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This research aims to introduce Scale Space as a distinct cosmological model while analyzing its implications for FLRW consistency diagnostics.

May 29, 2026Open Access

Paper 24: Scale-Space Signatures in FLRW Consistency Diagnostics: A Third Class of Cosmological Model

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Randomized trial reveals new cosmological model discrepancies in FLRW consistency diagnostics, indicating distinct behaviors.

This research aims to introduce Scale Space as a distinct cosmological model while analyzing its implications for FLRW consistency diagnostics.
Developed a five-dimensional metric with AdS4 geometry incorporating scale-direction momentum.
Derived null geodesic equations and closed-form solution for scale drift effect on observed redshift.
Analyzed FLRW consistency corrections and their polynomial relationships with redshift (u = ln(1 + z)).
Established that the ratio d^SS A /d^FLRW A (zobs) differs, showing scale drift dependence with β^2 s = α^2H^2L^2.
Identified FLRW consistency corrections ∆O > 0, ∆C < 0, and ∆A > 0 with robust functional predictions.
Asserted that for observational viability, β^2 s must be much smaller than 1, linked to undetermined cosmological parameter α.

Donald G Palmer (2026) studied this question.

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May 29, 2026Open Access

View Full Paper

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Authors

Randomized trial reveals new cosmological model discrepancies in FLRW consistency diagnostics, indicating distinct behaviors.

This research aims to introduce Scale Space as a distinct cosmological model while analyzing its implications for FLRW consistency diagnostics.
Developed a five-dimensional metric with AdS4 geometry incorporating scale-direction momentum.
Derived null geodesic equations and closed-form solution for scale drift effect on observed redshift.
Analyzed FLRW consistency corrections and their polynomial relationships with redshift (u = ln(1 + z)).
Established that the ratio d^SS A /d^FLRW A (zobs) differs, showing scale drift dependence with β^2 s = α^2H^2L^2.
Identified FLRW consistency corrections ∆O > 0, ∆C < 0, and ∆A > 0 with robust functional predictions.
Asserted that for observational viability, β^2 s must be much smaller than 1, linked to undetermined cosmological parameter α.

Donald G Palmer (2026) studied this question.

View Full Paper

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