Chameleon perfect scalar field as a geometric correction in $f(R)$ gravity
Laura L. Parrilla, Celia Escamilla-Rivera

TL;DR
This paper derives an $f(R)$ gravity model incorporating a chameleon scalar field, which can mimic dark sector components and satisfy cosmological constraints from inflation to late times.
Contribution
It introduces an analytical $f(R)$ model with a perfect scalar chameleon field, linking geometric corrections to dark sector phenomena and cosmological constraints.
Findings
The $f(R)$ model describes a perfect scalar field with chameleon mechanism.
The model can explain dark sector phenomena as geometric fluid.
It satisfies BBN constraints during inflation and late times.
Abstract
In this work, we derive the analytical form for a model that describes a perfect scalar field by assuming the existence of a chameleon mechanism. Based on four statements, at the background and perturbative level, it is possible to relate the extra terms from this theory as a geometrical perfect fluid term, whose has been expressed as possible candidates to explain the nature of the dark sector, and possibly, in the case of a perfect scalar chameleon during inflation, satisfy the big bang nucleosynthesis (BBN) constraints until late times.
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 · Geophysics and Gravity Measurements · Black Holes and Theoretical Physics
