Holographic thermal DC response in the hydrodynamic limit
arXiv:1609.08912 · doi:10.1088/1361-6382/aa51df
Abstract
We consider black hole solutions of Einstein gravity that describe deformations of CFTs at finite temperature in which spatial translations have been broken explicitly. We focus on deformations that are periodic in the non-compact spatial directions, which effectively corresponds to considering the CFT on a spatial torus with a non-trivial metric. We apply a DC thermal gradient and show that in a hydrodynamic limit the linearised, local thermal currents can be determined by solving linearised, forced Navier-Stokes equations for an incompressible fluid on the torus. We also show how sub-leading corrections to the thermal current can be calculated as well as showing how the full stress tensor response that is generated by the DC source can be obtained. We also compare our results with the fluid-gravity approach.
35 pages. Very minor typos corrected. Published version
References in corpus (11)
- Nonlinear Fluid Dynamics from Gravity
- Theory of the Nernst effect near quantum phase transitions in condensed matter, and in dyonic black holes
- Universality of the hydrodynamic limit in AdS/CFT and the membrane paradigm
- Momentum dissipation and effective theories of coherent and incoherent transport
- Thermoelectric DC conductivities from black hole horizons
- Conformal Nonlinear Fluid Dynamics from Gravity in Arbitrary Dimensions
- Quantum Critical Transport and the Hall Angle
- The thermoelectric properties of inhomogeneous holographic lattices
- Metal-insulator transition in holography
- Electromagnetic properties of viscous charged fluids
- Conformal field theories in with a helical twist