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Kinematic Dynamos in the Kerr Metric
Authors:Núñez  M
Institution:(1) Departamento de Análisis Matemático, Universidad de Valladolid, Spain.
Abstract:It is known that a sharp decrease in the angular velocity of the accretion disk around a black hole could in principle produce a kinematic axisymmetric dynamo, in contrast to the classical situation described by Cowling's antidynamo theorem. Here the effect of a nontrivial poloidal velocity of the disk is studied, showing that a strong gradient of this velocity enhances the possibilities of a working dynamo.
Keywords:Black hole  Accretion disk  Axisymmetry
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