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.

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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
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article

Acoustic Wave Expansion in the Cosmic Bulk: A Parametric Fit for DESI 2024 and Turnaround Predictions for Euclid

Bruno Luçardo Olivaes
Zenodo (CERN European Organization for Nuclear Research)
Cosmology and Gravitation Theories
article

Acoustic Wave Expansion in the Cosmic Bulk: A Parametric Fit for DESI 2024 and Turnaround Predictions for Euclid

Bruno Luçardo Olivaes
article en

Abstract

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.

Zenodo (CERN European Organization for Nuclear Research)
Universidad de Matamoros (MX)
Affordable and clean energy
Openalex Percentile: Top 9%
Cosmology and Gravitation Theories
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Acoustic Wave Expansion in the Cosmic Bulk: A Parametric Fit for DESI 2024 and Turnaround Predictions for Euclid — Bruno Luçardo Olivaes · Zenodo (CERN European Organization for Nuclear Research) (2026) | TGRS Research Map | TGRS