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Charged anisotropic matter with a linear equation of state, Classical and Quantum Gravity

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TLDR
In this paper, the authors considered the general situation of a compact relativistic body with anisotropic pressures in the presence of the electromagnetic field and found three classes of new exact solutions to the Einstein-Maxwell system.
Abstract
We consider the general situation of a compact relativistic body with anisotropic pressures in the presence of the electromagnetic field. The equation of state for the matter distribution is linear and may be applied to strange stars with quark matter. Three classes of new exact solutions are found to the Einstein–Maxwell system. This is achieved by specifying a particular form for one of the gravitational potentials and the electric field intensity. We can regain anisotropic and isotropic models from our general class of solutions. A physical analysis indicates that the charged solutions describe realistic compact spheres with anisotropic matter distribution. The equation of state is consistent with dark energy stars and charged quark matter distributions. The masses and central densities correspond to realistic stellar objects in the general case when anisotropy and charge are present.

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Charged anisotropic matter with linear or nonlinear equation of state

TL;DR: In this paper, the authors extended Krori and Barua's method to include pressure anisotropy and linear or nonlinear equations of state for self-gravitating, charged, anisotropic fluids and get even more flexibility in solving the Einstein-Maxwell equations.
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Some charged polytropic models

TL;DR: In this article, a polytropic equation of state with anisotropic pressures and electromagnetic field was used to obtain exact solutions for the relativistic compact stars and a neutral anisotropy gravitating body for a polytrope.
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Charged anisotropic matter with quadratic equation of state

TL;DR: In this article, the authors extended the work of Thirukkanesh and Maharaj (Class Quantum Gravity 25:235001, 2007) by considering quadratic equation of state for the matter distribution to study the general situation of a compact relativistic body.
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Exact anisotropic sphere with polytropic equation of state

TL;DR: In this paper, the authors study static spherically symmetric spacetime to describe compact objects with anisotropic matter distribution, and express the system of Einstein field equations as a new system of differential equations using a coordinate transformation.
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Regular models with quadratic equation of state

TL;DR: In this paper, the authors provided new exact solutions to the Einstein-Maxwell system of equations which are physically reasonable and showed that the spacetime is static and spherically symmetric with a charged matter distribution.
References
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Cosmic separation of phases

TL;DR: In this paper, a first-order QCD phase transition that occurred reversibly in the early universe would lead to a surprisingly rich cosmological scenario, which is at least conceivable that the phase transition would concentrate most of the quark excess in dense, invisible quark nuggets, providing an explanation for the dark matter in terms of QCD effects only.
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TL;DR: In this paper, the theory of the internal structure of stars and their evolution in time is introduced and the basic physics of stellar interiors, methods for solving the underlying equations, and the most important results necessary for understanding the wide variety of stellar types and phenomena.
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Pulsars: Structure and Dynamics

TL;DR: In the two years since the review of Hewish (1970) the number of observed pulsars has increased modestly from 50 to 58 (November 1971), accompanied by a plethora of over three hundred theoretical papers.
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