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Viscosity in Strongly Interacting Quantum Field Theories from Black Hole Physics

Pavel KovtunKavli Institute for Theoretical Physics, University of California, Santa Barbara, CA 93106, USAD. SonInstitute for Nuclear Theory, University of Washington, Seattle, Washington 98195-1550, USAAndrei O. StarinetsPerimeter Institute for Theoretical Physics, Waterloo, Ontario N2L 2Y5, Canada
2005en
ABI

Аннотация

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 variant Planck's over 2pi/4pik(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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