Abstract
Via a straightforward integration of the Einstein equations with a cosmological constant, all static circularly symmetric perfect fluid solutions are derived. The structural functions of the metric depend on the energy density, which remains, in general, arbitrary. Spacetimes for fluids satisfying linear and polytropic state equations are explicitly derived; they describe, among others, stiff matter, monatomic and diatomic ideal gases, nonrelativistic degenerate fermions, incoherent and pure radiation. As a by-product, we demonstrate the uniqueness of the constant energy density perfect fluid within the studied class of metrics. A full similarity of the perfect fluid solutions with a constant energy density of the and gravities is established.
- Received 5 November 2002
DOI:https://doi.org/10.1103/PhysRevD.67.064014
©2003 American Physical Society