Loop Quantum Cosmology Matter Bounce Reconstruction from $F(R)$ Gravity Using an Auxiliary Field
V.K. Oikonomou

TL;DR
This paper reconstructs specific $F(R)$ gravity models capable of producing matter bounce cosmological solutions, linking early inflation and late-time acceleration within a unified framework.
Contribution
It demonstrates how $F(R)$ gravities can generate matter bounce solutions and connects these models to inflation and dark energy phenomena.
Findings
$F(R) o R + ext{const} imes R^2$ at high curvature for inflation
$F(R) o 1/R$ at low curvature for late-time acceleration
Reconstructed scale factor closely matches matter bounce scenario in limits
Abstract
Using the reconstruction technique with an auxiliary field, we investigate which gravities can produce the matter bounce cosmological solutions. Owing to the specific functional form of the matter bounce Hubble parameter, the reconstruction technique leads, after some simplifications, to the same Hubble parameter as in the matter bounce scenario. Focusing the study to the large and small cosmic time limits, we were able to find which gravities can generate the matter bounce Hubble parameter. In the case of small cosmic time limit, which corresponds to large curvature values, the gravity is , which is an inflation generating gravity, and at small curvature, or equivalently, large cosmic time, the gravity generating the corresponding limit of the matter bounce Hubble parameter, is , a gravity known to produce…
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.
