2015/08/31 by Elias Kiritsis, Yoshinori Matsuo · 1 citation
Physics and Astronomy · #hep-th #hep-ph
paper · pdf · doi:10.1007/jhep12(2015)076
44 pages, v2: minor improvements and a list of definitions added, 48 pages, v3: Published version, many minor misprints corrected, 57 pages
arxiv created 2017/09/13 · arxiv updated 2017/09/14
Non-equilibrium black hole horizons are considered in scaling theories with generic Lifshitz invariance and an unbroken U(1) symmetry. There is also charge-hyperscaling violation associated with a non-trivial conduction exponent. The boundary stress tensor is computed and renormalized and the associated hydrodynamic equations derived. Upon a non-trivial redefinition of boundary sources associated with the U(1) gauge field, the equations are mapped to the standard non-relativistic hydrodynamics equations coupled to a mass current and an external Newton potential in accordance with the general theory of [arXiv:1502.00228]. The shear viscosity to entropy ratio is the same as in the relativistic case.