An exact rotating black-hole solution in pure Einstein-Maxwell theory admits a cosmological horizon whose radius is set by the electromagnetic field strength alone.
Static hairy black hole in 4D general relativity
2 Pith papers cite this work, alongside 1 external citations. Polarity classification is still indexing.
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2026 2representative citing papers
A new Ricci-flat rotating metric is obtained by demagnetizing the KBR solution, yielding a deformed Kerr geometry with non-flat asymptotics for which black hole thermodynamics is established.
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New Rotating Black Hole in Electromagnetic Fields: Cosmological Horizon without Cosmological Constant
An exact rotating black-hole solution in pure Einstein-Maxwell theory admits a cosmological horizon whose radius is set by the electromagnetic field strength alone.
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Demagnetizing KBR and New Ricci-flat Rotating Metric
A new Ricci-flat rotating metric is obtained by demagnetizing the KBR solution, yielding a deformed Kerr geometry with non-flat asymptotics for which black hole thermodynamics is established.