A Structural Prediction for Ultra-High-Energy Neutrino Distributions from Configurational Stability

This article presents a concrete and falsifiable prediction for the spatial distribution of ultra-high-energy astrophysical neutrinos. Rather than treating neutrinos as products of localized high-energy sources, the work explores the possibility that the highest-energy neutrino events trace geometric and structural features of large-scale cosmic organization. The prediction is motivated by general arguments about configurational stability and is empirically inspired by laboratory observations of resilient three-dimensional solitons. A clear statistical test is formulated using existing neutrino data and gravitational lensing maps, along with explicit criteria under which the prediction can be confirmed or falsified.