A Holographic Information-Damping Model for Dark Energy Evolution: Resolving the 10^120 Discrepancy and Hubble Tension

This research introduces the "L-Law," a groundbreaking information-theoretic framework to address the cosmological constant problem and the 10^{120} vacuum energy discrepancy. By treating the universe as a holographic processing system, we derive a dynamic vacuum energy density \rho_{\Lambda}(a) that undergoes exponential damping as a function of cosmic information growth S_{BH}.

Authors

Publication Details

Journal
Zenodo (CERN European Organization for Nuclear Research)
Published
2026-04-02
DOI
https://doi.org/10.5281/zenodo.19388888
Primary Topic
Cosmology and Gravitation Theories
Type
article
Field-Weighted Citation Impact
0.00
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article

A Holographic Information-Damping Model for Dark Energy Evolution: Resolving the 10^120 Discrepancy and Hubble Tension

Ahmed Mohammed
Zenodo (CERN European Organization for Nuclear Research)
Cosmology and Gravitation Theories
article

A Holographic Information-Damping Model for Dark Energy Evolution: Resolving the 10^120 Discrepancy and Hubble Tension

Ahmed Mohammed
article en

Abstract

This research introduces the "L-Law," a groundbreaking information-theoretic framework to address the cosmological constant problem and the 10^{120} vacuum energy discrepancy. By treating the universe as a holographic processing system, we derive a dynamic vacuum energy density \rho_{\Lambda}(a) that undergoes exponential damping as a function of cosmic information growth S_{BH}.

Zenodo (CERN European Organization for Nuclear Research)
Affordable and clean energy
Openalex Percentile: Top 5%
Cosmology and Gravitation Theories
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A Holographic Information-Damping Model for Dark Energy Evolution: Resolving the 10^120 Discrepancy and Hubble Tension — Ahmed Mohammed · Zenodo (CERN European Organization for Nuclear Research) (2026) | TGRS Research Map | TGRS