The conformal-to-Carter metric is the unique ansatz for the stated geometric conditions, and in Einstein-Maxwell theory the only non-trivial solutions are the Ovcharenko-Podolsky class for fully non-aligned non-null EM fields and the Plebański-Demiański class for double-aligned non-null EM fields.
Wang, Innermost stable circular orbit of Kerr–Bertotti–Robinson black holes and inspirals from it: Exact solutions, arXiv e-prints (2025), arXiv:2508.04684 [gr-qc]
2 Pith papers cite this work. Polarity classification is still indexing.
2
Pith papers citing it
citation-role summary
method 1
citation-polarity summary
years
2026 2verdicts
UNVERDICTED 2roles
method 1polarities
use method 1representative citing papers
Kerr-BR black hole images with magnetically coupled synchrotron emissivity show spin- and B-dependent shifts in the inner disk edge, altered lensing rings, and Doppler asymmetries, with retrograde cases displaying wider central depletion.
citing papers explorer
-
Uniqueness of stationary axisymmetric type D black holes with non-aligned electromagnetic field
The conformal-to-Carter metric is the unique ansatz for the stated geometric conditions, and in Einstein-Maxwell theory the only non-trivial solutions are the Ovcharenko-Podolsky class for fully non-aligned non-null EM fields and the Plebański-Demiański class for double-aligned non-null EM fields.
-
Optical Appearance of the Kerr-Bertotti-Robinson Black Hole with a Magnetically Driven Synchrotron Emissivity Model
Kerr-BR black hole images with magnetically coupled synchrotron emissivity show spin- and B-dependent shifts in the inner disk edge, altered lensing rings, and Doppler asymmetries, with retrograde cases displaying wider central depletion.