Can universe exit from phantom inflation due to gravitational back reaction?
Puxun Wu, Hongwei Yu

TL;DR
This paper explores whether gravitational back reaction can halt phantom inflation, showing that it can counteract phantom energy and potentially end inflation if certain conditions are met.
Contribution
It calculates the effective energy-momentum tensor of gravitational back reaction and demonstrates its potential to terminate phantom inflation.
Findings
Gravitational back reaction opposes phantom energy effects.
Back reaction can end phantom inflation if the phantom field exceeds a critical value.
The study provides a mechanism for ending phantom inflation via gravitational effects.
Abstract
The effects of the gravitational back reaction of cosmological perturbations are investigated in a phantom inflation model. The effective energy-momentum tensor of the gravitational back reaction of cosmological perturbations whose wavelengths are larger than the Hubble radius is calculated. Our results show that the effects of gravitational back reaction will counteract that of the phantom energy. It is demonstrated in a chaotic phantom inflation model that if the phantom field at the end of inflation is larger than a critical value determined by the necessary e-folds, the phantom inflation phase might be terminated by the gravitational back reaction.
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.
