Extremal Charged Black Holes with a Twisted Extra Dimension
Takamitsu Tatsuoka, Hideki Ishihara, Masashi Kimura, Ken Matsuno

TL;DR
This paper constructs extremal charged black hole solutions in odd dimensions with a twisted extra dimension, analyzing their horizon structure, curvature properties, and extensions, including cases with a positive cosmological constant.
Contribution
It introduces new extremal charged black hole solutions with a twisted S^1 dimension on Euclidean Taub-NUT spaces, including their horizon and curvature characteristics.
Findings
Existence of null hypersurfaces with vanishing expansion indicating black hole horizons.
Metrics admit C^0 extension across horizons despite curvature divergences.
Solutions with positive cosmological constant are also constructed.
Abstract
We construct odd-dimensional extremal charged black hole solutions with a twisted S^1 as an extra dimension on generalized Euclidean Taub-NUT spaces. There exists a null hypersurface where an expansion for an outgoing null geodesic congruence vanishes, then these spacetimes look like black holes. We show that the metrics admit C^0 extension across the horizon, but some components of Riemann curvature diverge there if the dimension is higher than five. The singularity is not much strong so that an observer along a free-fall geodesic can traverse the horizon. We also show solutions with a positive cosmological constant.
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