Constraining $f(R)$ gravity models with disappearing cosmological constant

TL;DR

This paper investigates $f(R)$ gravity models, focusing on their ability to mimic a disappearing cosmological constant while satisfying local gravity constraints and avoiding curvature singularities through fine tuning or quadratic corrections.

Contribution

It analyzes the conditions under which $f(R)$ models can evade local constraints and avoid singularities, proposing potential solutions like quadratic curvature corrections.

Findings

Large deviations violate local constraints or mimic cosmological constant

Curvature singularities are generic but avoidable with fine tuning

Quadratic corrections could circumvent singularity issues

Abstract

The $f(R)$ gravity models proposed by Hu-Sawicki and Starobinsky are generic for local gravity constraints to be evaded. The large deviations from these models either result into violation of local gravity constraints or the modifications are not distinguishable from cosmological constant. The curvature singularity in these models is generic but can be avoided provided that proper fine tuning is imposed on the evolution of scalaron in the high curvature regime. In principle, the problem can be circumvented by incorporating quadratic curvature correction in the Lagrangian though it might be quite challenging to probe the relevant region numerically.