The Physical Relevance of the Fiducial Cell in Loop Quantum Cosmology
arXiv:2109.10663 · doi:10.1103/PhysRevD.108.106004
Abstract
A common way to avoid divergent integrals in homogeneous spatially non-compact gravitational systems is to introduce a fiducial cell by cutting-off the spatial slice at a finite region . This is usually considered as an auxiliary regulator to be removed after computations by sending . In this paper, we analyse the dependence of the classical and quantum theory of homogeneous, isotropic and spatially flat cosmology on . We show that each fixed regularisation leads to a different canonically independent theory. At the classical level, the dynamics of observables is not affected by the regularisation on-shell. For the quantum theory, however, this leads to a family of regulator dependent quantum representations and the limit becomes then more subtle. First, we construct a novel isomorphism between different -regularisations, which allows us to identify states in the different -labelled Hilbert spaces to ensure equivalent dynamics for any value of . The limit would then correspond to choosing a state for which the volume assigned to the fiducial cell becomes infinite as appropriate in the late-time regime. As second main result of our analysis, quantum fluctuations of observables smeared over subregions , unlike those smeared over the full , explicitly depend on the size of the fiducial cell through the ratio interpreted as the (inverse) number of subcells homogeneously patched together into . Physically relevant fluctuations for a finite region, as e.g. in the early-time regime, which would be unreasonably suppressed in a naïve limit, become appreciable at small volumes. Our results suggest that the fiducial cell is not playing the role of a mere regularisation but is physically relevant at the quantum level and complement previous statements in the literature.
Published version, 13 pages (REVTeX format), 1 figure. Minor clarifications added
References in corpus (11)
- Quantum Nature of the Big Bang: Improved dynamics
- Corrections to the Friedmann Equations from LQG for a Universe with a Free Scalar Field
- Quantum cosmology: a review
- Singularities and Quantum Gravity
- Loop Quantum Cosmology: A brief review
- An elementary introduction to loop quantum gravity
- Effective Field Theory of Loop Quantum Cosmology
- Path integral renormalisation in loop quantum cosmology
- Space-time physics in background-independent theories of quantum gravity
- Canonical derivation of effective potentials
- Taming Fluctuations for Gaussian States in Loop Quantum Cosmology