Can Chameleon Field be identified with Quintessence ?
A. N. Ivanov, M. Wellenzohn

TL;DR
This paper investigates whether the chameleon scalar field in Einstein-Cartan theory can be equated with quintessence, concluding that while it influences dark energy and cosmic acceleration, it cannot be fully identified as quintessence.
Contribution
It provides an analysis of the chameleon field's role in cosmic acceleration within Einstein-Cartan theory, clarifying its limitations in being identified as quintessence.
Findings
Chameleon field affects dark energy dynamics.
It influences late-time cosmic acceleration.
Cannot be fully equated with quintessence.
Abstract
In the Einstein-Cartan gravitational theory with the chameleon field, changing its mass in dependence of a density of its environment, we analyze the Friedmann-Einstein equations for the Universe evolution with the expansion parameter dependent on time only. We analyze the problem of an identification of the chameleon field with quintessence, i.e. a canonical scalar field responsible for dark energy dynamics and for the acceleration of the Universe expansion. We show that since the cosmological constant, related to the relic dark energy density, is induced by torsion (Astrophys. J.829, 47 (2016)), the chameleon field may, in principle, possess some properties of quintessence such as an influence on the dark energy dynamics and the acceleration of the Universe expansion even on the late-time acceleration, but it cannot be identified with quintessence to full extent.
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 · Black Holes and Theoretical Physics · Solar and Space Plasma Dynamics
