  We study the inflation process of universe based on the renormalizable
quantum gravity formulated as a conformal field theory (CFT). We show that the
power-law CFT spectrum approaches to that of the Harrison-Zel'dovich-Peebles
type as the amplitude of gravitational potential gradually reduces during the
inflation. The non-Gaussanity parameter is preserved within order of unity due
to the diffeomorphism invariance. Sharp fall-off of the angular power spectrum
of cosmic microwave background (CMB) at large scale is understood as a
consequence of the existence of dynamical scale of the quantum gravity
\Lambda_QG (\simeq 10^{17})GeV. The angular power spectra are computed and
compared with the WMAP5 and ACBAR data with a quality of \chi^2/dof \simeq 1.1.

Cosmology and Nongalactic Astrophysics;General Relativity and Quantum Cosmology;High Energy Physics - Phenomenology;High Energy Physics - Theory