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May 25, 20260 citationsOpen Access

Inhomogeneous Dark Energy: How the Mainstream Closes Its Eyes to Reality and Falls Face-First into "Viscosity"

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ASAlexander Shlyapik

Key Points

  • This research aims to challenge the traditional view of dark energy by investigating its inhomogeneous nature and the effects on cosmic expansion.
  • Analyzed 2025 DESI data to identify changes in the dark energy equation of state w(z).
  • Explored the relationship between dark energy density and baryonic matter distribution according to the Fermionic Universe Hypothesis.
  • Demonstrated that the equation of state w varies over time and differs significantly in cosmic voids compared to galaxy clusters.
  • Explained the observed dipole anisotropy of H0 without requiring additional physics.

Abstract

The 2025 DESI data have definitively buried the myth of the cosmological constant Λ, recognizing the dynamics of the dark energy equation of state w(z). However, the mainstream continues to frantically cling to the dogma of spatial homogeneity, ignoring the obvious anisotropy of the Universe’s expansion. Within the framework of the Fermionic Universe Hypothesis (FUH), it is demonstrated that dark energy is a phase state of the viscous ψ-condensate (the Ocean), the density of which directly depends on the distribution of baryonic matter. We prove that w not only changes with time but also radically differs inside voids and within galaxy clusters, which explains the dipole anisotropy of H0 without invoking ”new physics”.

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Cite This Study

Alexander Shlyapik (2026) studied this question.

synapsesocial.com/papers/6a13e8d20e02ee3982d3365fhttps://doi.org/10.5281/zenodo.20355576
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