Covariant conservation of energy momentum in modified gravities
Tomi Koivisto

TL;DR
This paper proves that energy-momentum conservation is inherently maintained in various modified gravity theories, regardless of the formalism used, ensuring consistency with fundamental physical principles.
Contribution
It provides a general proof of covariant energy-momentum conservation in modified gravities with nonlinear curvature dependence, including metric and Palatini formalisms.
Findings
Energy-momentum conservation is a built-in feature of the field equations.
The covariant divergence of the energy-momentum tensor vanishes in these theories.
In the Einstein frame, a bi-metric structure emerges.
Abstract
An explicit proof of the vanishing of the covariant divergence of the energy-momentum tensor in modified theories of gravity is presented. The gravitational action is written in arbitrary dimensions and allowed to depend nonlinearly on the curvature scalar and its couplings with a scalar field. Also the case of a function of the curvature scalar multiplying a matter Lagrangian is considered. The proof is given both in the metric and in the first-order formalism, i.e. under the Palatini variational principle. It is found that the covariant conservation of energy-momentum is built-in to the field equations. This crucial result, called the generalized Bianchi identity, can also be deduced directly from the covariance of the extended gravitational action. Furthermore, we demonstrate that in all of these cases, the freely falling world lines are determined by the field equations alone and…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
