CDN-292: The Rheology Wall

CDN-292 formalizes the GCFT high-drive Xi-field rheology wall. The dynamic channel remains first-order Doppler-linear at low radial drive, enters a nonlinear dissipative transition near D_Xi = |v_r|/v_star with v_star = 0.15 c_Xi, and freezes out at high drive. For the CDN-274 reference scale c_Xi = 900 km/s, the wall sits at v_star = 135 km/s, with the inferred window range 97.5-174 km/s for c_Xi = 650-1160 km/s. The claim is explicitly bounded: this is a subluminal coherence-response boundary, not a derivation of the special-relativistic speed limit, not faster-than-light transport, and not a replacement for c.

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Publication Details

Journal
Zenodo (CERN European Organization for Nuclear Research)
Published
2026-06-18
DOI
https://doi.org/10.5281/zenodo.20740449
Primary Topic
Pulsars and Gravitational Waves Research
Type
article
Field-Weighted Citation Impact
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article

CDN-292: The Rheology Wall

Nicky Joseph Hubertus Catharina Hacquier
Zenodo (CERN European Organization for Nuclear Research)
Pulsars and Gravitational Waves Research
article

CDN-292: The Rheology Wall

Nicky Joseph Hubertus Catharina Hacquier
article en

Abstract

CDN-292 formalizes the GCFT high-drive Xi-field rheology wall. The dynamic channel remains first-order Doppler-linear at low radial drive, enters a nonlinear dissipative transition near D_Xi = |v_r|/v_star with v_star = 0.15 c_Xi, and freezes out at high drive. For the CDN-274 reference scale c_Xi = 900 km/s, the wall sits at v_star = 135 km/s, with the inferred window range 97.5-174 km/s for c_Xi = 650-1160 km/s. The claim is explicitly bounded: this is a subluminal coherence-response boundary, not a derivation of the special-relativistic speed limit, not faster-than-light transport, and not a replacement for c.

Zenodo (CERN European Organization for Nuclear Research)
Dynamique du noyau (FR)
Openalex Percentile: Top 6%
Pulsars and Gravitational Waves Research
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