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April 1, 2026Open Access

Infrared Observational Evidence for Non-Local Cosmic Dynamics: A Model-Independent Closure Test from Expansion Data

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Authors

FCFernando Cesar Coelho Coutinho

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Overview

Model-independent observations reveal non-local dynamics in cosmic expansion, suggesting deeper organizing principles.

Key Points

  • This work investigates whether cosmic expansion can be modeled as a local process or requires a non-local structure.
  • Constructed a dimensionless observable R(u) to assess dynamical closure.
  • Utilized Cosmic Chronometers, Pantheon+ supernovae, and DESI DR1 BAO data for evaluations.
  • Employed a robustness-controlled protocol for data reconstruction and analysis.
  • R(u) shows significant deviations from constant values, indicating non-local dynamics.
  • Analysis supports the existence of memory-dependent structures in cosmic expansion.
  • Findings align with a new framework suggesting cosmic acceleration as an entropic relaxation process.

Cite This Study

Fernando Cesar Coelho Coutinho (2026) studied this question.

synapsesocial.com/papers/69ccb7b016edfba7beb89bcdhttps://doi.org/10.5281/zenodo.19338600
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