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Re: The Dominium Model: Part 2
Move #9
In move #8 it was established that the main matrix of an embryonic galaxy situated near the centers of proto galaxies was compressed into black-hole material forming the AGN. Simultaneously, micelles of antimatter in the same region would also be compressed to black-hole material (AMBH). Together formed the “stable” central galactic supermassive black-holes seen in all galaxies, when AMBH accumulated at the gate-interface of the AGN thereby preventing further accretion. However, the center of the forming galaxy is only a subsection of the overall unit. This move will examine the dynamics of the rest of the proto-galaxies given our working premises.
Near to the center, AMBH could have been formed that was not subsequently dragged to the gate-interface of the forming AGN at the center of the galaxy. However, that is not to say that their presence did not or would not affect the subsequent evolution of the galaxy. Quite the contrary, the presence of these micelles within the main matrix (matter for the Milky Way) of the proto-galaxy would have acted as a physical deterrent acting against further collapse of the galaxy. A good analogy of the affect of opposite-type micellular presence within the main matrix would be comparable to the affects of bubbles of gas within bread-dough. Their presence essentially acts to puff-up the overall loaf.
Another necessary effect of the presence of immiscible micelles of AMBH within the young galaxy would be to act as mini barriers preventing sub-regions from overly coalescing, thereby keeping stars and eventual solar systems “smaller” than they otherwise might have become.
As a result of this, and previous discussions and moves 7 & 8, the current physical layout of our galaxy is categorically achieved: collapsed at the center, the central AGN walled off by the MAC cloud, and while the rest of the galaxy relatively puffed-out and spaced towards the perimeter.
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In comparison to the Universe we are all much more puny and more short-lived than microbes
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