Abstract:
We present the metric of a Schwarzschild (S) black hole coupled to an external,
stationary electromagnetic Bertotti–Robinson (BR) solution. This metric generalizes a previous
metric that served to unify the S and BR solutions. Limiting cases of our metric include the case
of a stationary electromagnetic universe in which conformal curvature arises due to rotation.
Description:
Due to copyright restrictions, the access to the publisher version (published version) of this article is only available via subscription. You may click URI (with DOI: 10.1088/0264-9381/12/12/017) and have access to the Publisher Version of this article through the publisher web site or online databases, if your Library or institution has subscription to the related journal or publication.