Shockwaves of Galactic Clusters and Implications of the Microcosm and Macrocosm Interrelationship

 I have repeatedly brought attention to the seminal work of Bernard Riemann on the principle of shockwave propagation. Keeping in mind his insistence as well that the physical geometry outside the range of our limited human or better yet perhaps mammalian perceptions may bring into play the alternative curvatures of of non-Euclidean "space." 

In this regard, the discovery of the presence of shockwave formations of merging galaxy clusters in the radio wave spectrum as so called radio relics is very important research for moving the frontiers of scientific progress forward. This is especially due to their almost unimaginably vast structure at the same time propelling the very smallest particles' acceleration to relativistic speed of light velocities.

 This is the indissoluble connection that is always apparent of the macrocosm with the microcosm as Nicholas of Cusa demonstrated in his "triune" principle. The very large and the very small macrocosm/microcosm connectedness as an analogue of the human relationship of the universal creator with the individual person via creative reason, in non religious terms.

The curvature as the shockwave front nears the limit of transmissibility for the medium of electromagnetic propagation proceeds naturally from a positive spheroid type to a negative horn. Indeed, Riemann is again proven correct that the physical system precedes choice of mathematical geometry. The various types of further such potential particle accelerations and scatterings, etc. are the platform upon which we can be confident scientific progress accruing to the future benefit of humanity will necessarily proceed as both Riemann and Cusa would surely agree. 

MeerKAT radio contours (magenta) on A2384 XMM-Newton image. Credit: Parekh et al., 2020

" The origin of the radio relic is puzzling.(...) This radio relic could be the result of shock wave propagation during the passage of the low-mass A2384(S) cluster through the massive A2384(N) cluster, creating a trail appearing as a hot X-ray filament." V. Parekh, et al.: https://arxiv.org/abs/2009.02724