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Interpretation of observed cosmic microwave background radiationIt is argued that the 'surface of last scattering' of the observed microwave background radiation corresponds to the distribution of dust in galaxies or protogalaxies with a temperature of about 110 K at the epoch corresponding to Z roughly equal to 40. This is in contrast with the plasma temperature of over 3,000 K at an earlier epoch (Z greater than about 1,000), as given by the canonical model of big bang cosmologies. In view of this, the claim that the microwave background radiation lends strong support to hot big bang cosmologies is without foundation.
Document ID
19770048630
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Alfven, H.
(California Univ. La Jolla, CA, United States)
Mendis, A.
(California, University La Jolla, Calif., United States)
Date Acquired
August 8, 2013
Publication Date
April 21, 1977
Publication Information
Publication: Nature
Volume: 266
Subject Category
Space Radiation
Accession Number
77A31482
Distribution Limits
Public
Copyright
Other

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