Galactic Gravitational Field Measurements Part 3: Galaxy Clusters

Read the full article See related articles

Listed in

This article is not in any list yet, why not save it to one of your lists.
Log in to save this article

Abstract

This paper extends to Part 3 of the Galactic Gravitational field Measurements, to the scale of galaxy clusters, demonstrating how energy dynamics within the auxiliary modulation coordinate explain cluster-scale gravitational phenomena without invoking dark matter.We analyze the Intracluster Medium (ICM) as a primary carrier of energy flow, showing that it accounts for 80-90 percent of the baryonic energy contribution to space-time curvature in clusters. Our mathematical model reveals how energy propagates through cluster volumes via a “bubble-within-bubble” architecture, with individual galactic energy structures nested within the larger ICM energy field.Using entropy-resolved resonance profile principles, we calculate energy density distributions, space-time curvature, and gravitational lensing effects across cluster scales. We provide a detailed case study of the Bullet Cluster, demonstrating how our framework explains the observed separation between X-ray emitting gas and gravitational lensing centers through differential energy flow dynamics in the auxiliary modulation coordinate.The framework accurately predicts cluster-scale phenomena including weak and strong gravitational lensing, X-ray emissions, and velocity dispersions of member galaxies. Our findings reveal that galaxy clusters represent cosmic-scale energy processing networks, with supermassive black holes providing localized energy injection that sustains global cluster dynamics through the auxiliary modulation coordinate dimension.

Article activity feed