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Local Fluid Dynamical Entropy from Gravity

2 Pith papers cite this work. Polarity classification is still indexing.

2 Pith papers citing it
abstract

Spacetime geometries dual to arbitrary fluid flows in strongly coupled N=4 super Yang Mills theory have recently been constructed perturbatively in the long wavelength limit. We demonstrate that these geometries all have regular event horizons, and determine the location of the horizon order by order in a boundary derivative expansion. Intriguingly, the derivative expansion allows us to determine the location of the event horizon in the bulk as a local function of the fluid dynamical variables. We define a natural map from the boundary to the horizon using ingoing null geodesics. The area-form on spatial sections of the horizon can then be pulled back to the boundary to define a local entropy current for the dual field theory in the hydrodynamic limit. The area theorem of general relativity guarantees the positivity of the divergence of the entropy current thus constructed.

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hep-th 2

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2026 1 2025 1

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UNVERDICTED 2

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Dissipative non-Abelian fluids from Scherk-Schwarz dimensional reduction

hep-th · 2026-05-22 · unverdicted · novelty 7.0

Scherk-Schwarz reduction of a neutral viscous conformal fluid yields a dissipative colored fluid in lower dimensions with explicit maps for equation of state, sound speed, color currents, entropy current, and first-order transport coefficients including η, τ, and κ.

Radiation in Fluid/Gravity and the Flat Limit

hep-th · 2025-08-02 · unverdicted · novelty 6.0

Establishes a holographic link between bulk gravitational radiation and dissipative corrections plus entropy production in boundary fluids, then constructs Carrollian analogues and celestial observables in the flat limit.

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  • Radiation in Fluid/Gravity and the Flat Limit hep-th · 2025-08-02 · unverdicted · none · ref 23 · internal anchor

    Establishes a holographic link between bulk gravitational radiation and dissipative corrections plus entropy production in boundary fluids, then constructs Carrollian analogues and celestial observables in the flat limit.