Study models cosmic expansion dynamics in dark energy, suggesting new implications for cosmology.
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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Bruno Luçardo Olivaes (2026) studied this question.
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