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Shape multipoles as Hamiltonian charges

Identify a phase-space and symmetry framework in which shape multipoles on a dynamical horizon segment arise as Hamiltonian surface charges associated with canonical transformations, paralleling the BMS supermomentum charges at null infinity.

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Background

The review highlights a striking functional identity between horizon multipoles and BMS supermomentum/dual supermomentum charges, even in radiative regimes, suggesting deep structural parallels between WIHSs and null infinity.

While BMS charges at null infinity are well-understood within Hamiltonian phase spaces, an analogous interpretation for shape multipoles on DHSs would unify quasi-local and asymptotic observables and clarify symmetry generators acting on horizon data.

References

Open Issue 9 (OI-9) The BMS supermomentum fluxes arise as Hamiltonians generating actions of BMS supertranslations on a phase space constructed at +. Is there a similar interpretation for shape multipoles on the DHS, given that the two charges have the same functional form?

Quasi-Local Black Hole Horizons: Recent Advances (2502.11825 - Ashtekar et al., 17 Feb 2025) in Section 5.3