Thick brane solutions and topology change transition on black hole backgrounds

Details Thick brane solutions and topology change transition on black hole backgrounds Thick brane solutions and topology change transition on black hole backgrounds

2010-06-23

arxiv.org/abs/1006.4424v1

Phys. Rev. D 82, 024035 (2010)

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

11 pages, 10 figures, accepted for publication in Phys. Rev. D

Scientific paper

10.1103/PhysRevD.82.024035

We consider static, axisymmetric, thick brane solutions on higher dimensional, spherically symmetric black hole backgrounds. It was found recently [1], that in cases when the thick brane has more than 2 spacelike dimensions, perturbative approaches break down around the corresponding thin solutions for Minkowski type topologies. This behavior is a consequence of the fact that thin solutions are not smooth at the axis, and for a general discussion of possible phase transitions in the system, one needs to use a non-perturbative approach. In the present paper we provide an exact, numerical solution of the problem both for black hole- and Minkowski type topologies with arbitrary number of brane and bulk dimensions. We also illustrate a topology change transition in the system for a 5-dimensional brane embedded in a 6-dimensional bulk.

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