This research investigates stability and consistency of minimal dark energy models relative to General Relativity, indicating challenges in observable deviations.
We investigate whether minimal luminal Effective Field Theory of Dark Energy (EFT-of-DE) models can produce observable deviations from ΛCDM while remaining stable and consistent with current cosmological constraints. Using a numerical parameter scan over a minimal EFT parametrization, we apply theoretical stability conditions (absence of ghost and gradient instabilities) together with observational consistency requirements derived from large-scale structure probes, including growth and lensing observables (μ, Σ, E_G). We find that although stable regions formally exist, the imposition of realistic growth–lensing consistency conditions leads to a collapse of the viable parameter space. This indicates a strong tension between stability, observational consistency, and detectability in minimal scalar–tensor modifications of gravity. Our results suggest that any observable deviation from General Relativity within the EFT-of-DE framework likely requires non-minimal structure, such as scale-dependent effects or extended couplings beyond the minimal parametrization.
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