General gravitational charges on null hypersurfaces
Gloria Odak, Antoine Rignon-Bret, Simone Speziale

TL;DR
This paper investigates the covariant symplectic potentials and charges on null hypersurfaces in general relativity, analyzing boundary conditions, symmetries, and their implications for conserved quantities and gravitational fluxes.
Contribution
It identifies a family of covariant symplectic potentials, clarifies conditions for charge conservation, and explores boundary conditions and symmetries on null hypersurfaces in GR.
Findings
Unique symplectic potential selected by stationarity conditions
Charges conserved on non-expanding horizons but not on flat spacetime
Positive flux at flat light-cones reproduces tidal heating and memory effects
Abstract
We perform a detailed study of the covariance properties of the symplectic potential of general relativity on a null hypersurface, and of the different polarizations that can be used to study conservative as well as leaky boundary conditions. This allows us to identify a one-parameter family of covariant symplectic potentials. We compute the charges and fluxes for the most general phase space with arbitrary variations. We study five symmetry groups that arise when different restrictions on the variations are included. Requiring stationarity as in the original Wald-Zoupas prescription selects a unique member of the family of symplectic potentials, the one of Chandrasekaran, Flanagan and Prabhu. The associated charges are all conserved on non-expanding horizons, but not on flat spacetime. We show that it is possible to require a weaker notion of stationarity which selects another…
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Taxonomy
TopicsBlack Holes and Theoretical Physics · Cosmology and Gravitation Theories · Noncommutative and Quantum Gravity Theories
