Extra Dimensions, Nonminimal Couplings, Horizons and Wormholes

dc.creatorBronnikov, Kirill A.
dc.date1997-03-07
dc.date.accessioned2026-07-07T03:31:31Z
dc.date.available2026-07-07T03:31:31Z
dc.descriptionStatic, spherically symmetric configurations of gravity with nonminimally coupled scalar fields are considered in D-dimensional space-times in the framework of generalized scalar-tensor theories. We seek special cases when the system has no naked singularity but instead forms either a black hole, or a wormhole. General conditions when this is possible are formulated. In particlar, some such special cases are indicated for multidimensional Brans-Dicke theory and for linear, massless, nonminimally coupled scalar fields. It is shown that in the Brans-Dicke theory the only black-hole solution corresponds to D=4 and the coupling constant ω< -2, and there is a wormhole solution for ω=0. For linear scalar fields it is shown that the only black-hole solution is the well-known one (D=4, a black hole with scalar charge), while the known 4-dimensional wormhole solution is generalized to systems with conformal coupling in arbitrary dimension.
dc.description6 pages, Latex
dc.identifierhttps://arxiv.org/abs/gr-qc/9703020
dc.identifierhttp://arxiv.org/abs/gr-qc/9703020
dc.identifierGrav.Cosmol. 2 (1996) 221-226
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/35890
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleExtra Dimensions, Nonminimal Couplings, Horizons and Wormholes
dc.typetext

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