A Cosmological No-Hair Theorem

Abstract

A generalisation of Price's theorem is given for application to Inflationary Cosmologies. Namely, we show that on a Schwarzschild--de Sitter background there are no static solutions to the wave or gravitational perturbation equations for modes with angular momentum greater than their intrinsic spin.

9 pages, NCL94 -TP4, (Revtex)

References in corpus (2)

• Cosmological Multi-Black Hole Solutions
• Testing Cosmic Censorship with Black Hole Collisions

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