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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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Enfriamiento de estrellas de neutrones a través de la emisión de neutrinos producidos en el proceso Urca directo

TL;DR: In this paper, the enfriamiento de estrellas de neutrones (NS) a traves de the emision de neutrinos producto del proceso Urca Directo (DUrca) was analyzed.
Journal ArticleDOI

Numerically Fitting The Electron Fermi Energy and The Electron Fraction in A Neutron Star

TL;DR: In this article, a special solution to electron Fermi energy of degenerate and relativistic electrons was obtained using numerically fitting, which can be universally suitable for the electron regions in the circumstances of common neutron stars.
Journal ArticleDOI

Exact versus Taylor-expanded energy density in the study of the neutron star crust–core transition

TL;DR: In this article, the importance of the fourth and higher order terms in the Taylor series expansion of the energy of asymmetric nuclear matter in the study of the neutron star crust-core phase transition is investigated using the finite range simple effective interaction.
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Constraints on the Neutron Star Equation of State from GW170817

TL;DR: The first detection of gravitational waves from a neutron star-neutron star merger, GW170817, has opened up a new avenue for constraining the ultradense-matter equation of state (EOS) as discussed by the authors.
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GW170817: observation of gravitational waves from a binary neutron star inspiral

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