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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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Variational study for the equation of state of asymmetric nuclear matter at finite temperatures

TL;DR: In this paper, an equation of state (EOS) for uniform asymmetric nuclear matter (ANM) is constructed at zero and finite temperatures by the variational method starting from the nuclear Hamiltonian that is composed of the Argonne v18 and Urbana IX potentials.
Journal ArticleDOI

Large amplitude behavior of the bulk viscosity of dense matter

TL;DR: In this article, the authors study the bulk viscosity of dense matter, taking into account nonlinear effects that arise in the large amplitude'supra-thermal' region where the deviation of the chemical potentials from chemical equilibrium fulfills.
Journal ArticleDOI

Pulsar glitches as probes of neutron star interiors

TL;DR: In this article, the authors analyzed post-glitch recovery in four pulsars and deduced that the loose component carries at least 8% of the total moment of inertia, independent of the form of the coupling.
Journal ArticleDOI

Equation of state of dense nuclear matter and neutron star structure from nuclear chiral interactions

TL;DR: In this article, a new microscopic equation of state (EOS) of dense symmetric nuclear matter, pure neutron matter, and asymmetric and β-stable nuclear matter at zero temperature was derived in the framework of chiral perturbation theory.
Journal ArticleDOI

Viscous damping of r-modes: Large amplitude saturation

TL;DR: In this article, the authors analyzed the viscous damping of r-mode oscillations of compact stars, taking into account non-linear viscous effects in the large-amplitude regime.
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