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  • Open Access

Consistent energy-momentum trace couplings of fluids

Christian G. Böhmer1,2,* and Eissa Al-Nasrallah1,3,†

  • 1Department of Mathematics, University College London, Gower Street, London WC1E 6BT, United Kingdom
  • 2Astrophysics Research Centre, School of Mathematics, Statistics and Computer Science, University of KwaZulu-Natal, Private Bag X54001, Durban 4000, South Africa
  • 3Department of Physics, College of Science, Kuwait University, Sabah Al Salem University City, P.O. Box 2544, Safat 1320, Kuwait

  • *Contact author: c.boehmer@ucl.ac.uk
  • †Contact author: eissa.alnasrallah.24@ucl.ac.uk

Phys. Rev. D 112, 124073 – Published 24 December, 2025

DOI: https://doi.org/10.1103/6wrh-lg9s

Abstract

Gravitational models with nonminimal couplings involving the trace of the energy-momentum tensor have become increasingly popular. The idea of coupling the trace of the matter tensor to the geometry can be applied to various matter models, including relativistic perfect fluids. However, it is well known that the variational formulation of perfect fluids involves some technicalities. We carefully derive the field equations including the trace coupling of a perfect fluid using two different approaches, namely, that given by Brown using Lagrange multipliers and that given by Schutz using velocity potentials. We show that previous results involving such trace couplings do not match the results presented here. We demonstrate that our fluid’s equations of motion are consistent with the gravitational field equations. Moreover, we present a simple on-shell argument which further supports the correctness of our results. Our work implies that a vast amount of the f(R,T) literature using perfect fluids needs to be revisited.

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