Toolkit for Scalar Fields in Universes with finite-dimensional Hilbert Space
Oliver Friedrich, Ashmeet Singh, Olivier Dor\'e

TL;DR
This paper develops tools to analyze scalar fields with finite-dimensional Hilbert spaces in cosmological settings, revealing how such constraints influence entropy, vacuum energy, and their evolution in the universe.
Contribution
It introduces a framework for studying finite-dimensional Hilbert spaces in quantum gravity and cosmology, including entropy and vacuum energy calculations, with potential for future research.
Findings
Maximum entropy scales with the universe's boundary area for certain parameters.
Entropy generally follows sub-volume scaling as Hilbert space dimension decreases with momentum.
Vacuum energy density is dynamical, decaying between two epochs.
Abstract
The holographic principle suggests that the Hilbert space of quantum gravity is locally finite-dimensional. Motivated by this point-of-view, and its application to the observable Universe, we introduce a set of numerical and conceptual tools to describe scalar fields with finite-dimensional Hilbert spaces, and to study their behaviour in expanding cosmological backgrounds. These tools include accurate approximations to compute the vacuum energy of a field mode as a function of the dimension of the mode Hilbert space, as well as a parametric model for how that dimension varies with . We show that the maximum entropy of our construction momentarily scales like the boundary area of the observable Universe for some values of the parameters of that model. And we find that the maximum entropy generally follows a sub-volume scaling as long as…
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Taxonomy
TopicsCosmology and Gravitation Theories · Black Holes and Theoretical Physics · Noncommutative and Quantum Gravity Theories
