Post-Newtonian expansion of a rigidly rotating disc of dust with a constant specific charge

DOI10.1088/0264-9381/30/8/085010zbMath1267.83019arXiv1301.5232OpenAlexW2065903471MaRDI QIDQ4923877

Stefan Palenta, Reinhard Meinel

Publication date: 27 May 2013

Published in: Classical and Quantum Gravity (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/1301.5232

zbMATH Keywords

Einstein-Maxwell equationspost-Newtonian expansionextreme Kerr-Newman black hole

Mathematics Subject Classification ID

Black holes (83C57) Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Exact solutions to problems in general relativity and gravitational theory (83C15) Approximation procedures, weak fields in general relativity and gravitational theory (83C25) Einstein-Maxwell equations (83C22)

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Geometry of charged rotating discs of dust in Einstein-Maxwell theory

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