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      Viscosity Bound Violation in Higher Derivative Gravity

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          Abstract

          Motivated by the vast string landscape, we consider the shear viscosity to entropy density ratio in conformal field theories dual to Einstein gravity with curvature square corrections. After field redefinitions these theories reduce to Gauss-Bonnet gravity, which has special properties that allow us to compute the shear viscosity nonperturbatively in the Gauss-Bonnet coupling. By tuning of the coupling, the value of the shear viscosity to entropy density ratio can be adjusted to any positive value from infinity down to zero, thus violating the conjectured viscosity bound. At linear order in the coupling, we also check consistency of four different methods to calculate the shear viscosity, and we find that all of them agree. We search for possible pathologies associated with this class of theories violating the viscosity bound.

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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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            String-generated gravity models.

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              Shear viscosity of strongly coupled N=4 supersymmetric Yang-Mills plasma

              , , (2010)
              Using the anti-de Sitter/conformal field theory correspondence, we relate the shear viscosity \eta of the finite-temperature N=4 supersymmetric Yang-Mills theory in the large N, strong-coupling regime with the absorption cross section of low-energy gravitons by a near-extremal black three-brane. We show that in the limit of zero frequency this cross section coincides with the area of the horizon. From this result we find \eta=\pi/8 N^2T^3. We conjecture that for finite 't Hooft coupling (g_YM)^2N the shear viscosity is \eta=f((g_YM)^2N) N^2T^3, where f(x) is a monotonic function that decreases from O(x^{-2}\ln^{-1}(1/x)) at small x to \pi/8 when x\to\infty.
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                Author and article information

                Journal
                05 December 2007
                2008-06-13
                Article
                10.1103/PhysRevD.77.126006
                0712.0805
                dd75c612-7339-4593-a5cb-475c13873e09

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

                History
                Custom metadata
                CAS-KITPC/ITP-025, MIT-CTP-3918, SU-ITP-07/22
                Phys.Rev.D77:126006,2008
                23 pages, 2 figures; v2: typos corrected, references added, notes added; v3: subsections IV.C and IV.D eliminated, comments on the null energy condition eliminated, minor revisions made
                hep-th gr-qc hep-ph

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