Gauge invariant variables for cosmological perturbation theory using geometrical clocks
Kristina Giesel, Adrian Herzog, Parampreet Singh

TL;DR
This paper links gauge choices in cosmological perturbation theory to geometrical clocks within a canonical framework, systematically deriving gauge invariant variables as Dirac observables for various gauges, enhancing understanding at both classical and quantum levels.
Contribution
It introduces a systematic method to derive gauge invariant variables as Dirac observables using geometrical clocks in the extended ADM-phase space, applicable to multiple gauges and higher-order perturbations.
Findings
Derives gauge invariant variables as Dirac observables for five common gauges.
Shows Bardeen potentials and Mukhanov-Sasaki variable naturally emerge as observables.
Provides a framework for extending analysis beyond linear order in perturbation theory.
Abstract
Using the extended ADM-phase space formulation in the canonical framework we analyze the relationship between various gauge choices made in cosmological perturbation theory and the choice of geometrical clocks in the relational formalism. We show that various gauge invariant variables obtained in the conventional analysis of cosmological perturbation theory correspond to Dirac observables tied to a specific choice of geometrical clocks. As examples, we show that the Bardeen potentials and the Mukhanov-Sasaki variable emerge naturally in our analysis as observables when gauge fixing conditions are determined via clocks in the Hamiltonian framework. Similarly other gauge invariant variables for various gauges can be systematically obtained. We demonstrate this by analyzing five common gauge choices: longitudinal, spatially flat, uniform field, synchronous and comoving gauge. For all…
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