The Semiclassical Limit of Causal Dynamical Triangulations
J. Ambjorn, A. Gorlich, J. Jurkiewicz, R. Loll, J. Gizbert-Studnicki, and T. Trzesniewski

TL;DR
This paper investigates the semiclassical limit of causal dynamical triangulations (CDT) in quantum gravity, confirming a de Sitter universe structure and exploring discretization effects and higher-order curvature terms.
Contribution
It provides a detailed nonperturbative analysis of the semiclassical limit in CDT, including a new method for fixing total four-volume in simulations.
Findings
Confirmation of de Sitter universe structure in CDT
Identification of short-distance discretization effects
First detailed investigation of higher-order curvature terms
Abstract
Previous work has shown that the macroscopic structure of the theory of quantum gravity defined by causal dynamical triangulations (CDT) is compatible with that of a de Sitter universe. After emphasizing the strictly nonperturbative nature of this semiclassical limit we present a detailed study of the three-volume data, which allows us to re-confirm the de Sitter structure, exhibit short-distance discretization effects, and make a first detailed investigation of the presence of higher-order curvature terms in the effective action for the scale factor. Technically, we make use of a novel way of fixing the total four-volume in the simulations.
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.
