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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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Compact stars for undergraduates
TL;DR: In this article, an undergraduate student project initiated in the summer semester of 2004 with the aim to establish equations of state for white dwarfs and neutron stars for computing mass-radius relations as well as corresponding maximum masses.
Journal ArticleDOI
Combined Rastall and rainbow theories of gravity with applications to neutron stars
TL;DR: In this paper, an alternative theory of gravity constructed with the combination of Rastall and rainbow theories was proposed, and the hydrostatic equilibrium equations were obtained in order to test the new theory in neutron stars, whose mass-radius diagrams are obtained using modern equations of state of nuclear matter derived from relativistic mean field models and compared with the ones computed by the Tolman-Oppenheimer-Volkoff equations.
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Oscillation modes of hybrid stars within the relativistic Cowling approximation
TL;DR: In this article, a relativistic Cowling approximation was used to calculate the oscillations of compact stars focusing on hybrid stars, with and without a mixed phase in their cores.
Journal ArticleDOI
Discontinuity gravity modes in hybrid stars: Assessing the role of rapid and slow phase conversions
L. Tonetto,Germán Lugones +1 more
TL;DR: In this paper, the role of the conversion rate at the interface of a quark-hadron hybrid star was studied and its properties were analyzed using modern hadronic and quark equations of state.
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Constraining the neutron-matter equation of state with gravitational waves
Michael McNeil Forbes,Michael McNeil Forbes,Suvadeep Bose,Suvadeep Bose,Sanjay Reddy,Dake Zhou,Arunava Mukherjee,Arunava Mukherjee,Soumi De +8 more
TL;DR: In this paper, the authors show how observations of gravitational waves from binary neutron star (BNS) mergers over the next few years can be combined with insights from nuclear physics to obtain useful constraints on the equation of state of dense matter.
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