Fragility of stealth solutions in mimetic gravity
Alireza Allahyari, Clarisse Donio, Mohammad Ali Gorji, Zahra Gorji, Javad T. Firouzjaee
Abstract
We study a broad class of constrained mimetic-type extensions of general relativity with action S=∫ d4x-g\,(R/2+λ\,C[g,Ψ]+ L m), where R is the Ricci scalar, λ is a Lagrange multiplier, C[g,Ψ] is a scalar functional of the metric and generic field content Ψ (possibly involving Ψ and its covariant derivatives) and L m is the matter Lagrangian. The branch λ 0, with the bar denoting a background value, provides a simple screening-like limit in which the constrained sector decouples, as in cosmological realizations where λ is typically nonzero on large scales while locally one expects λ 0. On the exactly stealth branch λ=0, the constrained sector drops out of the background dynamics, so, on domains where a background profile Ψ satisfying C=0 exists, the theory admits the corresponding general relativity geometries as stealth solutions. As an explicit realization of this mechanism, we consider the scalar field case, where C=gμν∂μϕ∂νϕ1=0 becomes a Hamilton-Jacobi equation selecting geodesic congruences; in this setting, we study spherically symmetric solutions and construct a stealth Kerr profile using Carter separability. We then show, at the general level, that the λ=0 branch is perturbatively degenerate with general relativity: the constrained sector contributes to the dynamics only through terms weighted by λ, which vanish on the stealth branch, while still imposing an infinite hierarchy of constraints on the fluctuations. Consequently, the λ0 limit is generically non-uniform, making the would-be screening perturbatively pathological.
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