Reissner-Nordstrom Black Holes and Thick Domain Walls
arXiv:gr-qc/0401031 · doi:10.1103/PhysRevD.69.084018
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.
arXiv comment18 pages, 10 figures, accepted for Phys. Rev. D
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