Structure of the Cauchy horizon singularity

dc.creatorBurko, Lior M.
dc.date1997-10-08
dc.date.accessioned2026-07-07T03:31:50Z
dc.date.available2026-07-07T03:31:50Z
dc.descriptionWe study the Cauchy horizon (CH) singularity of a spherical charged black hole perturbed nonlinearly by a self-gravitating massless scalar field. We show numerically that the singularity is weak both at the early and at the late sections of the CH, where the focusing of the area coordinate $r$ is strong. In the early section the metric perturbations vanish, and the fields behave according to perturbation analysis. We find exact analytical expressions for the gradients of $r$ and of the scalar field, which are valid at both sections. We then verify these analytical results numerically.
dc.description4 pages. Talk presented at the Eighth Marcel Grossmann Meeting, June 22 - June 27, 1997, Jerusalem, Israel
dc.identifierhttps://arxiv.org/abs/gr-qc/9710044
dc.identifierhttp://arxiv.org/abs/gr-qc/9710044
dc.identifierin The Eighth Marcel Grossmann Meeting, Volume I, edited by Tsvi Piran (World Scientific, Singapore, 1999), p.p. 673-675
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/36006
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleStructure of the Cauchy horizon singularity
dc.typetext

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