  We find that the amplitude of quantum fluctuations of the invariant de Sitter
vacuum coincides exactly with that of the vacuum of a comoving observer for a
massless scalar (inflaton) field. We propose redefining the actual physical
power spectrum as the difference between the amplitudes of the above vacua. An
inertial particle detector continues to observe the Gibbons-Hawking
temperature. However, although the resulting power spectrum is still
scale-free, its amplitude can be drastically reduced since now, instead of the
Hubble's scale at the inflationary period, it is determined by the square of
the mass of the inflaton fluctuation field.
