2015
DOI: 10.1007/jhep10(2015)103
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Thermoelectric DC conductivities and Stokes flows on black hole horizons

Abstract: We consider a general class of electrically charged black holes of EinsteinMaxwell-scalar theory that are holographically dual to conformal field theories at finite charge density which break translation invariance explicitly. We examine the linearised perturbations about the solutions that are associated with the thermoelectric DC conductivity. We show that there is a decoupled sector at the black hole horizon which must solve generalised Stokes equations for a charged fluid. By solving these equations we can… Show more

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Cited by 80 publications
(263 citation statements)
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References 64 publications
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“…to all orders in our derivative expansion. 14 These observations are deeply connected to a beautiful recent paper by Donos and Gauntlett [34] (similar ideas have been developed in [35,48,49].). There it was shown that the DC conductivity of quite general holographic models can be understood from solving the forced Navier-Stokes equations for a fluid living on the black hole horizon.…”
Section: Jhep10(2015)078supporting
confidence: 64%
See 1 more Smart Citation
“…to all orders in our derivative expansion. 14 These observations are deeply connected to a beautiful recent paper by Donos and Gauntlett [34] (similar ideas have been developed in [35,48,49].). There it was shown that the DC conductivity of quite general holographic models can be understood from solving the forced Navier-Stokes equations for a fluid living on the black hole horizon.…”
Section: Jhep10(2015)078supporting
confidence: 64%
“…The DC constitutive relations that we have derived (4.7) for the boundary quantum field theory are, for our model, just the same as the exact constitutive relation of the horizon fluid in 15 [34,35]. Similarly, our expression for the fluid velocity, (4.9), is identical to that obtained by solving the Navier-Stokes equation on the horizon.…”
Section: Jhep10(2015)078supporting
confidence: 53%
“…While all of these dc conductivities are large, κ ij dc and also κ in (3.44) are parametrically smaller as pointed out in [31,34]. Thus, from (3.46) we deduce that one of the frequencies will be proportional to L −1 while the other will be parametrically smaller.…”
Section: ð3:46þmentioning
confidence: 68%
“…In particular, it should be possible to obtain the Einstein relations in terms of the dc conductivities and the thermodynamic susceptibilities. It is now understood how, in general, the thermoelectric dc conductivity of the boundary field theory, when finite, can be obtained in terms of data on the black hole horizon [32,34,37]. Thus, providing one can obtain the susceptibilities in terms of horizon data, one should also be able to extract the Einstein relations.…”
Section: Final Commentsmentioning
confidence: 99%
“…Interestingly, though, even for generic ('non-Q') lattices which break translational symmetry in all the spatial dimensions the conductivity can be obtained by solving some linearized, time-independent, and forced Navier-Stokes-type equations of an effective (charged and incompressible) fluid living on the horizon [186][187][188][189], thus extending the 'membrane paradigm' along the lines of the general concept of a fluid-gravity correspondence [190][191][192][193]. The latter allows for a dual description of the bulk gravity theory in terms of the hydrodynamics of a certain boundary fluid whose stress-energy tensor acts as a source for the boundary metric.…”
Section: From Ads/cmt To Holographic Transportmentioning
confidence: 99%