arXiv · 1301.5232
Post-Newtonian expansion of a rigidly rotating disc of dust with a constant specific charge
Abstract
We present an algorithm for obtaining the post-Newtonian expansion of the asymptotically flat solution to the Einstein-Maxwell equations describing a rigidly rotating disc of dust with a constant specific charge. Explicit analytic expressions are calculated up to the eighth order. The results are used for a physical discussion of the extreme relativistic limiting cases. We identify strong evidence for a transition to an extreme Kerr-Newman black hole.
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Stefan Palenta, Reinhard Meinel. 2013-01-22. Post-Newtonian expansion of a rigidly rotating disc of dust with a constant specific charge. https://doi.org/10.1088/0264-9381/30/8/085010
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