
We propose a “structural vacuum” in which gravitation and effective spacetime geometry arise from deformation of a real physical medium described by a density fieldρ(x) and a rigidity λ(x, t). Matter corresponds to confined deformation; gravity to extended relaxation of ρ around defects; and radiation to internal gauge-field excitationspropagating on a stable background. A compact covariant action yields (i) a Poissonlike Newtonian limit for static weak deformations, (ii) an emergent Einstein sector atelastic equilibrium, and (iii) a clean linearized regime reproducing Klein–Gordon and Schrödinger kinematics. A multiscale rigidity profile λ(r)yields Newtonian gravity at short distances, MOND-like galactic dynamics at intermediate scales, and an effective late-time acceleration without inserting a fundamental cosmological constant. We highlight falsifiable signatures: mild drifts in G eff and c and possible birefringence from constitutive vacuum response.
Modified gravity, Field theory, Theoretical physics, Vacuum structure, Gravitation, Emergent gravity, Cosmology
Modified gravity, Field theory, Theoretical physics, Vacuum structure, Gravitation, Emergent gravity, Cosmology
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