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September 17, 2025Open Access

Scale-Invariant Cosmological Models: Resolution of the Hubble Tension, the S8 Tension, and Decreasing Dark Energy Density

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JHJohn Henderson

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Overview

New scale-invariant models resolve hubble and s8 tensions in cosmology, suggesting time-varying dark energy dynamics.

Key Points

  • A scale-invariant cosmological model effectively resolves the hubble tension and s8 tension observed in current data.
  • Recent DESI measurements indicate a preference for time-varying dark energy, as opposed to the constant lambda-cdm model.
  • This model predicts a decrease in dark energy density while conserving energy over time and maintaining physical laws.
  • It further elucidates features of early galaxies observed by JWST, showcasing a ~10% correction to the lambda-cdm framework.

Cite This Study

John Henderson (2025) studied this question.

synapsesocial.com/papers/68d45e6a31b076d99fa5eee9https://doi.org/10.20944/preprints202509.1163.v1
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