The cosmic microwave background radiation and galaxy formation

Details The cosmic microwave background radiation and galaxy formation The cosmic microwave background radiation and galaxy formation

Feb 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986cajph..64..147s&link_type=abstract

Canadian Journal of Physics (ISSN 0008-4204), vol. 64, Feb. 1986, p. 147-151.

Physics

5

Cosmology, Galactic Evolution, Relic Radiation, Big Bang Cosmology, Quadrupoles, Radiation Distribution

Scientific paper

Observational limits on the microwave-background-radiation anisotropy on various angular scales are reviewed. Comparison is made with the predictions of the gravitional-instability theory of galaxy formation from primordial fluctuations in the very early universe. There is no entirely satisfactory theory that presently reconciles inflationary cosmology predictions of the very early universe. There is no entirely satisfactory theory that presently reconciles inflationary cosmology predictions of the flatness of the universe and of the scale-invariant primordial fluctuations spectrum with the limits on the amplitude of the anisotropy (delta T/T), with the Virgo-cluster motion inferred from the dipole anisotropy, and with astronomical determinations of the cosmological density parameter.

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