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

Padmanabhan, T. (2011) Entropy density of spacetime and the Navier-Stokes fluid dynamics of null surfaces Physical Review D - Particles, Fields, Gravitation and Cosmology, 83 (4). 044048_1-044048_14. ISSN 1550-7998

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Official URL: http://prd.aps.org/abstract/PRD/v83/i4/e044048

Related URL: http://dx.doi.org/10.1103/PhysRevD.83.044048

Abstract

It has been known for several decades that Einstein's field equations, when projected onto a null surface, exhibit a structure very similar to the nonrelativistic Navier-Stokes equation. I show that this result arises quite naturally when gravitational dynamics is viewed as an emergent phenomenon. Extremizing 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 equation. This is in contrast to the usual description of the Damour-Navier-Stokes equation in a general coordinate system, in which there appears a Lie derivative rather than a 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 stress-tensor, involves the second derivatives of the metric and does not vanish in the local inertial frame, while the viscous stress-tensor itself vanishes so that inertial observers detect no dissipation. We thus provide an entropy extremization principle that leads to the Damour-Navier-Stokes equation, which makes the hydrodynamical analogy with gravity completely natural and obvious. Several implications of these results are discussed.

Item Type:Article
Source:Copyright of this article belongs to The American Physical Society.
ID Code:72649
Deposited On:29 Nov 2011 05:55
Last Modified:29 Nov 2011 05:55

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