Interstellar Hydrogen and Cosmic Background Radiation
arXiv:physics/0004036 · doi:10.1016/S0960-0779(00)00158-2
Abstract
It is shown that a collection of photons with nearly the same frequency exhibits a "condensation" type of phenomenon corresponding to a peak intensity. The observed cosmic background radiation can be explained from this standpoint in terms of the radiation due to fluctuations in interstellar Hydrogen.
3 pages, TeX