Curvature-matter couplings in modified gravity: from linear models to conformally invariant theories

TL;DR

This paper reviews modified gravity theories with curvature-matter couplings, exploring their cosmological implications, thermodynamics, and conformal invariance, proposing generalizations to standard cosmological models and discussing conformally invariant gravity theories.

Contribution

It introduces a comprehensive analysis of curvature-matter couplings in modified gravity, including thermodynamic implications and a conformally invariant gravity model with nonminimal matter coupling.

Findings

Non-conservation of energy-momentum tensor leads to non-geodesic motion.

Generalized cosmological model with particle creation and effective pressures.

Conformally invariant $f(R,L_m)$ gravity theory with nonminimal matter coupling.

Abstract

In this proceeding, we review modified theories of gravity with a curvature-matter coupling between an arbitrary function of the scalar curvature and the Lagrangian density of matter. This explicit nonminimal coupling induces a non-vanishing covariant derivative of the energy-momentum tensor, that implies non-geodesic motion and consequently leads to the appearance of an extra force. Here, we explore the physical and cosmological implications of the nonconservation of the energy-momentum tensor by using the formalism of irreversible thermodynamics of open systems in the presence of matter creation/annihilation. The particle creation rates, pressure, and the expression of the comoving entropy are obtained in a covariant formulation and discussed in detail. Applied together with the gravitational field equations, the thermodynamics of open systems lead to a generalization of the standard $\Lambda$CDM cosmological paradigm, in which the particle creation rates and pressures are effectively considered as components of the cosmological fluid energy-momentum tensor. Furthermore, we also briefly present the coupling of curvature to geometry in conformal quadratic Weyl gravity, by assuming a coupling term of the form $L_m\tilde{R}^2$, where $L_m$ is the ordinary matter Lagrangian, and $\tilde{R}$ is the Weyl scalar. The coupling explicitly satisfies the requirement of the conformal invariance of the theory. Expressing $\tilde{R}^2$ with the use of an auxiliary scalar field and of the Weyl scalar, the gravitational action can be linearized in the Ricci scalar, leading in the Riemann space to a conformally invariant $f\left(R,L_m\right)$ type theory, with the matter Lagrangian nonminimally coupled to geometry.