Early Super Massive Black Holes

The superluminal collision thermalized the overlap volume into a pre-baryonic plasma at temperatures far above the electroweak scale — a regime where the Standard Model particles as we know them did not yet exist as discrete entities. Angular momentum inheritance from the collision geometry immediately imposed density gradients across this plasma: regions corresponding to the highest-density angular momentum strata swirled inward, compressing their centers through ram pressure and gravitational focusing. In the most overdense nodes, the enclosed stress-energy crossed the Schwarzschild threshold before the plasma had cooled through the QCD transition. These regions underwent direct gravitational collapse into black holes without ever passing through a stellar phase — the first SMBHs were not grown from seeds, they were the seeds, formed from pre-baryonic plasma during the thermalization cooling epoch itself.

This mechanism operates entirely within established GR and the SCT collision framework and requires no new physics. The Schwarzschild radius is a function of enclosed mass-energy, not of the state of matter — it applies equally to plasma, quarks, and baryons. As the overdense plasma nodes collapsed, the quark degeneracy pressure mechanism in SCT set the interior structure, preventing true singularities and establishing finite-density cores, while the surrounding cooling plasma was left to recombine into the baryonic matter that would eventually form the host galaxy around the already-formed black hole. The SMBH did not form inside a galaxy; the galaxy formed around the SMBH, organized by the same inherited angular momentum field that concentrated the plasma in the first place.

The pre-existing compact objects and stellar populations inherited from the two colliding pockets add a further contribution: SMBHs that had already assembled through prior stellar evolution in those pockets arrived in the debris field already massive, providing a second population of early SMBHs alongside the direct-collapse objects formed within our own post-collision cooling epoch. Together, these two channels — direct plasma collapse and inherited prior-epoch SMBHs — produce the observed abundance and mass distribution of early supermassive black holes at z > 6 without requiring any period of sustained super-Eddington accretion from stellar-mass seeds.