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Journal ArticleDOI

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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Probing the phases of cold ultra-dense matter using neutron star physics

TL;DR: In this paper, the mean free path and kaonic contribution to the shear viscosity of cold dense matter using neutron star physics is investigated, and general analytic solutions as well as numerical solutions for amplitude-dependent bulk viscosities of dense matter are obtained for any equations of state where equilibration occurs via fermions.
Journal ArticleDOI

Nuclear pasta and symmetry energy in the relativistic point-coupling model

TL;DR: In this article, the authors investigated the influence of nuclear symmetry energy and its density dependence on nuclear pasta structures by introducing a coupling term between the isoscalar-vector and isovector-vector interactions.
Journal ArticleDOI

The Equation of State of Nuclear Matter and Neutron Stars Properties

TL;DR: In this article, the authors compared the relativistic Brueckner-Hartree-Fock (BHF) approach with a non-relativistic approach.
Journal ArticleDOI

Inner crust of neutron stars with mass-fitted Skyrme interaction

TL;DR: In this paper, the mass, radius and crustal fraction of moment of inertia in neutron stars are calculated using β-equilibrated nuclear matter obtained from Skyrme effective interaction.
Journal ArticleDOI

General relativistic ray-tracing algorithm for the determination of the electron–positron energy deposition rate from neutrino pair annihilation around rotating neutron and quark stars

TL;DR: In this article, a full general relativistic numerical code for estimating the energy-momentum deposition rate (EMDR) from neutrino pair annihilation is presented, where the source of the neutrinos is assumed to be a neutrini-cooled accretion disc around rotating neutron and quark stars.
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