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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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Impact of error analysis on the composition the outer crust of a neutron star

TL;DR: In this article, a full error analysis on the Duflo-Zucker mass model was performed on the outer crust of a non-accreting neutron star and the existence probability for each nuclear species was defined as a function of the depth of the crust.
Journal ArticleDOI

Searching optimum equations of state of neutron star matter in strong magnetic fields with rotation

TL;DR: In this article, the mass and radius of a neutron star were obtained in the presence of strong magnetic fields together with rotation in relativistic mean field (RMF) theory.
Journal ArticleDOI

EOS of nuclear matter at finite temperature and density in the 1/N expansion of the relativistic σ-ω model

TL;DR: In this article, the thermodynamic potential for nuclear matter is calculated in the 1/n expansion of the relativistic σ-ω model, which is used in this paper.

Direct URCA process in light of PREX-2

TL;DR: In this article , the authors study the implications of the recent development in nuclear symmetry energy constraints from PREX-2 data on dense matter equation of state and its impact on dURCA threshold density.
Journal ArticleDOI

Thermal state of transiently accreting neutron stars with additional heating beyond deep crustal heating

TL;DR: In this paper, the authors investigated the effect of shallow heating as well as compressional heating on the thermal state of transiently accreting neutron stars with the use of evolutionary calculations in the present work, and compared their theoretical predictions of the equilibrium redshifted luminosities produced by both deep crustal heating and shallow heating/compressional heating for different time-averaged mass-accretion rates.
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