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arXiv · 1512.04970

Geroch group for Einstein spaces and holographic integrability

Anastasios C. Petkou·P. Marios Petropoulos·Konstantinos Siampos
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Abstract

We review how Geroch's reduction method is extended from Ricci-flat to Einstein spacetimes. The Ehlers-Geroch SL(2,R) group is still present in the three-dimensional sigma-model that captures the dynamics, but only a subgroup of it is solution-generating. Holography provides an alternative three-dimensional perspective to integrability properties of Einstein's equations in asymptotically anti-de Sitter spacetimes. These properties emerge as conditions on the boundary data (metric and energy-momentum tensor) ensuring that the hydrodynamic derivative expansion be resummed into an exact four-dimensional Einstein geometry. The conditions at hand are invariant under a set of transformations dubbed holographic U-duality group. The latter fills the gap left by the Ehlers-Geroch group in Einstein spaces, and allows for solution-generating maps mixing e.g. the mass and the nut charge.

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Anastasios C. Petkou, P. Marios Petropoulos, Konstantinos Siampos. 2015-12-15. Geroch group for Einstein spaces and holographic integrability. https://arxiv.org/abs/1512.04970

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