No static bubbling spacetimes in higher dimensional Einstein-Maxwell theory
Hari K. Kunduri, James Lucietti

TL;DR
This paper proves that in higher-dimensional Einstein-Maxwell theory, static asymptotically flat spacetimes cannot have magnetic fields, leading to a complete classification of static black holes and ruling out non-trivial topologies.
Contribution
It establishes the non-existence of static magnetic solutions and static solitons in higher-dimensional Einstein-Maxwell theory, completing the classification of static black holes.
Findings
No static magnetic or soliton solutions exist in the theory.
Static non-extremal black holes are fully classified.
Asymptotically flat static spacetimes with non-trivial topology are absent.
Abstract
We prove that any asymptotically flat static spacetime in higher dimensional Einstein-Maxwell theory must have no magnetic field. This implies that there are no static soliton spacetimes and completes the classification of static non-extremal black holes in this theory. In particular, these results establish that there are no asymptotically flat static spacetimes with non-trivial topology, with or without a black hole, in Einstein-Maxwell theory.
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