7.2. The inflationary energy scale
The most solid observational result is the interpretation of the cosmic microwave anisotropies seen by COBE as giving the amplitude of the initial power spectrum. COBE is a particularly powerful probe because its large beam size makes it sensitive only to scales much larger than the horizon size when the microwave background formed. The perturbations are therefore seen in their primordial form, and depend only on the initial perturbations and not all the other parameters. (9)
The COBE normalization requires the perturbation at the present Hubble scale, H H(k = a0H0), to be given by [25]
Since
then unless proves to be
tiny (say much less than a hundredth) this will give
at the time when observable scales crossed outside the horizon, pretty
much the scale that particle physicists associate with Grand Unified
Theories.
9 There is a residual dependence on
0 and
which determine the relation
between the metric perturbations
and the matter perturbations, and also the evolution of perturbations,
but that is easily dealt with. I will assume critical density for
simplicity.
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