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Emergent Origin of the Hubble Tension

Livolsi, Edoardo
PhilArchive · Papers
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philosophy
This work shows that the Hubble tension is not an observational anomaly but a structural necessity arising from a closed quartic variational functional. Using the universal Ψ–Γ framework, the cosmological expansion rate emerges as an invariant of global variational closure rather than a dynamical quantity. When observational analysis is restricted to a local domain, loss of global closure forces the appearance of a distinct invariant, leading to HL>HG H L ​ >H G ​ as an unavoidable inequality. Any cosmological model that defines H H as a single global function of time—such as ΛCDM, Early Dark Energy models, or neutrino-sector extensions—cannot generate domain-dependent expansion scales, establishing a strict No-Go Theorem. The Hubble tension is therefore a calibration effect produced by projecting a globally constrained structure onto restricted observational domains, not evidence for new fields or parameters. The result is parameter-free, fully variational, and derived from the intrinsic mathematical closure of the Ψ–Γ functional.
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