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Holographic perfect fluidity, Cotton energy-momentum duality and transport properties

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TLDR
In this paper, the authors investigated background metrics for 2 + 1-dimensional holographic theories where the equilibrium solution behaves as a perfect fluid, and admits thus a thermodynamic description.
Abstract
We investigate background metrics for 2 + 1-dimensional holographic theories where the equilibrium solution behaves as a perfect fluid, and admits thus a thermodynamic description. We introduce stationary perfect-Cotton geometries, where the Cotton-York tensor takes the form of the energy-momentum tensor of a perfect fluid, i.e. they are of Petrov type Dt. Fluids in equilibrium in such boundary geometries have non-trivial vorticity. The corresponding bulk can be exactly reconstructed to obtain 3 + 1-dimensional stationary black-hole solutions with no naked singularities for appropriate values of the black-hole mass. It follows that an infinite number of transport coefficients vanish for holographic fluids. Our results imply an intimate relationship between black-hole uniqueness and holographic perfect equilibrium. They also point towards a Cotton/energy-momentum tensor duality constraining the fluid vorticity, as an intriguing boundary manifestation of the bulk mass/nut duality.

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Exact Space-Times in Einstein's General Relativity

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Holographic Thermodynamics of Accelerating Black Holes

TL;DR: In this paper, the dual energy-momentum tensor can be written as a three-dimensional perfect fluid plus a nonhydrodynamic contribution with a universal coefficient which is given in gauge theory variables.
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Flat holography and Carrollian fluids

TL;DR: In this paper, it was shown that a holographic description of four-dimensional asymptotically locally flat spacetimes is reached smoothly from the zero-cosmological-constant limit of anti-de Sitter holography.
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Supersymmetry of topological Kerr-Newman-Taub-NUT-aDS spacetimes

TL;DR: In this article, the topological Kerr-Newman-adS solutions were extended with NUT charge and generalizations of the Robinson-Bertotti solution to the negative cosmological constant case with different topologies.
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Flat holography and Carrollian fluids

TL;DR: In this article, it was shown that a holographic description of four-dimensional asymptotically locally flat spacetimes is reached smoothly from the zero-cosmological-constant limit of anti-de Sitter holography.
References
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Three-dimensional massive gauge theories

TL;DR: In this article, the authors analyzed three-dimensional Yang-Mills and gravity theories augmented by gauge-invariant mass terms and quantized a dimensionless mass-couplingconstant ratio.
Journal ArticleDOI

Topologically Massive Gauge Theories

TL;DR: In this article, the authors studied the effects of topological properties on the masses of the gauge fields in three-dimensional space-time, where novel, gauge invariant, P and T odd terms of topology origin give rise to masses for the gauge field.
Journal ArticleDOI

Rotating, charged, and uniformly accelerating mass in general relativity

TL;DR: In this paper, a new general class of solutions of the Einstein-Maxwell equations is presented, which is based on seven arbitrary parameters that group in a natural way into three complex parameters m + in, a + ib, e + ig, and the cosmological constant λ.
Journal ArticleDOI

Rotation and the AdS / CFT correspondence

TL;DR: In this paper, the authors examined the relationship between conformal field theory in rotating Einstein universes of dimensions two to four and Kerr-anti-de Sitter black holes in dimensions three to five.
Book

Exact Space-Times in Einstein's General Relativity

TL;DR: In this paper, the authors introduce the concept of space-time related to Schwarzchild and Taub-NUT space-times, and provide solutions for uniformly accelerating particles in the plane and pp-wave domain.
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