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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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Superfluid Friction and Late-Time Thermal Evolution of Neutron Stars

TL;DR: In this paper, the effects of superfluid friction on the long-term thermal and rotational evolution of a neutron star were studied and it was shown that the velocities between the superfluid and the crust (averaged over the inner crust moment of inertia) of PSR 1929 plus 10 and PSR 0950 plus 8 would account for their observed temperatures.
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Equation of state constraints from nuclear physics, neutron star masses, and future moment of inertia measurements

TL;DR: In this paper, the authors explore constraints on the equation of state (EOS) of neutron-rich matter based on microscopic calculations up to nuclear densities and observations of neutron stars.
Journal ArticleDOI

Hyperon puzzle, hadron-quark crossover and massive neutron stars

TL;DR: In this article, a phenomenological equation of state (EOS) based model of the hadron-quark crossover was used to study the properties of cold and hot neutron stars.
Journal ArticleDOI

Neutron Star Properties in a Chiral SU(3) Model

TL;DR: In this article, the authors investigated various properties of neutron star matter within an effective chiral SU(3)L × SU( 3)R model and compared the predictions of this model with a Walecka-type model.
Journal ArticleDOI

Electrical conductivity of a warm neutron star crust in magnetic fields

TL;DR: In this article, the electrical conductivity tensor of a supernova explosion or a binary neutron star merger was investigated in terms of the polarization tensor computed in the hard-thermal-loop effective field theory of QED plasma and the correlations of the background ionic component were derived from Monte Carlo simulations of one-component plasma.
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