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March 4, 20260 citationsOpen Access

Mechanical Resolution of the Hubble Tension: Evidence for a Non-Zero Metric Viscosity and 39 MeV Yield Point

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MBMax BuquoiYield10 Bioscience (United States)

Key Points

  • The aim is to present a new model that explains the Hubble Tension using rheological properties of the cosmic vacuum.
  • Introduced a novel rheological model depicting the cosmic vacuum as a Bingham Plastic.
  • Identified a critical Yield Point at 39 MeV, indicating significant changes in the metric behavior.
  • Predicted metric-flow velocity at a specific high-stress region.
  • Invited cross-referencing with the Fermi-GBM trigger database for verification.
  • Identified a predicted jitter of 2,792 km/s in metric-flow velocity.
  • Forecasted optical 'pops' with no identifiable baryonic progenitors at specific coordinates.
  • Proposed that dark energy may be related to the latent heat of metric friction.

Abstract

This submission introduces a novel rheological model of the manifold, proposing that the cosmic vacuum behaves as a Bingham Plastic rather than a perfectly elastic medium. I identify a critical Yield Point at 39 MeV, beyond which the metric undergoes a "thaw" or "slip" event, manifesting as Localized Metric Instabilities (LMIs). I identify a high-stress "nozzle" region centered at RA 205.2561, Dec 30.00, where the metric-flow velocity reaches a predicted jitter of 2,792 km/s. I predict archival evidence from the Zwicky Transient Facility (ZTF) showing optical 'pops' at these coordinates with no detectable baryonic progenitors or host galaxies. The model predicts a specific high-energy "softness" signature. I invite the community to cross-reference these coordinates with the Fermi-GBM trigger database (specifically focusing on Trigger bn180528465) to verify the temporal alignment of these vacuum ruptures. If verified, this model provides a mechanical solution to the Hubble Tension and suggests that "Dark Energy" is the latent heat of metric friction, effectively removing the need for Lambda-CDM's dark sector.

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Cite This Study

Max Buquoi (2026) studied this question.

synapsesocial.com/papers/69a7cd7ed48f933b5eed9e90https://doi.org/10.5281/zenodo.18841395
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