Conformal Nonlinear Fluid Dynamics from Gravity in Arbitrary Dimensions
Sayantani Bhattacharyya, R. Loganayagam, Ipsita Mandal, Shiraz Minwalla, Ankit Sharma
TL;DR
This work establishes a comprehensive map between conformal fluid dynamics in d dimensions and long-wavelength, asymptotically AdS_{d+1} gravity. By employing a Weyl-covariant derivative framework and a derivative expansion, the authors construct explicit bulk metrics and boundary stress tensors accurate to second order, valid on curved boundaries, and confirm consistency with exact AdS Kerr black holes. They derive a covariant entropy current from the bulk horizon, proving a local second-law-like monotonicity, and demonstrate that AdS Kerr solutions naturally fit the fluid-dynamical description. The results reveal universal structures in the second-order transport data and provide a robust platform for exploring holographic hydrodynamics in arbitrary dimensions, with potential extensions to charged or non-conformal setups.
Abstract
We generalize recent work to construct a map from the conformal Navier Stokes equations with holographically determined transport coefficients, in d spacetime dimensions, to the set of asymptotically locally AdS_{d+1} long wavelength solutions of Einstein's equations with a negative cosmological constant, for all d>2. We find simple explicit expressions for the stress tensor (slightly generalizing the recent result by Haack and Yarom (arXiv:0806.4602)), the full dual bulk metric and an entropy current of this strongly coupled conformal fluid, to second order in the derivative expansion, for arbitrary d>2. We also rewrite the well known exact solutions for rotating black holes in AdS_{d+1} space in a manifestly fluid dynamical form, generalizing earlier work in d=4. To second order in the derivative expansion, this metric agrees with our general construction of the metric dual to fluid flows.
