A natural fuzzyness of de Sitter space-time
Jean-Pierre Gazeau, Francesco Toppan

TL;DR
This paper introduces a non-commutative, fuzzy model of de Sitter spacetime using Pauli-Lubanski operators, revealing implications for particle masses and spacetime granularity depending on the chosen scenario.
Contribution
It proposes a novel fuzzy de Sitter space model based on non-commutative geometry and analyzes its physical implications for particle masses and spacetime structure.
Findings
Lower bound on particle masses related to Hubble scale in scenario I
Determination of spacetime granularity in scenario II
Recovery of classical de Sitter space at large distances
Abstract
A non-commutative structure for de Sitter spacetime is naturally introduced by replacing ("fuzzyfication") the classical variables of the bulk in terms of the dS analogs of the Pauli-Lubanski operators. The dimensionality of the fuzzy variables is determined by a Compton length and the commutative limit is recovered for distances much larger than the Compton distance. The choice of the Compton length determines different scenarios. In scenario I the Compton length is determined by the limiting Minkowski spacetime. A fuzzy dS in scenario I implies a lower bound (of the order of the Hubble mass) for the observed masses of all massive particles (including massive neutrinos) of spin s>0. In scenario II the Compton length is fixed in the de Sitter spacetime itself and grossly determines the number of finite elements ("pixels" or "granularity") of a de Sitter spacetime of a given curvature.
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
