  The present day mass spectrum for dark matter compact objects is calculated
based on the assumption that a uniform population of PBHs was created at a
definite red-shift, and that the mass spectrum evolved as a result of
gravitational radiation. The predicted present day spectrum extends over many
decades of mass and allows one to connect the abundance of MACHOs in the halo
of our galaxy with the abundance of galactic seeds. Present day astrophysical
constraints on the abundance of dark matter PBHs appear to be consistent with
our predicted mass spectrum if it is assumed that the seeds for the present day
dark matter MACHOs were created at a time ~ 10-4 second after the big bang.
Remarkably the total cosmological energy density at this time obtained by
extrapolating the sum of the present day dark matter and CMB energies backward
in time is very close to the mass-energy density of an Einstein-de Sitter
universe at the same time. This suggests that the radiation precursor to the
CMB was created at about the same time as the seeds for the present day dark
matter.
