The long wavelength spectrum of the Cosmic Microwave Background

Details The long wavelength spectrum of the Cosmic Microwave Background The long wavelength spectrum of the Cosmic Microwave Background

May 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999aipc..476..149s&link_type=abstract

Conference on 3K cosmology. AIP Conference Proceedings, Volume 476, pp. 149-153 (1999).

Astronomy and Astrophysics

Astrophysics

2

Background Radiations, Observational Cosmology

Scientific paper

The search of distortions (deviations from a Planck distribution) in the spectrum of the Cosmic Microwave Background allows to probe the conditions existing in our Universe up to Z~=106. We analyze the status of the observations (so far no distortion has been detected) and discuss the possibility and the astrophysical interest of searching distortions at long wavelengths, in the Rayleigh Jeans portion of the Cosmic Microwave Background spectrum.

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