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Reissner-Nordstrom Black Holes and Thick Domain Walls

R. Moderski·M. Rogatko
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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.

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BibTeXRIS

R. Moderski, M. Rogatko. 2004-01-09. Reissner-Nordstrom Black Holes and Thick Domain Walls. https://doi.org/10.1103/physrevd.69.084018

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