Semiclassical Universe from First Principles
J. Ambjorn, J. Jurkiewicz, R. Loll

TL;DR
This paper demonstrates that in four-dimensional Causal Dynamical Triangulations, the emergent macroscopic universe behaves as a semiclassical bounce, with a well-defined ground state wave function depending on the global scale factor.
Contribution
It provides a first-principles derivation of a semiclassical bouncing universe within nonperturbative quantum gravity using Causal Dynamical Triangulations.
Findings
Emergence of a four-dimensional bounce in CDT
Ground state wave function as a function of scale factor
Semiclassical equation satisfied by the macroscopic universe
Abstract
Causal Dynamical Triangulations in four dimensions provide a background-independent definition of the sum over space-time geometries in nonperturbative quantum gravity. We show that the macroscopic four-dimensional world which emerges in the Euclidean sector of this theory is a bounce which satisfies a semiclassical equation. After integrating out all degrees of freedom except for a global scale factor, we obtain the ground state wave function of the universe as a function of this scale factor.
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