Modified gravity in the presence of matter creation: scenario for the late Universe
Giovanni Montani, Nakia Carlevaro, Mariaveronica De Angelis

TL;DR
This paper proposes a modified gravity model with matter creation to explain late Universe evolution, aiming to resolve the Hubble tension by fitting observational data within a consistent theoretical framework.
Contribution
It introduces a novel $f(R)$ gravity model incorporating matter creation, providing a new approach to reconcile Planck data with late Universe observations.
Findings
The model can reconcile Planck Hubble measurements with late Universe data.
The scalar field potential determines the current vacuum energy density.
Constraints on matter creation parameters eliminate tachyonic instabilities.
Abstract
We consider a dynamic scenario for characterizing the late Universe evolution, aiming to mitigate the Hubble tension. Specifically, we consider a metric gravity in the Jordan frame which is implemented to the dynamics of a flat isotropic Universe. This cosmological model incorporates a matter creation process, due to the time variation of the cosmological gravitational field. We model particle creation by representing the isotropic Universe (specifically, a given fiducial volume) as an open thermodynamic system. The resulting dynamical model involves four unknowns: the Hubble parameter, the non-minimally coupled scalar field, its potential, and the energy density of the matter component. We impose suitable conditions to derive a closed system for these functions of the redshift. In this model, the vacuum energy density of the present Universe is determined by the scalar field…
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.
