Dilatonic Black Holes Time Stability

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dc.creatorKhovanskaya, O.
dc.date2002-01-23
dc.date.accessioned2026-07-07T03:26:37Z
dc.date.available2026-07-07T03:26:37Z
dc.descriptionThe stability under small time perturbations of the dilatonic black hole solution near the determinant curvature singularity is proved. This fact gives the additional arguments that the investigated topological configuration can realise in nature. In the frames of this model primordial black hole remnants are examined as time stable objects, which can form an significant part of a dark matter in the Universe.
dc.descriptionLaTeX, 4 pages, uses gc-99.sty, submitted to Grav. & Cosmol
dc.identifierhttps://arxiv.org/abs/gr-qc/0201075
dc.identifierhttp://arxiv.org/abs/gr-qc/0201075
dc.identifierGrav.Cosmol. 8 (2002) 197-200
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/34112
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleDilatonic Black Holes Time Stability
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