Integral representation for non-Planckian distributions and the cosmic background radiation

Details Integral representation for non-Planckian distributions and the cosmic background radiation Integral representation for non-Planckian distributions and the cosmic background radiation

Feb 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980phrvl..44..359a&link_type=abstract

Physical Review Letters, vol. 44, Feb. 4, 1980, p. 359-361.

Physics

5

Background Radiation, Cosmic Rays, Distribution Functions, Radiation Spectra, Big Bang Cosmology, Black Body Radiation, Field Theory (Physics), Functional Integration, Photons, Quantum Mechanics, Universe

Scientific paper

A general result for the nonequilibrium distribution function for photons gives a greatest lower bound for the radiation flux spectrum. This inequality allows one to establish, from the recent measurements of the cosmic background radiation, that the observed spectrum arises from the superposition of single sources. Since the primeval fireball may be one of the single sources, it is inferred that the observed spectrum is consistent with a big-bang origin for the universe.

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