Staticity Theorem for Non-Rotating Black Holes with Non-Minimally Coupled Self-Interacting Scalar Fields

dc.creatorAyón-Beato, Eloy
dc.date1996-06-28
dc.date2001-01-30
dc.date.accessioned2026-07-07T09:02:58Z
dc.date.available2026-07-07T09:02:58Z
dc.descriptionSelf-interacting scalar field configurations which are non-minimally coupled ($ζ\neq0$) to the gravity of a strictly stationary black hole with non-rotating horizon are studied. It is concluded that for analytical configurations the corresponding domain of outer communications is static.
dc.description8 pages, LaTeX; new version to appear in ``Exact Solutions and Scalar Fields in Gravity: Recent Developments,'' eds. A. Macias, J. Cervantes-Cota, and C. Laemmerzahl (Kluwer Academic Publishing)
dc.identifierhttps://arxiv.org/abs/gr-qc/9606081
dc.identifierhttp://arxiv.org/abs/gr-qc/9606081
dc.identifier``Exact Solutions and Scalar Fields in Gravity: Recent Developments,'' edited by A. Macias, J.L. Cervantes-Cota, and C. Laemmerzahl (Kluwer Academic/Plenum Publishers, New York 2001), p. 263.
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/148836
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleStaticity Theorem for Non-Rotating Black Holes with Non-Minimally Coupled Self-Interacting Scalar Fields
dc.typetext

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