Thermal photon dispersion law and modified black-body spectra

Physics – High Energy Physics – High Energy Physics - Theory

Scientific paper

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v2: 13 pages, 6 figures; sec. 2.1. added to explain effective theory; references added; matches journal published version

Scientific paper

10.1002/andp.200910348

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 $p^2=0$. While this approximation turns out to be excellent for temperatures $\le 2 T_{\tiny{CMB}}$ 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 $p^2=0$, remain valid.

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