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arxiv: gr-qc/0702046 · v1 · submitted 2007-02-08 · 🌀 gr-qc

A class of relativistic stars with a linear equation of state

R. Sharma , S. D. Maharaj This is my paper
classification 🌀 gr-qc
keywords solutionsstarsclassequationlinearmatterstateadmit
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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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Cited by 2 Pith papers

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    Numerical computation of mass-radius profiles, compactness, and gravitational redshift for strange quark stars in 5D Gauss-Bonnet gravity across several values of the Gauss-Bonnet parameter.

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    Exact analytical solution for anisotropic CFL strange quark stars with non-linear EOS, satisfying energy conditions, yielding mass-radius profiles and compactness values.