Thermal photon dispersion law and modified black-body spectra
arXiv:0806.0972 · doi:10.1002/andp.200910348
Abstract
Based on the postulate that photon propagation is governed by an SU(2) gauge principle we numerically compute the one-loop dispersion for thermalized photon propagation on the radiatively induced mass shell. Formerly, the dispersion was addressed by assuming . While this approximation turns out to be excellent for temperatures the exact result exhibits a much faster (power-like) shrinking of the gap in the black-body spectral intensity with rising temperature. Our previous statements on anomalous large-angle CMB temperature-temperature correlations, obtained in the approximation , remain valid.
v2: 13 pages, 6 figures; sec. 2.1. added to explain effective theory; references added; matches journal published version
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