Structural Closure and the Cosmological Misnomer: Admissibility, Expansion, and the Geometry of Closed Systems

Chast K. Wolfe

doi:10.5281/zenodo.20694803

June 14, 2026Open Access

Structural Closure and the Cosmological Misnomer: Admissibility, Expansion, and the Geometry of Closed Systems

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Key Points

To clarify the distinction between FLRW curvature terminology and structural closure criteria in cosmology.
Aligns the S³ claim with the frame-complete manifold-stage theorem.
Separates local expansion kinematics from curvature-sensitive measures.
Examines implications for FLRW models.
Demonstrates that structural closure is a necessary admissibility condition.
Finds a clear distinction between local expansion kinematics and global curvature measures.

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Implication

The study distinguishes curvature terminology from structural closure, highlighting implications for cosmological models.

Abstract

Distinguishes FLRW open/flat/closed curvature terminology from structural closure as an admissibility condition. Version 3 aligns the S³ claim with the frame-complete manifold-stage theorem and separates local expansion kinematics from curvature-sensitive FLRW distance measures.

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Cite This Study

Chast K. Wolfe (2026) studied this question.

synapsesocial.com/papers/6a323e6ad50b63ecad2079e5 https://doi.org/10.5281/zenodo.20694803

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Structural Closure and the Cosmological Misnomer: Admissibility, Expansion, and the Geometry of Closed Systems

Key Points

Ask about this paper

Implication

Abstract

Discussion

Cite This Study

Structural Closure and the Cosmological Misnomer: Admissibility, Expansion, and the Geometry of Closed Systems

Key Points

Ask about this paper

Implication

Abstract

Discussion

Cite This Study

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