Equivalent Theories and Changing Hamiltonian Observables in General Relativity
J. Brian Pitts

TL;DR
This paper explores different definitions of observables in Hamiltonian General Relativity, proposing a systematic approach that reconciles gauge invariance and change, with implications for understanding gravitational observables.
Contribution
It introduces a combined framework using the gauge generator G and non-zero Lie derivative brackets to define observables, addressing limitations of previous definitions in GR.
Findings
The Pons-Salisbury-Sundermeyer definition with G succeeds in gauge electromagnetism.
The usual definition fails for gauge electromagnetism, but the new approach succeeds.
Lie derivative as Poisson bracket aligns with gauge invariance in GR.
Abstract
Change and local spatial variation are missing in Hamiltonian General Relativity according to the most common definition of observables (0 Poisson bracket with all first-class constraints). But other definitions have been proposed. Seeking Hamiltonian-Lagrangian equivalence, Pons, Salisbury and Sundermeyer use the Anderson-Bergmann-Castellani gauge generator G, a tuned sum of first-class constraints. Kucha\v{r} waived the 0 Poisson bracket condition for the Hamiltonian constraint to achieve changing observables. A systematic combination of the two reforms might use the gauge generator but permit non-zero Lie derivative Poisson brackets. One can test definitions by calculation using two formulations of a theory, one without gauge freedom and one with it, which must have equivalent observables. For de Broglie-Proca non-gauge massive electromagnetism, all constraints are second-class, so…
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