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CFT description of three-dimensional Kerr-de Sitter space-time
2002 (English)In: Nucl.Phys.B641:376-392Article in journal (Refereed)
Abstract [en]

We describe three-dimensional Kerrde Sitter space using similar methods as recently applied to the BTZ black hole. A rigorous form of the classical connection between gravity in three dimensions and two-dimensional conformal field theory is employed, where the fundamental degrees of freedom are described in terms of two dependent SL(2,C) currents. In contrast to the BTZ case, however, quantization does not give the BekensteinHawking entropy connected to the cosmological horizon of Kerrde Sitter space

Place, publisher, year, edition, pages
2002.
National Category
Physical Sciences
Research subject
Physics
Identifiers
URN: urn:nbn:se:kau:diva-17607OAI: oai:DiVA.org:kau-17607DiVA, id: diva2:591216
Available from: 2013-01-21 Created: 2013-01-21 Last updated: 2013-01-21

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http://dx.doi.org/10.1016/S0550-3213(02)00588-6http://arxiv.org/abs/hep-th/0206113

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Fjelstad, Jens

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