  We investigate the issue of initial conditions of curvature and tensor
perturba- tions at the beginning of slow roll inflation and their effect on the
power spectra. Renormalizability and small back reaction constrain the high k
behavior of the Bogoliubov coefficients that define these initial conditions.We
introduce a transfer function D(k) which encodes the effect of generic initial
conditions on the power spectra. The constraint from renormalizability and
small back reaction entails that D(k) < mu^2/k^2 for large k, implying that
observable effects from initial conditions are more prominent in the low
multipoles. This behavior affects the CMB quadrupole by the observed amount
\~10-20% when mu is of the order of the energy scale of inflation. The effects
on high l-multipoles are suppressed by a factor ~1/l^2 due to the fall off of
D(k) for large wavevectors k. We show that the determination of generic initial
conditions for the fluc- tuations is equivalent to the scattering problem by a
potential V(eta) localized just prior to the slow roll stage. Such potential
leads to a transfer function D(k) which automatically obeys the
renormalizability and small backreaction constraints. We find that an
attractive potential V(eta) yields a suppression of the lower CMB
multipoles.Both for curvature and tensor modes, the quadrupole suppression
depends only on the energy scale of V(eta) and on the time interval where
V(eta) is nonzero. A suppression of the quadrupole for curvature pertur-
bations consistent with the data is obtained when the scale of the potential is
of the order of k^2_Q where k_Q is the wavevector whose physical wavelength is
the Hubble radius today.
