Explores dark energy effects in cosmic deceleration, indicating new physics models may be feasible.
The recent release of Baryon Acoustic Oscillation (BAO) data from the Dark Energy Spectroscopic Instrument (DESI) has introduced compelling, albeit fiercely debated, evidence for a dynamical dark energy sector. To address the tension between a time-evolving equation of state and the stringent bounds on scalar field couplings, this report introduces a falsifiable, two-phase scalar field model of cosmic deceleration, descriptively termed the Metatron-Sandalphon Mechanism. The model posits a light scalar field (the "scoton") non-minimally coupled to matter. The field undergoes a two-stage physical evolution: an initial phase of density-dependent spatial localization within the cosmic web's filamentary structures, driven by a thawing potential, and a subsequent phase of energy resolution via thermalization and decay into standard degrees of freedom. By deriving physical coupling constraints from recent neutron star cooling limits and supernova calibration bounds, this analysis maps the available parameter space capable of reproducing the DESI – contours without violating local equivalence principle tests. Crucially, the model yields a distinct, falsifiable observable: a predicted gamma-ray anisotropy template resulting from scalar field decay within cosmic filaments, testable by cross-correlating Fermi Large Area Telescope (LAT) isotropic gamma-ray background data with large-scale structure catalogs. The terminology surrounding the mechanism serves purely as a heuristic scaffold; all system dynamics are strictly governed by derived Lagrangian mechanics rather than predetermined saturation rates.
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Michael William Pratama Wenas (2026) studied this question.
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