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A Common Dark-Matter Q-Field Background in Spacetime Ladder Theory: Explaining Five Particle Anomalies via the Jupiter Perihelion–La Niña Window and Predicting the Next One

Year: 2026
Type: preprint
Abstract: We examine five persistent particle-physics anomalies—the W-boson mass shift, the muon anomalous magnetic moment , the cross-section tension, the angular-distribution anomaly, and the LZ 248 keV nuclear-recoil candidate—by binning the existing local data according to the overlapping “Jupiter perihelion + La Niña” window rather than by multi-year cumulative averages. In every case the identifiable anomalous interval falls inside or immediately adjacent to this astronomical–climatic window. Within the Spacetime Ladder Theory (STLT) these five signals are interpreted as phenomenological manifestations of a single, spatially extended dark-matter background field—the unified energy-field / Q-field ground state—whose local strength is modulated by solar-system polarization (quantified by the Life-Space and Time-Initial Value, LSI) and by the global climate phase (ENSO). The Standard Model, having assigned dark matter no dynamical role, necessarily registers the modulation as unexplained residuals. The present work is explicitly phenomenological: it establishes a temporal correlation and advances a common-background-field hypothesis, but does not yet derive the five anomalies from a completed action principle. Its principal scientific value lies in its sharp, pre-registered falsifiability. Precision measurements performed during the next well-defined Jupiter-perihelion–La Niña overlap window will constitute an independent, decisive test of the proposed Q-field background. Confirmation would elevate the correlation to a predictive success of STLT; absence of the predicted enhancements would falsify the present phenomenological claim cleanly.
DOI: 10.5281/zenodo.23786030
Language: English
Open Access status: green
OpenAlex ID: W7224790738
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