Perfect fluid Lagrangian and its cosmological implications in theories of gravity with nonminimally coupled matter fields

TL;DR

This paper investigates the dependence of the perfect fluid Lagrangian on microscopic properties and explores its implications for modified gravity theories, providing constraints based on cosmic microwave background observations.

Contribution

It demonstrates that the on-shell Lagrangian of a perfect fluid can depend on microscopic details and shows how this affects gravity theories with matter Lagrangians explicitly in the equations.

Findings

The on-shell Lagrangian equals the trace of the energy-momentum tensor for soliton-like fluids.

Modified gravity theories with matter Lagrangians can lead to observable spectral distortions in the CMB.

Constraints on $f(R,\mathcal{L}_m)$ theories are derived from COBE-FIRAS data.

Abstract

In this paper we show that the on-shell Lagrangian of a perfect fluid depends on microscopic properties of the fluid, giving specific examples of perfect fluids with different on-shell Lagrangians but with the same energy-momentum tensor. We demonstrate that if the fluid is constituted by localized concentrations of energy with fixed rest mass and structure (solitons) then the average on-shell Lagrangian of a perfect fluid is given by ${\mathcal L}_m=T$, where $T$ is the trace of the energy-momentum tensor. We show that our results have profound implications for theories of gravity where the matter Lagrangian appears explicitly in the equations of motion of the gravitational and matter fields, potentially leading to observable deviations from a nearly perfect cosmic microwave background black body spectrum: $n$-type spectral distortions, affecting the normalization of the spectral energy density. Finally, we put stringent constraints on $f(R,{\mathcal L}_m)$ theories of gravity using the COBE-FIRAS measurement of the spectral radiance of the cosmic microwave background.