A small cosmological constant due to non-perturbative quantum effects
Jan Holland, Stefan Hollands

TL;DR
This paper suggests that non-perturbative quantum effects can produce an exponentially small vacuum energy, potentially explaining the observed smallness of the cosmological constant, by analyzing a toy model and extrapolating to the Standard Model.
Contribution
It introduces a novel approach linking non-perturbative effects to the small cosmological constant, supported by a rigorous analysis of the 2D Gross-Neveu model.
Findings
Non-perturbative effects lead to an exponentially suppressed vacuum energy.
The analysis addresses renormalization ambiguities in the stress energy tensor.
Extrapolation suggests a tiny vacuum energy in the Standard Model due to non-perturbative factors.
Abstract
We propose that the expectation value of the stress energy tensor of the Standard Model should be given by , with a vacuum energy that differs from the usual "dimensional analysis" result by an exponentially small factor associated with non-perturbative effects. We substantiate our proposal by a rigorous analysis of a toy model, namely the 2-dimensional Gross-Neveu model. In particular, we address, within this model, the key question of the renormalization ambiguities affecting the calculation. The stress energy operator is constructed concretely via the operator-product-expansion. The non-perturbative factor in the vacuum energy is seen as a consequence of the facts that a) the OPE-coefficients have an analytic dependence on , b) the vacuum correlations have a non-analytic (=non-perturbative) dependence on , which we propose…
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.
