A Reasonable Ab Initio Cosmological Constant Without Holography
Aaron D. Trout

TL;DR
This paper proposes a novel explanation for dark energy as a residual negative scalar-curvature arising from spacetime discreteness, with a model predicting a cosmological constant consistent with observations without relying on holography.
Contribution
It introduces a discrete spacetime model using dynamical triangulations to derive the cosmological constant from vacuum energy differences, providing a rigorous, parameter-free prediction.
Findings
Predicted cosmological constant magnitude matches observed value (~10^{-123})
Vacuum energy levels are quantized in increments related to Planck length and volume
Model predicts the correct sign of the cosmological constant based on entropy considerations.
Abstract
We give a well-motivated explanation for the origin of dark energy, claiming that it arises from a small residual negative scalar-curvature present even in empty spacetime. The vacuum has this residual curvature because spacetime is fundamentally discrete and there are more ways for a discrete geometry to have negative curvature than positive. We explicitly compute this effect in the well-known {\em dynamical triangulations} (DT) model for quantum gravity and the predicted cosmological constant agrees with observation. We begin by almost completely characterizing the DT-model's vacuum energies in dimension three. Remarkably, the energy gap between states comes in increments of [\Delta\mathcal{A} =\frac{\ell}{8\mathcal{V}}] in natural units, where is the "Planck length" in the model and is the volume of the universe. Then, using only vacua in the …
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.
Taxonomy
TopicsCosmology and Gravitation Theories · Noncommutative and Quantum Gravity Theories · Relativity and Gravitational Theory
