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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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Competition between delta isobars and hyperons and properties of compact stars

TL;DR: In this article, the Δ-isobar degrees of freedom are included in the covariant density functional (CDF) theory to study the equation of state (EoS) and composition of dense matter in compact stars.
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Hybrid stars in a strong magnetic field

TL;DR: In this article, the effects of high magnetic fields on the particle population and equation of state of hybrid stars using an extended hadronic and quark SU(3) non-linear realization of the sigma model were studied.
Journal ArticleDOI

Towards understanding astrophysical effects of nuclear symmetry energy

TL;DR: In this article, the authors review recent progress in predicting the nuclear symmetry energy and identify new challenges to the best knowledge we have on several selected topics critical for understanding astrophysical effects of the nuclear symmetric energy.
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Magnetically driven explosions of rapidly rotating white dwarfs following accretion-induced collapse

TL;DR: In this paper, a multigroup flux-limited diffusion magnetohydrodynamics (MHD) simulation of the accretion-induced collapse (AIC) of a rapidly rotating white dwarf is presented.
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Neutron star radii, universal relations, and the role of prior distributions

TL;DR: In this paper, the role of prior assumptions on neutron star structure arising from the assumptions that neutron stars have crusts, that recent calculations of pure neutron matter limit the equation of state of neutron star matter near the nuclear saturation density, and that the high-density equation is limited by causality and that general relativity is the correct theory of gravity.
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