Explores a dynamic dark fluid model to resolve Hubble tension, suggesting new frameworks for cosmology.
The modern cosmological crisis centered around the Hubble Tension (~67 km/s/Mpc from early-universe CMB vs. ~73 km/s/Mpc from late-time local observations) strongly indicates that the static standard Lambda-CDM model is fundamentally incomplete. We propose a self-consistent framework that resolves this tension by replacing the cosmological constant with a dynamic, unified dark fluid embedded within an elastomeric spacetime brane.
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Mario Lucas Ota (2026) studied this question.
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