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May 8, 20260 citationsOpen Access

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

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MSMyron C. Schoenfelder

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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Cite This Study

Myron C. Schoenfelder (2026) studied this question.

synapsesocial.com/papers/69fd7f0dbfa21ec5bbf0763bhttps://doi.org/10.5281/zenodo.20045078
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