Construction of a Penrose Diagram for a Spatially Coherent Evaporating Black Hole

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dc.creatorBrown, Beth A.
dc.creatorLindesay, James
dc.date2007-10-10
dc.date.accessioned2026-07-07T11:37:58Z
dc.date.available2026-07-07T11:37:58Z
dc.descriptionA Penrose diagram is constructed for an example black hole that evaporates at a steady rate as measured by a distant observer, until the mass vanishes, yielding a final state Minkowski space-time. Coordinate dependencies of significant features, such as the horizon and coordinate anomalies, are clearly demonstrated on the diagram. The large-scale causal structure of the space-time is briefly discussed.
dc.description12 pages, 3 figures
dc.identifierhttps://arxiv.org/abs/0710.2032
dc.identifierhttp://arxiv.org/abs/0710.2032
dc.identifierClass.Quant.Grav.25:105026,2008
dc.identifierdoi:10.1088/0264-9381/25/10/105026
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/199398
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleConstruction of a Penrose Diagram for a Spatially Coherent Evaporating Black Hole
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