neutron star matter, QHC19, with a smooth crossover from the hadronic regime at lower densities to the quark regime at higher densities.
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