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Preprint . 2026
License: CC BY
Data sources: Datacite
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Preprint . 2026
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Preprint . 2026
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Preprint . 2026
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Preprint . 2026
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Preprint . 2026
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Preprint . 2026
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ZENODO
Preprint . 2026
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Kinematic Constraints at Radiative Boundaries: A Geometric Normalization for the Dark Sector

Authors: Bashan, Nadav;

Kinematic Constraints at Radiative Boundaries: A Geometric Normalization for the Dark Sector

Abstract

Physics currently treats the vacuum catastrophe, dark energy, and the Hubble tension as distinct crises. We propose they are symptoms of a single dimensional category error: modeling macroscopic expansion as a 3D bulk fluid rather than a 2D boundary tension. Evaluating equilibrium at radiative decoupling surfaces causes explicit mass dependence to cancel, yielding a purely geometric invariant: pi^3/15 ≈ 2.0671. Projecting this limit to the cosmic horizon gives the observed dark energy fraction, Omega_Lambda = pi^3/45 ≈ 0.6890, without tunable parameters. This predicts the acceleration onset, relaxes early dark matter requirements, and reframes the Hubble tension as geometry. Area-governs-volume is established in black holes and quantum boundary potentials; the universe may follow the same rule.

Keywords

cosmology --- dark energy --- dark matter --- gravitation --- early universe --- galaxies: high-redshift

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selected citations
These citations are derived from selected sources.
This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Citations provided by BIP!
popularity
This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network.
BIP!Popularity provided by BIP!
influence
This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Influence provided by BIP!
impulse
This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network.
BIP!Impulse provided by BIP!
0
Average
Average
Average
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