Double-extended Kerr-Schild form for electrovacuum solutions
arXiv:2109.09497 · doi:10.1007/s10714-022-03013-3
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.
arXiv comment13 pages
References in corpus (21)
- D--branes and Spinning Black Holes
- The General Kerr-de Sitter Metrics in All Dimensions
- General Non-Extremal Rotating Black Holes in Minimal Five-Dimensional Gauged Supergravity
- General Kerr-NUT-AdS Metrics in All Dimensions
- Classification of the Weyl Tensor in Higher Dimensions and Applications
- Survey of Two-Time Physics
- Separability and Killing Tensors in Kerr-Taub-NUT-de Sitter Metrics in Higher Dimensions
- D=5 Einstein-Maxwell-Chern-Simons Black Holes
- Generalized Killing-Yano equations in D=5 gauged supergravity
- Note on Rotating Charged Black Holes in Einstein-Maxwell-Chern-Simons Theory
- Special symmetries of the charged Kerr-AdS black hole of D=5 minimal gauged supergravity
- New improved form of black holes of type D
- Untangling the Newman-Janis algorithm
- An Extended Kerr-Schild Ansatz
- Charged Rotating AdS Black Holes with Chern-Simons coupling
- Remarks on the Myers-Perry and Einstein Gauss-Bonnet Rotating Solutions
- Charged rotating black holes in Einstein--Maxwell--Chern-Simons theory with a negative cosmological constant
- de Sitter Relativity and Quantum Physics
- Extended Kerr-Schild spacetimes: General properties and some explicit examples
- Implications of Kleinian relativity
- Electrovacuum geometries in five dimensions