  We prove that the primordial black holes in the early universe did not decay
until the gravity decoupled from the other interactions. Rabinowitz' two
objections to the formation of Holeums are shown to be inapplicable. We show
that primordial black holes having masses beween 8x10^18 GeV and 10^19 GeV
formed gravitational bound states called Holeums when the temperature of the
universe was between 10^30 K and 10^29 K. We prove that the black holes in a
fire ball produced in an accelerator such as the LHC, modified into an inertial
confinement type set up, will not emit Hawking radiation as long as the fire
ball is maintained in thermal equilibrium or is allowed to expand
adiabatically.
