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The general solution for relativistic spherical shells

J. Kijowski·G. Magli·D. Malafarina
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Abstract

The general exact solution of the Einstein-matter field equations describing spherically symmetric shells satisfying an equation of state in closed form is discussed under general assumptions of physical reasonableness. The solutions split into two classes: a class of "astro-physically interesting" solutions describing "ordinary" matter with positive density and pressure, and a class of "phantom-like" solutions with positive density but negative active gravitational mass, which can also be of interest in several "very strong fields" regimes. Known results on linear-barotropic equations of state are recovered as particular cases.

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J. Kijowski, G. Magli, D. Malafarina. 2005-12-15. The general solution for relativistic spherical shells. https://doi.org/10.1142/s0218271809014996

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