magnetized static, balanced black holes with event horizon topology
arXiv:1303.2190 · doi:10.1016/j.physletb.2013.04.053
Abstract
We construct static, nonextremal black hole solutions of the Einstein-Maxwell equations in spacetime dimensions, with an event horizon of topology. These configurations are asymptotically flat, the U(1) field being purely magnetic, with a spherical distribution of monopole charges but no net charge measured at infinity. They can be viewed as generalizations of the static dipole black ring, sharing its basic properties, in particular the presence of a conical singularity. The magnetized version of these solutions is constructed by applying a Harrison transformation, which puts them into an external magnetic field. For , balanced configurations approaching asymptotically a Melvin universe background are found for a critical value of the background magnetic field.
12 pages, 2 figures
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