preprintZenodo (CERN European Organization for Nuclear Research)Jan 2, 2026GREEN OA

Deriving the Galaxy Cluster MOND Enhancement from 7D Vlasov Dispersion

MHMartin Helmut Schrotz
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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.

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Topics & keywords

Topics
Keywords
  • Cluster (spacecraft)
  • Galaxy cluster
  • Galaxy
  • Velocity dispersion
  • Offset (computer science)
  • Brightest cluster galaxy
  • Anisotropy
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