Joined: Fri Jan 06, 2012 9:14 pm +0000
Posts: 189
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Hi nodAmanaV,
I approach black holes with a question: what happens when you try to squeeze all the space out of a big ball of matter?
Native astrophysics has worked out how medium sized stars can cool and contract to become white dwarfs, and how larger stars can collapse as neutron stars. But the fun begins when a neutron star, in a binary system, with an accretion disk, pulls in a little bit too much mass, and starts to collapse.
See this YouTube video (or this pdf script) for what I believe happens next.
The idea is that if a dark island accumulates enough mass for its self-gravity to force the ultimatons in its collapsed matter to come too close together, the "mother of all exclusion principles" kicks in. I think this is what the UB means by "the limiting and critical explosion point of ultimatonic condensation" (see 41:3.6 and 41:7.15).
But if dark islands explode upon reaching a certain mass, then we face the question: what are the supermassive objects that appear to anchor galaxies? My first thought is that they are some kind of (absonite?) artifact left by the perpendicular departure of the Associate Transcendental Master Force Organizer who spun up that system of stars. Maybe something like the belts of dark gravity bodies surrounding Havona?
Fun to speculate!
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