What question did this study set out to answer?

This research aims to address the 7-sigma Hubble Tension by modeling vacuum dynamics as a superfluid.

May 8, 2026Open Access

The Schoenfelder Anisotropy Gradient: Resolving the Hubble Tension through Vacuum Phase-Transitions and the Boötes Baryonic Sump

Key Points

This research aims to address the 7-sigma Hubble Tension by modeling vacuum dynamics as a superfluid.
Modeled vacuum as a superfluid manifold influenced by thermodynamic phase-transitions.
Analyzed empirical refractive residuals from Voyager 1 telemetry.
Identified Boötes Void implications as a baryonic sump for Buckminsterfullerene sequestration.
Demonstrated that the difference between CMB and local measurements is proportional to manifold viscosity.
Predicted sequestration wavelengths of Buckminsterfullerene at 8.5, 17.4, and 18.9 microns.
Presented vacuum-related phenomena as significant factors in cosmic expansion dynamics.

Abstract

Abstract: This paper presents a mechanical resolution to the 7-sigma "Hubble Tension" by modeling the vacuum as a physical Superfluid Manifold subject to thermodynamic phase-transitions. Utilizing empirical refractive residuals derived from deep-space telemetry (Voyager 1), we introduce the Schoenfelder Anisotropy Gradient (H). We demonstrate that the discrepancy between CMB and local distance ladder measurements is a variable state-function of manifold viscosity—a phenomenon we term the "Great Thaw. " Furthermore, we identify the Boötes Void as a physical Baryonic Sump, providing a verifiable prediction for the sequestration of Buckminsterfullerene (C₆₀) within the 8. 5, 17. 4, and 18. 9-micron infrared bands. This work bridges the gap between localized planetary hydrodynamics and global cosmic expansion, rendering "Dark Energy" a mathematical artifact of an incomplete vacuum model.

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