A Simplified Mathematical Model for the Formation of Null Singularities Inside Black Holes II

dc.creatorGorbonos, Dan
dc.creatorWolansky, Gershon
dc.date2006-12-27
dc.date.accessioned2026-07-07T11:21:39Z
dc.date.available2026-07-07T11:21:39Z
dc.descriptionWe study a simple system of two hyperbolic semi-linear equations, inspired by the Einstein equations. The system, which was introduced in gr-qc/0612136, is a model for singularity formation inside black holes. We show for a particular case of the equations that the system demonstrates a finite time blowup. The singularity that is formed is a null singularity. Then we show that in this particular case the singularity has features that are analogous to known features of models of black-hole interiors - which describe the inner-horizon instability. Our simple system may provide insight into the formation of null singularities inside spinning or charged black holes.
dc.description25 pages, 10 figures
dc.identifierhttps://arxiv.org/abs/gr-qc/0612173
dc.identifierhttp://arxiv.org/abs/gr-qc/0612173
dc.identifierJ.Math.Phys.48:092503,2007
dc.identifierdoi:10.1063/1.2779949
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/194323
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleA Simplified Mathematical Model for the Formation of Null Singularities Inside Black Holes II
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