Evolution of a Self-interacting Scalar Field in the spacetime of a Higher Dimensional Black Hole

Physics – High Energy Physics – High Energy Physics - Theory

Scientific paper

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RevTex, 6 pages, 8 figures, to be published in Phys.Rev.D15

Scientific paper

10.1103/PhysRevD.72.044027

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.

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