On the origin of possible deviation from the blackbody spectrum of the cosmic microwave background radiation - Inverse Compton hypothesis based upon the explosion scenario

Details On the origin of possible deviation from the blackbody spectrum of the cosmic microwave background radiation - Inverse Compton hypothesis based upon the explosion scenario On the origin of possible deviation from the blackbody spectrum of the cosmic microwave background radiation - Inverse Compton hypothesis based upon the explosion scenario

Dec 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987apj...323l...7y&link_type=abstract

Astrophysical Journal, Part 2 - Letters to the Editor (ISSN 0004-637X), vol. 323, Dec. 1, 1987, p. L7-L11.

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Computational Astrophysics, Interstellar Matter, Inverse Scattering, Relic Radiation, Astronomical Models, Black Body Radiation, Compton Effect, Space Temperature

Scientific paper

Possible deviation from the blackbody spectrum of the cosmic microwave background radiation at the Wien part is indicated by the rocket observation of Nagoya-Berkeley group. Here, the inverse Compton hypothesis is examined based upon the explosion scenario for galaxy formation. Allowed ranges of physical parameters for reproducing the observation are explored in relation to the isotropy of spectrum at the Rayleigh-Jeans part, the size of voids, and the X-ray background radiation.

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