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New Solutions of Einstein Equations in Spherical Symmetry: The Cosmic Censor to the Court

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 A new class of solutions of the Einstein field equations in spherical symmetry is found. The new solutions are mathematically described as the metrics admitting separation of variables in area-radius coordinates. Physically, they describe the gravitational collapse of a class of anisotropic elastic materials. Standard requirements of physical acceptability are satisfied, in particular, existence of an equation of state in closed form, weak energy condition, and existence of a regular Cauchy surface at which the collapse begins. The matter properties are generic in the sense that both the radial and the tangential stresses are non-vanishing, and the kinematical properties are generic as well, since shear, expansion, and acceleration are also non-vanishing. As a test-bed for cosmic censorship, the nature of the future singularity forming at the center is analyzed as an existence problem for o.d.e. at a singular point using techniques based on comparison theorems, and the spectrum of endstates – blackholes or naked singularities – is found in full generality. Consequences of these results on the Cosmic Censorship conjecture are discussed.

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Received: 4 April 2002 / Accepted: 11 November 2002 Published online: 18 February 2003

RID="*"

ID="*" On leave from Departamento de Matemática, Universidade de São Paulo, Brazil

RID="**"

ID="**" Author partially sponsored by CNPq (Brazil), Grant No. \ 200615/01-7.

Communicated by H. Nicolai

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Giambò, R., Giannoni, F., Magli, G. et al. New Solutions of Einstein Equations in Spherical Symmetry: The Cosmic Censor to the Court. Commun. Math. Phys. 235, 545–563 (2003). https://doi.org/10.1007/s00220-003-0793-9

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  • DOI: https://doi.org/10.1007/s00220-003-0793-9

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