Equivalence of matter-type modified gravity theories to general relativity with nonminimal matter interaction

In this study, we first establish that gravity models incorporating matter-related terms, such as f(Lm), f(gμνTμν), and f(TμνTμν), into the usual matter Lagrangian density Lm, are equivalent to general relativity (GR) with nonminimal matter interactions. Through the redefinition Lm+f→Lmtot, these models are exactly GR, yet the usual material field Tμν and its accompanying partner, namely, the modification field Tμνmod, engage in nonminimal interactions. Specifically, T=-Qν=-μTμνmod, where Qν is the interaction kernel that governs the rate of energy transfer. Our focus narrows on the specific model of f(TμνTμν), known as energy-momentum squared gravity (EMSG), where the usual material field Tμν is accompanied by an energy-momentum squared field (EMSF), Tμνemsf, along with a sui generis nonminimal interaction between them. We demonstrate that a particular Tμνemsf can be introduced by removing ∂2Lm∂gμν∂gσϵ (the new term emerging in models that incorporate scalars formed from Tμν), thanks to the freedom in determining the interaction kernel, but this approach compromises the Lagrangian formulation of EMSG. Additionally, we address the ambiguities regarding the perfect fluid stemming from this new term. We show the proper way of calculating this term for a perfect fluid, revealing that it is indeed nonzero, contrary to common assumption in the literature. Finally, we reexamine cosmological models within the realm of EMSG, offering new insights into the applicability and interpretation of our findings in EMSG and similar theoretical frameworks.