Evolution of a Self-interacting Scalar Field in the spacetime of a Higher Dimensional Black Hole
arXiv:hep-th/0508175 · doi:10.1103/PhysRevD.72.044027
Abstract
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.
RevTex, 6 pages, 8 figures, to be published in Phys.Rev.D15