Deriving the Galaxy Cluster MOND Enhancement from 7D Vlasov Dispersion

Zenodo (CERN European Organization for Nuclear Research) 2026 Preprint Open access

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Authors: Martin Helmut Schrotz
DOI: 10.5281/zenodo.18135957
Cited by: 4
References: 2

Abstract

Cluster sqrt(3) Enhancement from 7D Vlasov (Version 3) Resolves the "cluster problem" (MOND underpredicts cluster masses by ~1.7x). Extends CGT to 7D with two Planck-scale dimensions. Hot plasma supports collective W-Langmuir modes that activate cross-coupling channels; cold stellar systems do not. Channel counting: 1 direct + 2 cross = 3 channels, giving sqrt(3) = 1.73 enhancement. Validated against X-COP data (7 clusters, mean ratio 0.98 +/- 0.09). Appendix B presents lensing offset mechanism for Bullet-type mergers via anisotropic director field.

Fields of Study & Subjects

Galaxies: Formation Evolution Phenomena Gamma-ray bursts and supernovae Astronomy and Astrophysical Research

Publication details

Journal / source
Zenodo (CERN European Organization for Nuclear Research)
Publication date
2 January 2026
Document type
Preprint