Dynamical Resolution of the Hubble Tension via Generalized Chaplygin Gas Phase Transitions and Elastomeric Brane Topologies

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.

Authors

Publication Details

Journal
Zenodo (CERN European Organization for Nuclear Research)
Published
2026-06-28
DOI
https://doi.org/10.5281/zenodo.20997125
Primary Topic
Cosmology and Gravitation Theories
Type
preprint
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preprint

Dynamical Resolution of the Hubble Tension via Generalized Chaplygin Gas Phase Transitions and Elastomeric Brane Topologies

Mario Lucas Ota
Zenodo (CERN European Organization for Nuclear Research)
Cosmology and Gravitation Theories
preprint

Dynamical Resolution of the Hubble Tension via Generalized Chaplygin Gas Phase Transitions and Elastomeric Brane Topologies

Mario Lucas Ota
preprint en

Abstract

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.

Zenodo (CERN European Organization for Nuclear Research)
Cosmology and Gravitation Theories
DOIOpen Access PDFOpenAlex
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Dynamical Resolution of the Hubble Tension via Generalized Chaplygin Gas Phase Transitions and Elastomeric Brane Topologies — Mario Lucas Ota · Zenodo (CERN European Organization for Nuclear Research) (2026) | TGRS Research Map | TGRS