Images:
Note iron (Fe, Z=26) undergoes
endothermic
nuclear burning
NOT
exothermic
nuclear burning.
So trying to burn
iron cools the
iron core.
At this point, electrons
in the iron core
find it energetically favorable to
very rapidly bind with the protons
(of the iron nuclei)
via electron capture (p+e(-)→n+μ_e)
to create neutrons.
The rapid disappearance of the
electrons
and their
degenerate electron gas pressure
leads to an
implosion.
The implosion
turns into an
explosion
because the creation of
the neutrons releases
neutrinos
(specifically electron neutrinos
which in this dense environment do interact significantly with
matter)
which push outward the outer layers of the
star.
The explosion is a, in fact,
core collapse supernova.