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Evolution of a Self-interacting Scalar Field in the spacetime of a Higher Dimensional Black Hole
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Evolution of a Self-interacting Scalar Field in the spacetime of a Higher Dimensional Black Hole
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In the spacetime of n-dimensional static charged black hole we examine the mechanism by which the self-interacting scalar hair decay. It is turned out that the intermediate asymptotic behaviour of the self-interacting scalar field is determined by an oscilatory inverse power law. We confirm our results by numerical calculations.
Forward citations
Cited by 2 Pith papers
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