The first variation of the matter energy-momentum tensor with respect to the metric, and its implications on modified gravity theories

TL;DR

This paper derives the variation of the matter energy-momentum tensor with respect to the metric, crucial for modified gravity theories like $f(R,T)$, and demonstrates its implications through a cosmological model fitting observational data.

Contribution

It provides a new expression for the variation of the energy-momentum tensor independent of the matter Lagrangian, applicable to $f(R,T)$ gravity theories.

Findings

The variation expression is independent of the matter Lagrangian.

A generalized $f(R,T)$ model fits observational Hubble data up to redshift 2.5.

The model offers a good cosmological description with a $T^n$ term.

Abstract

The first order variation of the matter energy-momentum tensor $T_{\mu \nu}$ with respect to the metric tensor $g^{\alpha \beta}$ plays an important role in modified gravity theories with geometry-matter coupling, and in particular in the $f(R,T)$ modified gravity theory. We obtain the expression of the variation $\delta T_{\mu \nu}/\delta g^{\alpha \beta}$ for the baryonic matter described by an equation given in a parametric form, with the basic thermodynamic variables represented by the particle number density, and by the specific entropy, respectively. The first variation of the matter energy-momentum tensor turns out to be independent on the matter Lagrangian, and can be expressed in terms of the pressure, the energy-momentum tensor itself, and the matter fluid four-velocity. We apply the obtained results for the case of the $f(R,T)$ gravity theory, where $R$ is the Ricci scalar, and $T$ is the trace of the matter energy-momentum tensor, which thus becomes a unique theory, also independent on the choice of the matter Lagrangian. A simple cosmological model, in which the Hilbert-Einstein Lagrangian is generalized through the addition of a term proportional to $T^n$ is considered in detail, and it is shown that it gives a very good description of the observational values of the Hubble parameter up to a redshift of $z\approx 2.5$.