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Neutron star matter

Nuclear Physics A, 1971
Abstract The matter in neutron stars is essentially in its ground state and ranges in density up to and beyond 3 × 10 14 g/cm 3 , the density of nuclear matter. Here we determine the constitution of the ground state of matter and its equation of state in the regime from 4.3 × 10 11 g/cm 3 where free neutrons begin to “drip” out of the nuclei, up ...
GORDON BAYM   +2 more
openaire   +1 more source

Neutron star cores

Astrophysics and Space Science, 1975
Current theories, and the astrophysical implications, of the nature of high density neutron star matter are reviewed. Suggestions are made for a compromise between the alternatives of neutron crystallization and pion condensation.
openaire   +1 more source

Coalescence of black hole–neutron star binaries

Living Reviews in Relativity, 2021
Keisuke Taniguchi   +2 more
exaly  

GW170817: Measurements of Neutron Star Radii and Equation of State

Physical Review Letters, 2018
Stefano Ascenzi, Heinz-Bernd Eggenstein
exaly  

Colloquium: Measuring the neutron star equation of state using x-ray timing

Reviews of Modern Physics, 2016
Gian Luca Israel   +2 more
exaly  

Masses, Radii, and the Equation of State of Neutron Stars

Annual Review of Astronomy and Astrophysics, 2016
Paulo Freire, Feryal Özel
exaly  

Neutron Skins and Neutron Stars in the Multimessenger Era

Physical Review Letters, 2018
Farrukh Fattoyev   +2 more
exaly  

Properties of the Binary Neutron Star Merger GW170817

Physical Review X, 2019
Stefano Ascenzi   +2 more
exaly  

Thermal luminosities of cooling neutron stars

Monthly Notices of the Royal Astronomical Society, 2020
Alexander Y. Potekhin   +2 more
exaly  

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