Some general properties of the renormalized stress-energy tensor for static quantum states on (n+1)-dimensional spherically symmetric black holes

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dc.creatorMorgan, Dean
dc.creatorThom, Stuart
dc.creatorWinstanley, Elizabeth
dc.creatorYoung, Phil M.
dc.date2007-05-08
dc.date2007-06-28
dc.date.accessioned2026-07-07T10:35:47Z
dc.date.available2026-07-07T10:35:47Z
dc.descriptionWe study the renormalized stress-energy tensor (RSET) for static quantum states on (n+1)-dimensional, static, spherically symmetric black holes. By solving the conservation equations, we are able to write the stress-energy tensor in terms of a single unknown function of the radial co-ordinate, plus two arbitrary constants. Conditions for the stress-energy tensor to be regular at event horizons (including the extremal and ``ultra-extremal'' cases) are then derived using generalized Kruskal-like co-ordinates. These results should be useful for future calculations of the RSET for static quantum states on spherically symmetric black hole geometries in any number of space-time dimensions.
dc.description9 pages, no figures, RevTeX4, references added, accepted for publication in General Relativity and Gravitation
dc.identifierhttps://arxiv.org/abs/0705.1131
dc.identifierhttp://arxiv.org/abs/0705.1131
dc.identifierGen.Rel.Grav.39:1719-1734,2007
dc.identifierdoi:10.1007/s10714-007-0486-3
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/179845
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleSome general properties of the renormalized stress-energy tensor for static quantum states on (n+1)-dimensional spherically symmetric black holes
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