Acoustic Wave Expansion in the Cosmic Bulk: A Parametric Fit for DESI 2024 and Turnaround Predictions for Euclid
The standard cosmological model assumes a constant dark energy density, yet recent DESI 2024 measurements suggest a dynamic parameter. We propose that the dark energy tension is physically resolved by modeling cosmic expansion as a macroscopic acoustic wave resonating within a higher-dimensional bulk.Formal Verification & Source Code: The rigorous Lean 4 proofs and framework codebase are open-source and available at the Ouroboros GitHub Repository.
Authors
- Bruno Luçardo Olivaes
Institutions
- Universidad de Matamoros (MX)
Publication Details
- Journal
- Zenodo (CERN European Organization for Nuclear Research)
- Published
- 2026-07-23
- DOI
- https://doi.org/10.5281/zenodo.21516848
- Primary Topic
- Cosmology and Gravitation Theories
- Type
- article
- Field-Weighted Citation Impact
- 0.00