Pair Creation of Black Holes

dc.creatorGauntlett, Jerome P.
dc.date1994-04-13
dc.date.accessioned2026-07-07T04:20:09Z
dc.date.available2026-07-07T04:20:09Z
dc.descriptionThis article is based on a talk given at the IInd International Colloquium on Modern Quantum Field Theory, Bombay 1994. The Ernst solution of dilaton gravity describes charged black holes undergoing uniform accleration in a background magnetic field. By analytically continuing the Ernst solution one obtains instantons that describe the pair production of black holes in the background field. We review various aspects of these solutions paying special attention to the Einstein-Maxwell, low-energy string and $d=5$ Kaluza-Klein theories. It is based on work done in collaboration with {}F. Dowker, S. Giddings, G. Horowitz, D. Kastor and J. Traschen \refs{\DGKT,\DGGH}.
dc.description19 Harvmac l-pages, EFI-94-17
dc.identifierhttps://arxiv.org/abs/hep-th/9404076
dc.identifierhttp://arxiv.org/abs/hep-th/9404076
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/53846
dc.subjectHigh Energy Physics - Theory
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titlePair Creation of Black Holes
dc.typetext

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