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The study aims to understand how quantum correlations are transferred during cosmological expansion and its impact on dark energy.

April 5, 2026Open Access

Correlation Transfer, the Direction of Information Flow, and the Dark Energy Fraction

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The study aims to understand how quantum correlations are transferred during cosmological expansion and its impact on dark energy.
Proposes a model of quantum correlations during both accelerating and decelerating expansion.
Analyzes the implications of Landauer's principle on energy density at the cosmological horizon.
Utilizes standard horizon thermodynamics to connect energy densities to cosmic parameters.
Establishes a parameter-free prediction for dark energy density as Ω_Λ = ln 2.
Finds consistency with Planck 2018 dark energy measurements.
Identifies a self-consistency constraint affecting the relationship between energy density and the Friedmann equation.

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This research explores information flow during cosmic expansion, revealing implications for dark energy dominance.

Scott Weller (2026) studied this question.

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