Scalar field with the source in the form of the stress-energy tensor trace as a dark energy model
I. G. Dudko, Yu. P. Vyblyi

TL;DR
This paper explores a scalar-tensor gravity model where the scalar field's source is its own stress-energy trace, demonstrating a slow-roll regime that can reproduce current cosmological parameters.
Contribution
It introduces a novel scalar-tensor model with the scalar source as the stress-energy trace, providing numerical solutions that match observed cosmological data.
Findings
Existence of a slow-roll regime in the model
Reproduction of current Hubble and deceleration parameters
Potential explanation for dark energy phenomena
Abstract
We consider a scalar-tensor theory of gravitation with the scalar source being the trace of the stress-energy tensor of the scalar field itself and matter. We obtain an example of a numerical solution of the cosmological equations which shows that under some special choice of the scalar parameters, there exists a slow-roll regime in which the modern values of the Hubble and deceleration parameters may be obtained.
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.
