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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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Unified equation of state for neutron stars and supernova cores using the nuclear energy-density functional theory

TL;DR: In this article, a unified approach to the equation of state (EoS) of dense matter at any temperature, based on the nuclear energy density functional (EDF) theory, was presented.
Journal ArticleDOI

Bayesian Analysis of Neutron-star Properties with Parameterized Equations of State: The Role of the Likelihood Functions

TL;DR: In this article , a Bayesian-inference analysis of the equation of state (EOS) of neutron stars employing either variable- or constant-likelihood functions is presented.

Turbulent Thermonuclear Combustion in Degenerate Stars

TL;DR: In this article, a subgrid scale model is proposed to simulate the burning process of a supernova in a degenerate star, where turbulence is artificially produced by a stochastic force field in a cubic domain.
Journal ArticleDOI

Compressional modes in two-superfluid neutron stars with leptonic buoyancy

TL;DR: In this article, the authors investigate the compressional modes of cold neutron stars with cores consisting of superfluid neutrons, superconducting protons, normal fluid electrons and muons, and crusts that contain superfluide neutrons plus a normal fluid of (spherical) nuclei and electrons.
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Neutron stars with spin polarized self-interacting dark matter

TL;DR: In this article, the authors investigated the structure of neutron stars which are influenced by the spin polarized self-interacting dark matter and the behavior of the neutron star matter and dark matter portions for the stars with different values of the interaction between dark matter particles and spin polarization of dark matter.
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