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Anisotropic Stars in General Relativity

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arxiv gr-qc/0110103 v2 pith:WKEZ2SKQ submitted 2001-10-24 gr-qc

M. K. Mak , T. Harko This is my paper · ORCID
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keywords anisotropicsolutionsstarsanisotropyassumingastrophysicalbasicclass
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We present a class of exact solutions of Einstein's gravitational field equations describing spherically symmetric and static anisotropic stellar type configurations. The solutions are obtained by assuming a particular form of the anisotropy factor. The energy density and both radial and tangential pressures are finite and positive inside the anisotropic star. Numerical results show that the basic physical parameters (mass and radius) of the model can describe realistic astrophysical objects like neutron stars.

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  1. Anisotropic quantum polytropes

    gr-qc 2025-06 reject novelty 5.0 of 10

    In pressureless quantum polytropes, positive pressure anisotropy compresses the structure and stronger gravity weakens binding, opposite to classical polytrope behavior.

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