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${\rm BMS}_3$ invariant fluid dynamics at null infinity

Robert F. Penna

TL;DR

The paper shows that the boundary dynamics of three-dimensional asymptotically flat gravity can be formulated as Hamiltonian flow on the dual of a semidirect-product Lie algebra, with the symmetry group $S={\rm Diff}(S^1) \ltimes_{\rm Ad} {\rm \mathfrak{vir}}$ and central charge $c=3/G$. It identifies the boundary energy and momentum densities with fluid-like variables $p$ and $j$, and derives their evolution from a Hamiltonian $H=\int_{S^1} \xi j\,d\phi$, reproducing the boundary fluid equations via the Lie-Poisson structure. The associated conserved charges form a centrally extended ${\rm BMS}_3$ algebra, providing a fluid-dynamics perspective on BMS symmetries and a streamlined route to their central extension. The approach clarifies how the Schwarzian term and diffeomorphism data fix the central charge and offers a path toward understanding the four-dimensional BMS group within a membrane-paradigm / fluid-dynamics framework, and suggests generalizations to AdS contexts. Overall, it unifies boundary gravity with boundary fluid dynamics through a concrete Hamiltonian/Lie-Poisson formulation.

Abstract

We revisit the boundary dynamics of asymptotically flat, three dimensional gravity. The boundary is governed by a momentum conservation equation and an energy conservation equation, which we interpret as fluid equations, following the membrane paradigm. We reformulate the boundary's equations of motion as Hamiltonian flow on the dual of an infinite-dimensional, semi-direct product Lie algebra equipped with a Lie-Poisson bracket. This gives the analogue for boundary fluid dynamics of the Marsden-Ratiu-Weinstein formulation of the compressible Euler equations on a manifold, $M$, as Hamiltonian flow on the dual of the Lie algebra of ${\rm Diff}(M)\ltimes C^\infty(M)$. The Lie group for boundary fluid dynamics turns out to be ${\rm Diff}(S^1) \ltimes_{\rm Ad} {\rm \mathfrak{vir}}$, with central charge $c=3/G$. This gives a new derivation of the centrally extended, three-dimensional Bondi-van der Burg-Metzner-Sachs (${\rm BMS}_3$) group. The relationship with fluid dynamics helps to streamline and physically motivate the derivation. For example, the central charge, $c=3/G$, is simply read off of a fluid equation in much the same way as one reads off a viscosity coefficient. The perspective presented here may useful for understanding the still mysterious four-dimensional BMS group.

${\rm BMS}_3$ invariant fluid dynamics at null infinity

TL;DR

The paper shows that the boundary dynamics of three-dimensional asymptotically flat gravity can be formulated as Hamiltonian flow on the dual of a semidirect-product Lie algebra, with the symmetry group and central charge . It identifies the boundary energy and momentum densities with fluid-like variables and , and derives their evolution from a Hamiltonian , reproducing the boundary fluid equations via the Lie-Poisson structure. The associated conserved charges form a centrally extended algebra, providing a fluid-dynamics perspective on BMS symmetries and a streamlined route to their central extension. The approach clarifies how the Schwarzian term and diffeomorphism data fix the central charge and offers a path toward understanding the four-dimensional BMS group within a membrane-paradigm / fluid-dynamics framework, and suggests generalizations to AdS contexts. Overall, it unifies boundary gravity with boundary fluid dynamics through a concrete Hamiltonian/Lie-Poisson formulation.

Abstract

We revisit the boundary dynamics of asymptotically flat, three dimensional gravity. The boundary is governed by a momentum conservation equation and an energy conservation equation, which we interpret as fluid equations, following the membrane paradigm. We reformulate the boundary's equations of motion as Hamiltonian flow on the dual of an infinite-dimensional, semi-direct product Lie algebra equipped with a Lie-Poisson bracket. This gives the analogue for boundary fluid dynamics of the Marsden-Ratiu-Weinstein formulation of the compressible Euler equations on a manifold, , as Hamiltonian flow on the dual of the Lie algebra of . The Lie group for boundary fluid dynamics turns out to be , with central charge . This gives a new derivation of the centrally extended, three-dimensional Bondi-van der Burg-Metzner-Sachs () group. The relationship with fluid dynamics helps to streamline and physically motivate the derivation. For example, the central charge, , is simply read off of a fluid equation in much the same way as one reads off a viscosity coefficient. The perspective presented here may useful for understanding the still mysterious four-dimensional BMS group.

Paper Structure

This paper contains 7 sections, 52 equations.