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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Analytical representations of unified equations of state of neutron-star matter
Alexander Y. Potekhin,Alexander Y. Potekhin,Anthea Fantina,Nicolas Chamel,J. M. Pearson,Stéphane Goriely +5 more
TL;DR: In this paper, the authors derived analytical representations for two equations of state (EOSs) of neutron-star matter: FPS and SLy, which describe the crust and core of a neutron star using the same physical model.
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Implications from GW170817 and I-Love-Q relations for relativistic hybrid stars
Vasileios Paschalidis,Kent Yagi,David Alvarez-Castillo,David Blaschke,David Blaschke,David Blaschke,Armen Sedrakian +6 more
TL;DR: In this article, a new parametrization for hybrid hadron-quark equations of state, which give rise to low-mass twin stars, and test them against GW170817 is found consistent with the coalescence of a binary hybrid star-neutron star.
Journal ArticleDOI
Effects of Strong Magnetic Fields on Neutron Star Structure
TL;DR: In this article, the authors studied static neutron stars with poloidal magnetic fields and a simple class of electric current distributions consistent with the requirement of stationarity, and they found that magnetic fields are too large for static configurations to exist when the magnetic force pushes a sufficient amount of mass off-center that the gravitational force points outward near the origin in the equatorial plane.
Journal ArticleDOI
GW170817: Constraining the nuclear matter equation of state from the neutron star tidal deformability
Tuhin Malik,N. Alam,N. Alam,M. Fortin,Constança Providência,B. K. Agrawal,B. K. Agrawal,T. K. Jha,Bharat Kumar,Bharat Kumar,S. K. Patra,S. K. Patra +11 more
TL;DR: In this paper, a set of relativistic and non-relativistic mean field models were examined by using the values of the tidal deformability, inferred from GW170817, for key parameters of the nuclear matter equation of state.
Journal ArticleDOI
Neutron Stars—Cooling and Transport
TL;DR: In this paper, the basics of thermal evolution for isolated neutron stars with strong magnetic fields are reviewed, including most relevant thermodynamic and kinetic properties in the stellar core, crust, and blanketing envelopes.
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