The angular distribution of the background radiation in homogeneous cosmological models

Details The angular distribution of the background radiation in homogeneous cosmological models The angular distribution of the background radiation in homogeneous cosmological models

Jun 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984a%26a...135...53f&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 135, no. 1, June 1984, p. 53-58.

Astronomy and Astrophysics

Astrophysics

7

Background Radiation, Cosmology, Relic Radiation, Angular Distribution, Anisotropy, Astronomical Models, Spherical Harmonics

Scientific paper

A general harmonic analysis method is developed for obtaining solutions to modes of the angular distribution of the 3 K background. The anisotropy of the background is due to a dipole movement of the observer, the motion of the emitting matter, and shear forces. A spherical harmonic decomposition is defined for decoupling the temporal and angular dependence of the anisotropy. The method is applied to models with a Friedmann class of solutions of the Bianchi types I, V, and IX.

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