Constraints on Black Holes in Classical and Semiclassical Theories of Gravity

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dc.creatorAnderson, Paul R.
dc.creatorMull, Courtney D.
dc.date1997-07-11
dc.date.accessioned2026-07-07T03:31:42Z
dc.date.available2026-07-07T03:31:42Z
dc.descriptionConstraints on the geometry of a static spherically symmetric black hole are obtained by requiring the spacetime curvature to be analytic at the event horizon. For a zero temperature black hole further constraints are obtained by also requiring that the semiclassical trace equation be satisfied when conformally invariant fields are present. It is found that zero temperature black holes whose sizes lie within a certain range do not exist. The range depends on the numbers and types of conformally invariant quantized fields that are present.
dc.description7 pages, ReVTeX
dc.identifierhttps://arxiv.org/abs/gr-qc/9707026
dc.identifierhttp://arxiv.org/abs/gr-qc/9707026
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/35953
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleConstraints on Black Holes in Classical and Semiclassical Theories of Gravity
dc.typetext

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