The classification of static electro--vacuum space--times containing an asymptotically flat spacelike hypersurface with compact interior

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dc.creatorChrusciel, Piotr T.
dc.creatorTod, Paul
dc.date2005-12-06
dc.date2007-01-29
dc.date.accessioned2026-07-07T10:28:13Z
dc.date.available2026-07-07T10:28:13Z
dc.descriptionWe show that static electro--vacuum black hole space--times containing an asymptotically flat spacelike hypersurface with compact interior and with both degenerate and non--degenerate components of the event horizon do not exist. This is done by a careful study of the near-horizon geometry of degenerate horizons, which allows us to eliminate the last restriction of the static electro-vacuum no-hair theory.
dc.descriptionLatex2e, 14 pages in A4, minor corrections and improvements of the presentation
dc.identifierhttps://arxiv.org/abs/gr-qc/0512043
dc.identifierhttp://arxiv.org/abs/gr-qc/0512043
dc.identifierCommun.Math.Phys.271:577-589,2007
dc.identifierdoi:10.1007/s00220-007-0191-9
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/177373
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleThe classification of static electro--vacuum space--times containing an asymptotically flat spacelike hypersurface with compact interior
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