Gravitational Edge Modes, Coadjoint Orbits, and Hydrodynamics William Donnelly,1 Laurent Freidel,1 Seyed Faroogh Moosavian,1;2 Antony J. Speranza1 1Perimeter Institute for Theoretical Physics, 31 Caroline St. N., Waterloo ON, N2L 2Y5, Canada 2Department of Physics, McGill University, Ernest Rutherford Physics Building, 3600 Rue Univer- sity, Montr´eal, QC H3A 2T8, Canada E-mail:
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[email protected] Abstract: The phase space of general relativity in a finite subregion is characterized by edge modes localized at the codimension-2 boundary, transforming under an infinite- dimensional group of symmetries. The quantization of this symmetry algebra is conjectured to be an important aspect of quantum gravity. As a step towards quantization, we derive a complete classification of the positive-area coadjoint orbits of this group for boundaries that are topologically a 2-sphere. This classification parallels Wigner's famous classification of representations of the Poincar´egroup since both groups have the structure of a semidirect product. We find that the total area is a Casimir of the algebra, analogous to mass in the Poincar´egroup. A further infinite family of Casimirs can be constructed from the curvature of the normal bundle of the boundary surface. These arise as invariants of the little group, which is the group of area-preserving diffeomorphisms, and are the analogues of spin. Additionally, we show that the symmetry group of hydrodynamics appears as a reduction of the corner symmetries of general relativity. Coadjoint orbits of both groups are classified by the same arXiv:2012.10367v1 [hep-th] 18 Dec 2020 set of invariants, and, in the case of the hydrodynamical group, the invariants are interpreted as the generalized enstrophies of the fluid.