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... Gravitational pressure "squeezes" the quark-gluon plasma, and the quarks, which have been flowing through the seething array of gluon flux tubes, are "squeezed" out. The matter surrounding the quagma sphere is therefore hit with a pure quark wave. Simultaneously, the gluons are compacted enough to fuse and form a "short-lived" gluon star that will eventually, if it absorbs enough matter, go supernova and leave behind a black hole...
... In some cases, a squark/gluino analog of an atomic-molecular star collides with another dark-matter star at the same point in space as where two baryonic stars are colliding. Though the two regular stars do not interact with the dark-matter stars, their gravitons and gravitinos do. Accordingly, not only do the collisions and accompanying novae generate two separate black holes, but these black holes involve the fusion of gravitons and gravitinos at their core, which creates a small shell of gravitational fusion energy around the absolute core. In other words, the tetra-star collapse compounds the gravitational turbulence that already arises in the case of a regular black hole and generates a supermassive black hole (with an epochal intide (inwave) that draws matter towards the black hole, from the neighboring star systems, over a vast enough space that the SBH quickly absorbs more and more stellar masses within a "short" (let's say 1,000-year period)). [The inwave manages to suck a massive number of neutrinos/sneutrinos into itself, which adds up to a sizable amount of the mass constituency of the initial hole.]
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RETRACTION: I now think that the gluons would get squeezed out of the quark manifold, because the quarks would form a superfoam, and the thermal pressure surrounding the foam manifold would squeeze it like a sponge. So a quark star, albeit small and short-lived, would form at the center of the thermal manifold.
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