Journal ArticleDOI
The Ground state of matter at high densities: Equation of state and stellar models
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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.read more
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Quark core impact on hybrid star cooling
TL;DR: In this article, the authors investigated the thermal evolution of hybrid stars, objects composed of a quark matter core, enveloped by ordinary hadronic matter, and found a set of microscopic parameters that lead to a good agreement with those of observed cooling neutron stars.
Journal ArticleDOI
The Thermal Evolution of Ultramagnetized Neutron Stars
Jeremy S. Heyl,Lars Hernquist +1 more
TL;DR: In this article, the effects of ultrastrong magnetic fields on the thermal evolution of a neutron star were estimated using analytic and numerical models for the thermal structure of ultramagnetized neutron stars.
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Tabulated equation of state for supernova matter including full nuclear ensemble
Nihal Büyükçizmeci,Nihal Büyükçizmeci,A. S. Botvina,A. S. Botvina,Igor Mishustin,Igor Mishustin +5 more
TL;DR: In this paper, a database of stellar matter properties calculated within the framework of the Statistical Model for Supernova Matter (SMSM) is presented, where the main ingredients of the SMSM are briefly outlined, and the data structure and content of the tables are explained.
Journal ArticleDOI
Pressure of degenerate and relativistic electrons in a superhigh magnetic field
TL;DR: In this article, the authors deduced a general formula for pressure of degenerate and relativistic electrons, P-e, which is suitable for superhigh magnetic fields, and discussed the quantization of Landau levels of electrons, and considered the quantum electrodynamic (QED) effects on the equations of states (EOSs) for different matter systems.
Journal ArticleDOI
Consistent Skyrme parametrizations constrained by GW170817
TL;DR: In this paper, Dutra et al. studied the high-density behavior of stellar matter composed of nucleons and leptons under equilibrium and charge neutrality conditions with the Skyrme parametrizations shown to be consistent with nuclear matter, pure neutron matter, symmetry energy and its derivatives.
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