Reconstructing the Universe
J. Ambjorn, J. Jurkiewicz, R. Loll
TL;DR
This work demonstrates that a nonperturbative quantum gravity theory defined via causal dynamical triangulations yields a large-scale four-dimensional spacetime with semiclassical volume dynamics, while exhibiting highly nonclassical microstructure. By performing extensive Monte Carlo simulations at fixed four-volume, the authors show four-dimensional global scaling (D_H ≈ 4) and a scale-dependent spectral dimension that flows from D_S(0) ≈ 2 to D_S(∞) ≈ 4, indicating a dynamically generated ultraviolet cutoff. An effective Euclidean action for the scale factor is extracted, matching the minisuperspace form up to a sign flip in the kinetic term, thereby resolving conformal-instability concerns in the Euclidean sector. The analysis of spatial slices reveals a rich nonclassical geometry—thin slices resemble branched polymers with D_S ≈ 1.56 and d_H ≈ 3, while thick slices exhibit D_H ≈ 4 and D_S ≈ 2 with suppressed baby universes—pointing to a nuanced, scale-dependent quantum geometry with potential analytic bridges to branched-polymer models and quantum cosmology.
Abstract
We provide detailed evidence for the claim that nonperturbative quantum gravity, defined through state sums of causal triangulated geometries, possesses a large-scale limit in which the dimension of spacetime is four and the dynamics of the volume of the universe behaves semiclassically. This is a first step in reconstructing the universe from a dynamical principle at the Planck scale, and at the same time provides a nontrivial consistency check of the method of causal dynamical triangulations. A closer look at the quantum geometry reveals a number of highly nonclassical aspects, including a dynamical reduction of spacetime to two dimensions on short scales and a fractal structure of slices of constant time.
