Double-extended Kerr-Schild form for $5D$ electrovacuum solutions

Abstract

Five-dimensional Einstein-Maxwell-Chern-Simons equations are investigated in the framework of an extended Kerr-Schild strategy to search for black holes solutions. The fulfillment of Einstein equations constrains the Chern-Simons coupling constant to a value determined by the trace of the energy-momentum tensor of the electromagnetic configuration.

13 pages

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Cited by in corpus (1)

• Revisiting a family of five-dimensional charged, rotating black holes