English

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

High Energy Physics - Theory 2013-10-22 v3 General Relativity and Quantum Cosmology

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 {\it emergent} gravity, the gravitational (metric) field g\mng_\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 (dS4_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(Z2_2)-symmetry is introduced in order to treat the problem separately with respect to the Z2_2 parity. This procedure much helps both UV and IR regularization to work well.

Keywords

Cite

@article{arxiv.1308.1163,
  title  = {New Approach to Cosmological Fluctuation using the Background Field Method and CMB Power Spectrum},
  author = {Shoichi Ichinose},
  journal= {arXiv preprint arXiv:1308.1163},
  year   = {2013}
}

Comments

6 pages, 5 figures, Presentation at APPC12(Makuhari,Chiba,Japan,2013.7.14-19), JPS Conference Proceedings (in press)