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A class of relativistic stars with a linear equation of state

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arxiv gr-qc/0702046 v1 pith:FUGYIJAA submitted 2007-02-08 gr-qc

R. Sharma , S. D. Maharaj This is my paper · ORCID
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 3 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. On Modeling Anisotropic Quark Stars: The Role of Anisotropy in Radial Oscillation Spectra

    gr-qc 2026-08 conditional novelty 6.0 of 10

    Radial oscillation spectra of an anisotropic strange quark star model of Cen X-3 are computed for three anisotropy prescriptions and differ by up to 40 percent between models.

  2. Relativistic strange quark stars in Lovelock gravity

    gr-qc 2019-07 unverdicted novelty 5.0 of 10

    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.

  3. Anisotropic strange quark stars with a non-linear equation-of-state

    gr-qc 2019-07 unverdicted novelty 4.0 of 10

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

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