Reissner-Nordstrom Black Holes and Thick Domain Walls
General Relativity and Quantum Cosmology
2009-11-10 v1
Abstract
We solve numerically equations of motion for real self-interacting scalar fields in the background of Reissner-Nordstrom black hole and obtained a sequence of static axisymmetric solutions representing thick domain walls charged black hole systems. In the case of extremal Reissner-Nordstrom black hole solution we find that there is a parameter depending on the black hole mass and the width of the domain wall which constitutes the upper limit for the expulsion to occur.
Cite
@article{arxiv.gr-qc/0401031,
title = {Reissner-Nordstrom Black Holes and Thick Domain Walls},
author = {R. Moderski and M. Rogatko},
journal= {arXiv preprint arXiv:gr-qc/0401031},
year = {2009}
}
Comments
18 pages, 10 figures, accepted for Phys. Rev. D