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New Approach to Cosmological Fluctuation Using the Background Field Method and CMB Power Spectrum
Author(s) -
Shoichi Ichinose
Publication year - 2014
Publication title -
proceedings of the 12th asia pacific physics conference (appc12)
Language(s) - English
Resource type - Conference proceedings
DOI - 10.7566/jpscp.1.013103
Subject(s) - cosmic microwave background , spectral density , field (mathematics) , physics , spectrum (functional analysis) , statistical physics , computer science , mathematics , quantum mechanics , telecommunications , anisotropy , pure mathematics
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 {\it emergent} gravity, the gravitational (metric) field $g_\mn$ 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 (dS$_4$) 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 ($\ell$) is introduced for the time axis as the periodicity. Time reversal(Z$_2$)-symmetry is introduced in order to treat the problem separately with respect to the Z$_2$ parity. This procedure much helps both UV and IR regularization to work well.

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