Reconsidering a higher-spin-field solution to the main cosmological constant problem
V. Emelyanov, F. R. Klinkhamer

TL;DR
This paper proposes a model with two massless vector fields that dynamically cancel the cosmological constant, leading to a stable Minkowski spacetime without affecting local gravity, thus addressing the cosmological constant problem.
Contribution
The paper introduces a new vector field model that cancels the cosmological constant without disrupting local Newtonian gravity, improving upon previous models.
Findings
Minkowski spacetime emerges as an attractor in the model
The model cancels arbitrary cosmological constants
Local gravitational physics remains unaffected
Abstract
Following an earlier suggestion by Dolgov, we present a specific model of two massless vector fields which dynamically cancel a cosmological constant of arbitrary magnitude and sign. Flat Minkowski spacetime appears asymptotically as an attractor of the field equations. Unlike the original model, the new model does not upset the local Newtonian gravitational dynamics.
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.
