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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Nearly model-independent constraints on dense matter equation of state in a Bayesian approach
TL;DR: In this paper , the authors apply a Bayesian approach to construct a large number of minimally constrained equations of state (EOSs) and study their correlations with a few selected properties of a neutron star.
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Neutron star sequences and the starquake glitch model for the Crab and the Vela pulsars
TL;DR: In this paper, the authors constructed the sequences of stable neutron star (NS) models capable of explaining simultaneously, the glitch healing parameters, $Q$, of both the pulsars, the Crab and the Vela, on the basis of starquake mechanism of glitch generation, whereas conventional NS models cannot give such consistent explanation.
Journal ArticleDOI
Neutron star structure in a quark model with excluded volume correction
R. Aguirre,A. L. De Paoli +1 more
TL;DR: In this article, the effects of the finite size of baryons on the equation of state of homogeneous hadronic matter were studied in the framework of the Quark Meson Coupling model.
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Hadron-Quark phase transition in the context of GW190814
TL;DR: In this article, the properties of the neutron stars are calculated for the hadronic matter within the density-dependent relativistic mean-field model (DD-RMF), and the phase transition to the quark matter is studied and the hybrid star matter properties are systematically calculated using the Vector-Enhanced Bag model (vBag).
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Astrophysical Constraints on the Symmetry Energy and the Neutron Skin of $^{208}$Pb with Minimal Modeling Assumptions
TL;DR: In this article, a nonparametric equation of state representation based on Gaussian processes was used to constrain the symmetry energy of the neutron-skin thickness and its density dependence from observations of neutron stars with minimal modeling assumptions.
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