Quantum Gravity, or The Art of Building Spacetime
J. Ambjorn, J. Jurkiewicz, R. Loll
TL;DR
The paper presents causal dynamical triangulations (CDT) as a background-independent, Lorentzian path integral for quantum gravity implemented via a foliated set of causal, simplicial spacetimes. Using Monte Carlo simulations, it demonstrates that a macroscopic four-dimensional universe with a dynamical scale factor emerges, and its large-scale dynamics are captured by an effective action derived from integrating out all other degrees of freedom, yielding a semiclassical bounce akin to tunneling from nothing. The results reveal a scale-dependent spectral dimension, with $D_S(\sigma)$ approaching $4$ at large diffusion times and $\approx 2$ at short times, and show that the observed effective dynamics align with a minisuperspace-like model once quantum fluctuations at small scales are incorporated. These findings support CDT as a viable nonperturbative approach to quantum gravity with a controllable continuum limit and motivate further exploration of renormalization, matter coupling, and transverse gravitational degrees of freedom.
Abstract
The method of four-dimensional Causal Dynamical Triangulations provides a background-independent definition of the sum over geometries in quantum gravity, in the presence of a positive cosmological constant. We present the evidence accumulated to date that a macroscopic four-dimensional world can emerge from this theory dynamically. Using computer simulations we observe in the Euclidean sector a universe whose scale factor exhibits the same dynamics as that of the simplest mini-superspace models in quantum cosmology, with the distinction that in the case of causal dynamical triangulations the effective action for the scale factor is not put in by hand but obtained by integrating out {\it in the quantum theory} the full set of dynamical degrees of freedom except for the scale factor itself.
