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Black Holes and Wormholes in 2+1 Dimensions

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Mathematical and Quantum Aspects of Relativity and Cosmology

Part of the book series: Lecture Notes in Physics ((LNP,volume 537))

Abstract

Vacuum Einstein theory in three spacetime dimensions is locally trivial, but admits many solutions that are globally different, particularly if there is a negative cosmological constant. The classical theory of such locally “anti-de Sitter” spaces is treated in an elementary way, using visualizable models. Among the objects discussed are black holes, spaces with multiple black holes, their horizon structure, closed universes, and the topologies that are possible.

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© 2000 Springer-Verlag Berlin Heidelberg

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Brill, D. (2000). Black Holes and Wormholes in 2+1 Dimensions. In: Cotsakis, S., Gibbons, G.W. (eds) Mathematical and Quantum Aspects of Relativity and Cosmology. Lecture Notes in Physics, vol 537. Springer, Berlin, Heidelberg. https://doi.org/10.1007/3-540-46671-1_6

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  • DOI: https://doi.org/10.1007/3-540-46671-1_6

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  • Publisher Name: Springer, Berlin, Heidelberg

  • Print ISBN: 978-3-540-66865-7

  • Online ISBN: 978-3-540-46671-0

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