Emergent time, cosmological constant and boundary dimension at infinity in combinatorial quantum gravity
Carlo A. Trugenberger

TL;DR
This paper explores how combinatorial quantum gravity models lead to emergent space-time with a transition from negative to positive curvature, revealing a universe that avoids singularities and exhibits a boundary dimension of three at infinity.
Contribution
It provides a detailed picture of space-time emergence in combinatorial quantum gravity, linking discrete graph models to Lorentzian manifolds and cosmological constants.
Findings
Emergent space-time is modeled as a transition from negative to positive curvature.
The boundary dimension at infinity is always three for negative curvature manifolds.
The universe avoids a big bang singularity through a negative-curvature phase.
Abstract
Combinatorial quantum gravity is governed by a discrete Einstein-Hilbert action formulated on an ensemble of random graphs. There is strong evidence for a second-order quantum phase transition separating a random phase at strong coupling from an ordered, geometric phase at weak coupling. Here we derive the picture of space-time that emerges in the geometric phase, given such a continuous phase transition. In the geometric phase, ground-state graphs are discretizations of Riemannian, negative-curvature Cartan-Hadamard manifolds. On such manifolds, diffusion is ballistic. Asymptotically, diffusion time is soldered with a manifold coordinate and, consequently, the probability distribution is governed by the wave equation on the corresponding Lorentzian manifold of positive curvature, de Sitter space-time. With this asymptotic Lorentzian picture, the original negative curvature of the…
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