Stability of black holes in de Sitter space

Details Stability of black holes in de Sitter space Stability of black holes in de Sitter space

Jan 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990phrvd..41..403m&link_type=abstract

Physical Review D (Particles and Fields), Volume 41, Issue 2, 15 January 1990, pp.403-409

Mathematics

Logic

57

Scientific paper

The theory of black-hole perturbations is extended to charged black holes in de Sitter space. These spacetimes have wormholes connecting different asymptotic regions. It appears that, at least in some cases, these holes are stable even at the Cauchy horizon. It follows that they violate cosmic censorship and an observer could in principle travel through the black hole to another universe. The stability of these spacetimes also implies the existence of a cosmological ``no hair'' theorem.

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