Essentially all known analytical exact single black hole solutions in four-dimensional Einstein-Maxwell theory belong to the accelerating Kerr-Newman-NUT family placed in backgrounds that are subcases of the conjugated Kerr-Newman-NUT spacetime with arbitrary angular topology.
Charged black hole accelerated by spatially homogeneous electric field of Bertotti- Robinson (AdS2 x S2) space-time
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Einstein-Maxwell solutions satisfying a constant-invariant condition extend to conformally invariant nonlinear electrodynamics via constant rescaling of the electromagnetic field, covering all static cases.
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Black holes in rotating, electromagnetic backgrounds and topological Kerr-Newman-NUT spacetimes
Essentially all known analytical exact single black hole solutions in four-dimensional Einstein-Maxwell theory belong to the accelerating Kerr-Newman-NUT family placed in backgrounds that are subcases of the conjugated Kerr-Newman-NUT spacetime with arbitrary angular topology.
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Einstein-Maxwell fields as solutions of Einstein gravity coupled to conformally invariant non-linear electrodynamics
Einstein-Maxwell solutions satisfying a constant-invariant condition extend to conformally invariant nonlinear electrodynamics via constant rescaling of the electromagnetic field, covering all static cases.