1987
DOI: 10.1063/1.527697
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General exact solutions of Einstein equations for static perfect fluids with spherical symmetry

Abstract: The gravitational field equations for a spherical symmetric perfect fluid are completely solved. The general analytical solution obtained depends on an arbitrary function of the radial coordinate. As illustrations of the proposed procedure the exterior and interior Schwarzschild solutions are regained.

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Cited by 36 publications
(24 citation statements)
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“…It should be stressed that the physical variables ρ, p and p ⊥ as well as the metric coefficients e λ and e ν can be obtained as known functions of for a given g(r) and ω(r). Following Berger et al (1987) equation (15) can be integrated to give…”
Section: Field Equations and Generating Functionmentioning
confidence: 99%
“…It should be stressed that the physical variables ρ, p and p ⊥ as well as the metric coefficients e λ and e ν can be obtained as known functions of for a given g(r) and ω(r). Following Berger et al (1987) equation (15) can be integrated to give…”
Section: Field Equations and Generating Functionmentioning
confidence: 99%
“…The method is a generalization of one originally developed by Berger et al (1987) for isotropic fluid sphere, and later applied to charged perfect fluid case by Pantino and Rago (1989) in GR and Khadekar and Kandalkar (2004) representing neutral sphere in bimetric relativity. The approach of this work is based on the introduction of the generating function.…”
Section: Introductionmentioning
confidence: 98%
“…Whereas some steps toward finding all possible solutions to the perfect fluid constraint in the absence of a specific equation of state were presented in work early of Wyman and Hojman et al [4,5], explicit and fully general solutions of the perfect fluid constraint have only very recently been developed [6,7]. In this article we present a variant of Lake's algorithm [7] using curvature coordinates wherein:…”
Section: Introductionmentioning
confidence: 99%