pith. machine review for the scientific record. sign in

arxiv: 0712.2456 · v4 · submitted 2007-12-14 · ✦ hep-th · gr-qc· nucl-th

Recognition: unknown

Nonlinear Fluid Dynamics from Gravity

Authors on Pith no claims yet
classification ✦ hep-th gr-qcnucl-th
keywords boundaryfluiddynamicsequationsexpansionads5arbitraryderivative
0
0 comments X
read the original abstract

Black branes in AdS5 appear in a four parameter family labeled by their velocity and temperature. Promoting these parameters to Goldstone modes or collective coordinate fields -- arbitrary functions of the coordinates on the boundary of AdS5 -- we use Einstein's equations together with regularity requirements and boundary conditions to determine their dynamics. The resultant equations turn out to be those of boundary fluid dynamics, with specific values for fluid parameters. Our analysis is perturbative in the boundary derivative expansion but is valid for arbitrary amplitudes. Our work may be regarded as a derivation of the nonlinear equations of boundary fluid dynamics from gravity. As a concrete application we find an explicit expression for the expansion of this fluid stress tensor including terms up to second order in the derivative expansion.

This paper has not been read by Pith yet.

discussion (0)

Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.

Forward citations

Cited by 5 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score.

  1. All-order fluctuating hydrodynamics of the SYK lattice

    hep-th 2026-04 conditional novelty 8.0

    Derives the all-order fluctuating hydrodynamics effective action and transport coefficients for the SYK lattice from its microscopic pseudo-Goldstone boson action.

  2. Universal analytic dependence of the stress-energy tensor at thermodynamic equilibrium in curved space-time

    hep-th 2026-04 unverdicted novelty 7.0

    The analytic part of the stress-energy tensor at thermodynamic equilibrium has a universal covariant form independent of specific curved spacetime geometry for the massless scalar field, argued to hold for any quantum...

  3. Quasinormal Modes of pp-Wave Spacetimes and Zero Temperature Dissipation

    gr-qc 2026-04 unverdicted novelty 7.0

    Scalar quasinormal modes on pp-wave spacetimes show zero-temperature dissipation for d >= 3 via an irregular singular point acting as absorber, with exact non-dissipative spectrum for d=2 and gapped modes proven by re...

  4. Relativistic BDNK MHD Evolution in a Boost-Invariant Medium and Its Impact on Dilepton Production

    nucl-th 2026-05 unverdicted novelty 5.0

    Coupled BDNK MHD evolution in boost-invariant flow enhances cooling and suppresses the low-mass dilepton spectrum via magnetic-thermal feedback.

  5. Quasinormal modes of black holes and black branes

    gr-qc 2009-05 unverdicted novelty 2.0

    Quasinormal modes are eigenmodes of dissipative gravitational systems whose spectra encode near-equilibrium transport coefficients in dual quantum field theories and enable tests of general relativity through gravitat...