New Approach to Cosmological Fluctuation Using the Background Field Method and CMB Power Spectrum

Abstract

A new field theory formulation is presented for the analysis of the CMB power spectrum distribution in the cosmology. The background-field formalism is fully used. Stimulated by the recent idea of the emergent gravity, the gravitational (metric) field gμν is not taken as the quantum-field, but as the background field. The statistical fluctuation effect of the metric field is taken into account by the path (hyper-surface)-integral over the space-time. Using a simple scalar model on the curved (dS4) space-time, we explain the above things with the following additional points: 1) Clear separate treatment of the classical effect, the statistical effect and the quantum effect; 2) The cosmological fluctuation comes not from the ’quantum’ gravity but from the unkown ’microscopic’ movement; 3) IR parameter (`) is introduced for the time axis as the periodicity. Time reversal(Z2)-symmetry is introduced in order to treat the problem separately with respect to the Z2 parity. This procedure much helps both UV and IR regularization to work well.