Rotating spacetimes with a cosmological constant
Christos Charmousis, David Langlois, Daniele Steer, Robin Zegers

TL;DR
This paper develops solution-generating techniques for higher-dimensional rotating spacetimes with a cosmological constant, extending classical methods and providing new explicit solutions like deformations of AdS black holes.
Contribution
It generalizes solution-generating methods to arbitrary dimensions with a cosmological constant and constructs new solutions from four-dimensional seeds.
Findings
Decoupling of field equations in higher dimensions for zero cosmological constant
Extension of Ernst and Papapetrou methods to higher dimensions with cosmological constant
Explicit solutions including deformations of AdS soliton and black hole
Abstract
We develop solution-generating techniques for stationary metrics with one angular momentum and axial symmetry, in the presence of a cosmological constant and in arbitrary spacetime dimension. In parallel we study the related lower dimensional Einstein-Maxwell-dilaton static spacetimes with a Liouville potential. For vanishing cosmological constant, we show that the field equations in more than four dimensions decouple into a four dimensional Papapetrou system and a Weyl system. We also show that given any four dimensional 'seed' solution, one can construct an infinity of higher dimensional solutions parametrised by the Weyl potentials, associated to the extra dimensions. When the cosmological constant is non-zero, we discuss the symmetries of the field equations, and then extend the well known works of Papapetrou and Ernst (concerning the complex Ernst equation) in four-dimensional…
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