Topology of event horizon in axially symmetric spacetime: Classification of Maxwell set with symmetry

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dc.creatorSiino, Masaru
dc.date2005-05-01
dc.date.accessioned2026-07-07T03:29:41Z
dc.date.available2026-07-07T03:29:41Z
dc.descriptionThe crease set of an event horizon is studied in a spacetime with discrete or continuous symmetry. It determines possible topologies on spatial sections of an event horizon. We thereby investigate the classification of stable topological structure of the crease sets in a spacetime with any symmetry. In practice, we show the classification of the crease set in axially symmetric spacetime. By that we realize the topological structure of axially symmetric event horizons. We will finc that many new topological structures become stable which is not stable without symmetry.
dc.description27pages, 5 figures
dc.identifierhttps://arxiv.org/abs/gr-qc/0505004
dc.identifierhttp://arxiv.org/abs/gr-qc/0505004
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/35274
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleTopology of event horizon in axially symmetric spacetime: Classification of Maxwell set with symmetry
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