If the mass of a star is sufficiently large, then this implosion produces an enormous heating, which stops only after quark-gluon plasma of a temperature about 100 MeV (or even higher) is formed to withstand the gravitational compression (whereas the highest temperatures of supernovae bursts are, at least, one order lower). As a consequence, a ”burning wall” must be, most probably, erected on the way of further collapsing the matter towards a black hole formation.
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