Ray aberration and large-scale anisotropy of the cosmic background radiation

Details Ray aberration and large-scale anisotropy of the cosmic background radiation Ray aberration and large-scale anisotropy of the cosmic background radiation

Dec 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977nciml..20..563f&link_type=abstract

Nuovo Cimento, Lettere, vol. 20, Dec. 10, 1977, p. 563-568.

Physics

3

Background Radiation, Big Bang Cosmology, Cosmic Rays, Radiation Distribution, Space-Time Functions, Aberration, Angular Distribution, Anisotropy

Scientific paper

Calculations are performed to show how the large-scale anisotropy of the cosmic background can be affected by the aberration of radiation rays that occurs during the free propagation of photons in an anisotropically expanding universe. This effect is considerable in the late Milne epoch of type V and type VII Bianchi spaces. The predicted anisotropy produced by the aberration of rays is such that one can conclude from the present isotropy of up to one part in one thousand that the universe is in its quasi-isotropic stage or it entered the Milne epoch only recently.

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