Fluctuations in the microwave background at large angular scale

Details Fluctuations in the microwave background at large angular scale Fluctuations in the microwave background at large angular scale

Jun 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980phys...21..619s&link_type=abstract

(University of Copenhagen, Danish Research Council and Nordisk Institut for Teoretisk Atomfysik, Copenhagen Symposium on the Uni

Mathematics

Logic

8

Angular Distribution, Background Radiation, Cosmic Rays, Cosmology, Microwave Emission, Universe, Anisotropy, Big Bang Cosmology, Galactic Evolution, Isotropy, Microwave Frequencies, Solar Orbits, Spherical Harmonics

Scientific paper

The measurements of fluctuations in the cosmic microwave background are shown to be consistent with the first order anisotropy at the level of about one part in a thousand and the limits of about one part in three thousand for fluctuations on any other scale. It is suggested that the first order anisotropy is due to the motion of the solar system relative to the radiation. This interpretation is evidence supporting the Cosmological Principle. The observed isotropy of the cosmic microwave background contradicts the concept of an indefinite hierarchy of clustering in the universe.

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