  I show that the mutual consistency of the Bekenstein Bound, the Standard
Model (SM) of particle physics, and general relativity implies that the
universe began in a unique state. I solve the coupled EYM equations for this
unique state, show how the horizon problem is solved, and how SM baryogenesis
naturally results from the triangle anomoly. Since the SU(2) winding number
state is thus non-zero, the universe is not in the QCD ground state, and this
plausibly yields a (small) positive cosmological constant. Since the initial
state is unique, it is necessarily homogeneous and isotropic, as required by
the Bekenstein Bound. Wheeler-DeWitt quantization implies an $S^3$ cosmology
must be very close to flat if the universe is to be classical today. I show
that the spectrum of any classical gauge field (or interacting massless scalar
field) in a FRW universe necessarily obeys the Wien displacement law and the
corresponding quantized field the Planck distribution law with the reciprocal
of the scale factor playing the role of temperature, even if the fields have
zero temperature. Thus the CBR could even today be a pure SU(2) electroweak
field at zero temperature coupled to the Higgs field, in spite of early
universe inverse double Compton and thermal bremsstrahlung.Such a CBR would not
couple to right-handed electrons, and this property can be detected with a
Penning trap or even using the late 1960's CBR detector with appropriate
filters. I argue that ultrahigh energy (UHE) Genesisf.tex Genesisf.tex cosmic
ray protons would not produce pions by interacting with such a CBR, and thus
the existence of such protons may constitute an observation of this CBR
property.
