Mechanical Resolution of the Hubble Tension: Calculating the Yield Duration
Defines the temporal interval required for the vacuum to re-harden after a metric slip, calculated as the ratio of vacuum viscosity to Planck-normalized yield stress. Matches the calculated re-hardening duration to the decay profile of the Fermi-GBM event bn180528465, providing a "Mechanical Signature" for localized metric instabilities.
Authors
- Max Buquoi
Institutions
- Yield10 Bioscience (United States) (US)
Publication Details
- Journal
- Zenodo (CERN European Organization for Nuclear Research)
- Published
- 2026-03-05
- DOI
- https://doi.org/10.5281/zenodo.18879447
- Primary Topic
- Cosmology and Gravitation Theories
- Type
- article
- Field-Weighted Citation Impact
- 0.00