Geometry for the accelerating universe
Raffaele Punzi, Frederic P. Schuller, Mattias N.R. Wohlfarth

TL;DR
This paper introduces an area metric framework for cosmology, replacing the Lorentzian metric, which naturally accounts for the universe's acceleration without dark energy or fine-tuning.
Contribution
It proposes a novel geometric approach using area metrics derived from string and gauge theories to explain cosmic acceleration.
Findings
Area metric cosmology explains late universe acceleration
No need for dark energy or fine-tuning in this model
Reinterprets Einstein-Hilbert action using area metric curvature scalar
Abstract
The Lorentzian spacetime metric is replaced by an area metric which naturally emerges as a generalized geometry in quantum string and gauge theory. Employing the area metric curvature scalar, the gravitational Einstein-Hilbert action is re-interpreted as dynamics for an area metric. Without the need for dark energy or fine-tuning, area metric cosmology explains the observed small acceleration of the late Universe.
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.
