A class of relativistic stars with a linear equation of state
R. Sharma, S. D. Maharaj
TL;DR
This paper derives new exact solutions to Einstein's equations for anisotropic compact stars, featuring a linear equation of state suitable for modeling strange stars with quark matter.
Contribution
It introduces a novel class of solutions with a linear equation of state, expanding the modeling options for relativistic stars with anisotropic matter.
Findings
Solutions are relevant for describing strange stars with quark matter.
The solutions satisfy Einstein's field equations with anisotropic matter.
The linear equation of state is a key feature for modeling compact stars.
Abstract
By assuming a particular mass function we find new exact solutions to the Einstein field equations with an anisotropic matter distribution. The solutions are shown to be relevant for the description of compact stars. A distinguishing feature of this class of solutions is that they admit a linear equation of state which can be applied to strange stars with quark matter.
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