Anisotropic stars in general relativity

DOI10.1098/RSPA.2002.1014zbMATH Open1029.83023arXivgr-qc/0110103OpenAlexW3105849999MaRDI QIDQ4405526

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Publication date: 6 February 2004

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Abstract: 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.

Full work available at URL: https://arxiv.org/abs/gr-qc/0110103

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