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      Universality of the hydrodynamic limit in AdS/CFT and the membrane paradigm

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          Abstract

          We show that at the level of linear response the low frequency limit of a strongly coupled field theory at finite temperature is determined by the horizon geometry of its gravity dual, i.e. by the "membrane paradigm" fluid of classical black hole mechanics. Thus generic boundary theory transport coefficients can be expressed in terms of geometric quantities evaluated at the horizon. When applied to the stress tensor this gives a simple, general proof of the universality of the shear viscosity in terms of the universality of gravitational couplings, and when applied to a conserved current it gives a new general formula for the conductivity. Away from the low frequency limit the behavior of the boundary theory fluid is no longer fully captured by the horizon fluid even within the derivative expansion; instead we find a nontrivial evolution from the horizon to the boundary. We derive flow equations governing this evolution and apply them to the simple examples of charge and momentum diffusion.

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          Viscosity in Strongly Interacting Quantum Field Theories from Black Hole Physics

          The ratio of shear viscosity to volume density of entropy can be used to characterize how close a given fluid is to being perfect. Using string theory methods, we show that this ratio is equal to a universal value of \(\hbar/4\pi k_B\) for a large class of strongly interacting quantum field theories whose dual description involves black holes in anti--de Sitter space. We provide evidence that this value may serve as a lower bound for a wide class of systems, thus suggesting that black hole horizons are dual to the most ideal fluids.
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            Membrane viewpoint on black holes: Properties and evolution of the stretched horizon

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              Universality of the shear viscosity in supergravity

              Kovtun, Son and Starinets proposed a bound on the shear viscosity of any fluid in terms of its entropy density. We argue that this bound is always saturated for gauge theories at large 't Hooft coupling, which admit holographically dual supergravity description.
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                Author and article information

                Journal
                23 September 2008
                2008-12-17
                Article
                10.1103/PhysRevD.79.025023
                0809.3808
                5dbbd29d-ccab-48e0-bbb7-34eff792ee7a

                http://arxiv.org/licenses/nonexclusive-distrib/1.0/

                History
                Custom metadata
                MIT-CTP-3983
                Phys.Rev.D79:025023,2009
                15 pages; added references, minor clarifications in text
                hep-th gr-qc

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