Accelerating Black Holes and Spinning Spindles
arXiv:2012.08530 · doi:10.1103/PhysRevD.104.046007
Abstract
We study solutions in the Plebański--Demiański family which describe an accelerating, rotating and dyonically charged black hole in . These are solutions of Einstein-Maxwell theory with a negative cosmological constant and hence minimal gauged supergravity. It is well known that when the acceleration is non-vanishing the black hole metrics have conical singularities. By uplifting the solutions to supergravity using a regular Sasaki-Einstein -manifold, , we show how the free parameters can be chosen to eliminate the conical singularities. Topologically, the solutions incorporate an fibration over a two-dimensional weighted projective space, , also known as a spindle, which is labelled by two integers that determine the conical singularities of the metrics. We also discuss the supersymmetric and extremal limit and show that the near horizon limit gives rise to a new family of regular supersymmetric solutions of supergravity, which generalise a known family by the addition of a rotation parameter. We calculate the entropy of these black holes and argue that it should be possible to derive this from certain , quiver gauge theories compactified on a spinning spindle with appropriate magnetic flux.
arXiv comment76 pages, 8 figures; v2: very minor changes, published version
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