Holographic fluid from nonminimally coupled scalar-tensor theory of gravity
arXiv:1401.6487 · doi:10.1088/0264-9381/31/10/105018
Abstract
We establish the gravity/fluid correspondence in the nonminimally coupled scalar-tensor theory of gravity. Imposing Petrov-like boundary conditions over the gravitational field, we find that, for a certain class of background metrics, the boundary fluctuations obey the standard Navier-Stokes equation for an incompressible fluid without any external force term in the leading order approximation under the near horizon expansion. That is to say, the scalar field fluctuations does not contribute in the leading order approximation regardless of what kind of boundary condition we impose on it.
10 pages, submitted to CQG
References in corpus (10)
- Building an AdS/CFT superconductor
- Nonlinear Fluid Dynamics from Gravity
- Non-Relativistic Fluid Dual to Asymptotically AdS Gravity at Finite Cutoff Surface
- Thermodynamical properties of hairy black holes in n spacetimes dimensions
- From Petrov-Einstein to Navier-Stokes
- Magnetohydrodynamics from gravity
- Incompressible Navier-Stokes Equations from Einstein Gravity with Chern-Simons Term
- Holographic charged fluid dual to third order Lovelock gravity
- Higher Curvature Gravity and the Holographic fluid dual to flat spacetime
- Petrov type I Spacetime and Dual Relativistic Fluids
Cited by in corpus (7)
- Petrov type I Spacetime and Dual Relativistic Fluids
- Three dimensional rotating hairy black holes, asymptotics and thermodynamics
- Flat space compressible fluid as holographic dual of black hole with curved horizon
- Compressible forced viscous fluid from product Einstein manifolds
- Fluids and vortex from constrained fluctuations around C-metric black hole
- Time evolving fluid from Vaidya spacetime
- Fluid/Gravity Correspondence with Scalar Field and Electromagnetic Field