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Preprint . 2026
License: CC BY
Data sources: Datacite
ZENODO
Preprint . 2026
License: CC BY
Data sources: Datacite
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Density-Dependent Length Contraction with Angular Spin Torque

Dichteabhängige Längenkontraktion: Ein Modell mit flachem Raumzeit und expliziten Ableitungen V2
Authors: Karagiannis, Boris;

Density-Dependent Length Contraction with Angular Spin Torque

Abstract

A flat-spacetime scalar model where gravity emerges as radial ruler contraction along the line-of-sight: s = max(1 - κ_eff ∫ ρ ds, 0.01), with κ_eff = 7.39 × 10^5 m² kg^{-1} (Gaia DR3 calibrated) scaling as κ_eff ∝ 1/(1 + ρ/ρ_crit)^2, ρ_crit = 10^{-24} kg m^{-3}. Reproduces Milky Way rotation (220 km/s at 8 kpc → 195 km/s at 30 kpc) without dark matter, LIGO strain via density shear, redshift as λ_obs = λ_0 / s. Includes GPS clock match, proposed muonium lab test (Δf ≈ 10^{-10} Hz at 1 atm), and falsifiable predictions: JWST z>5 SN extra stretch, Swarm SAA cosmic-ray spike, NANOGrav nHz background from density variance. Further, spin (angular momentum L = Iω, ω Planck-scale) introduces angular drag on rulers: length contraction is accompanied by a small twist, without invoking curved spacetime. This torque enhances the squeeze effect while preserving the same density parameter κ = 7.39 × 10⁵ m²/kg, adding realism to the model. All open—no funding. (full txt open bellow no download in need)

Keywords

Radial ruler contraction, Gaia DR3, Flat spacetime gravity, Density gradient, Galactic rotation curves, No dark matter, Redshift mechanism, LIGO strain mimic, Alternative gravity, Density-dependent length contraction

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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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