Entropy density of spacetime and the Navier-Stokes fluid dynamics of null surfaces
T. Padmanabhan

TL;DR
This paper demonstrates that Einstein's equations projected on null surfaces naturally resemble Navier-Stokes fluid dynamics when viewed through an entropy extremisation lens, highlighting gravity's emergent, hydrodynamical nature.
Contribution
It introduces an entropy extremisation principle that derives Navier-Stokes equations from gravitational dynamics in a local inertial frame, clarifying the hydrodynamical analogy.
Findings
Einstein's equations on null surfaces resemble Navier-Stokes equations in an inertial frame.
The entropy extremisation leads directly to the Damour-Navier-Stokes equation.
Viscous forces involve second derivatives of the metric, detectable by inertial observers.
Abstract
It has been known for several decades that Einstein's field equations, when projected onto a null surface, exhibits a structure very similar to non-relativistic Navier-Stokes equation. I show that this result arises quite naturally when gravitational dynamics is viewed as an emergent phenomenon. Extremising the spacetime entropy density associated with the null surfaces leads to a set of equations which, when viewed in the local inertial frame, becomes identical to the Navier-Stokes (NS) equation. This is in contrast with the usual description of Damour-Navier-Stokes (DNS) equation in a general coordinate system, in which there appears a Lie derivative rather than convective derivative. I discuss this difference, its importance and why it is more appropriate to view the equation in a local inertial frame. The viscous force on fluid, arising from the gradient of the viscous…
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