Primordial fluctuations from quantum gravity: 16-cell topological model
Pietropaolo Frisoni, Francesco Gozzini, Francesca Vidotto

TL;DR
This paper numerically analyzes a quantum gravity model of the early universe using covariant Loop Quantum Gravity, focusing on a 16-cell topological truncation, and finds that refinement does not significantly alter the overall physical picture.
Contribution
It introduces a numerical approach to study the Hartle-Hawking state in quantum gravity using a 16-cell topological model within the covariant Loop Quantum Gravity framework.
Findings
Mean geometry and fluctuations computed
Results show refinement does not change global picture
Supports stability of quantum cosmological models
Abstract
We present a numerical analysis of an Hartle-Hawking state for the early universe, in the deep quantum regime, computed using the covariant Loop Quantum Gravity formalism, in a truncation defined by 16-cell and in a simplified case where the dynamics is defined by SU(2) BF theory. We compute mean geometry, fluctuations and correlations. The results are consistent with the hypothesis that refining the triangulation does not affect the global physical picture substantially.
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.
Taxonomy
TopicsBlack Holes and Theoretical Physics · Noncommutative and Quantum Gravity Theories · Cosmology and Gravitation Theories
