Analysis of F(R,T) Gravity Models Through Energy Conditions

Understand

This paper is devoted to study the energy conditions in F(R,T) gravity for FRW universe with perfect fluid, where $R$ is the Ricci scalar and $T$ is the torsion scalar.

• We construct the general energy conditions in this theory and reduce them in F(R) as well as F(T) theory of gravity.
• Further, we assume some viable models and investigate bounds on their constant parameters to satisfy the energy condition inequalities.
• We also plot some of the cases using present-day values of the cosmological parameters.