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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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The Skyrme Interaction in finite nuclei and nuclear matter

TL;DR: In this article, a comprehensive survey of the performance of one of the most successful non-relativistic self-consistent method, the Skyrme-Hartree-Fock model (SHF), with respect to these constraints is presented.
Journal ArticleDOI

Nuclear matter and neutron-star properties calculated with the Skyrme interaction

TL;DR: In this paper, a systematic study of the predictions of the various Skyrme parametrizations for the density dependence of the characteristic observables of nuclear matter was carried out.
Journal ArticleDOI

Constraining Neutron Star Matter with Quantum Chromodynamics

TL;DR: In this paper, the authors demonstrate that significant further restrictions can be placed by additionally requiring the pressure to approach that of deconfined quark matter at high densities, which turns out to be highly insensitive to the amount of quark atoms inside the stars.
Journal ArticleDOI

Quarkyonic Matter and Neutron Stars

TL;DR: This work makes a simple model of quarkyonic matter and shows that generically the sound velocity is a nonmonotonic function of density-it reaches a maximum at relatively low density, decreases, and then increases again to its asymptotic value of 1/sqrt[3].
Journal ArticleDOI

Dense baryon matter calculations with realistic potentials

TL;DR: In this paper, the equation of state for dense hyperonic matter is calculated from five potential interaction models, the form of the potential is the same as that of Reid, a sum of Yukawa functions, the coefficients of which are adjusted separately in each partial wave to fit experimental nucleon nucleon data.
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