Generalizing the coupling between geometry and matter: $f(R,L_m,T)$ gravity
Zahra Haghani, Tiberiu Harko

TL;DR
This paper introduces a new class of gravity models where the gravitational Lagrangian depends on the Ricci scalar, matter Lagrangian, and energy-momentum trace, unifying previous models and exploring their physical and cosmological implications.
Contribution
It generalizes and unifies $f(R,T)$ and $f(R,L_m)$ gravity models by proposing a function of $R$, $T$, and $L_m$, deriving field equations, and analyzing their physical and cosmological consequences.
Findings
Derived generalized field equations and equations of motion.
Identified conditions for non-geodesic motion and extra forces.
Explored cosmological solutions and stability conditions.
Abstract
We generalize and unify the and type gravity models by assuming that the gravitational Lagrangian is given by an arbitrary function of the Ricci scalar , of the trace of the energy-momentum tensor , and of the matter Lagrangian , so that . We obtain the gravitational field equations in the metric formalism, the equations of motion for test particles, and the energy and momentum balance equations, which follow from the covariant divergence of the energy-momentum tensor. Generally, the motion is non-geodesic, and takes place in the presence of an extra force orthogonal to the four-velocity. The Newtonian limit of the equations of motion is also investigated, and the expression of the extra acceleration is obtained for small velocities and weak gravitational fields. The generalized Poisson equation is also obtained in the Newtonian limit,…
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