Published May 26, 2026 | Version v2

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

Contributors

Description

The Scale Space framework treats logarithmic scale as a genuine fourth spatial coordinate, producing a five-dimensional metric with AdS4 geometry in which matter geodesics include a scale-direction component. A photon propagating through this geometry acquires a scale-direction momentum (scale drift) generated by the Christoffel coupling Γ^s xx, even when emitted with zero scale velocity. This modifies the angular diameter distance dA(z) and therefore all FLRW-consistency diagnostics. We derive the null geodesic equations, obtain the closed-form analytic solution for the scale drift, compute the observed redshift from the matter congruence, and prove an exact algebraic theorem: the ratio d^SS A /d^FLRW A (zobs) = sqrt[1 +β^2 s], where β^2 s = α^2H^2L^2 is the dimensionless scale kinetic energy of co-moving matter. This ratio is proved invariant under any constant-F correction to gtt. The resulting FLRW consistency corrections are ∆O > 0 (apparent spatial openness), ∆C < 0 (CBL test violation), and ∆A > 0 (KSS eff < 0, open-curvature-like), all organising naturally as polynomials in u = ln(1 + z) rather than power laws in (1+ z). This log-scale functional form distinguishes Scale Space as a third class of cosmological model in the Heinesen–Clifton taxonomy, alongside but distinct from Dyer–Roeder optical effects and Buchert backreaction. With the local gravity parameter identification β2 s = 8, the corrections are observationally too large; quantitative viability requires β2 s ≪ 1, which depends on the cosmological value of α not yet determined by the current framework. The qualitative signatures and the log-scale functional form are robust predictions
of the toy model.

Other

The mathematical development in this paper was produced in dialogue with Claude.ai (Anthropic) in Spring 2026, directed by the author. Use of AI assistance is acknowledged in accordance with standard scholarly practice.

Files

paper24_flrw_diagnostics_v1.pdf

Files (380.3 kB)

Name Size Download all
md5:dd7b73e7981cd58cf0d29a90fa259392
292.3 kB Preview Download
md5:f4f783af7e5b24a4ad46a7645c3819a8
17.6 kB Preview Download
md5:37c07ed7d88ab9e11de2e38296eae423
19.9 kB Download
md5:6eb20d8d30a9ffc3e5bab1dae8ed6e69
32.4 kB Preview Download
md5:87882378f782a48b703ecb5d65430517
18.1 kB Preview Download