Scale-invariant density perturbations, anisotropy of the cosmic microwave background, and large-scale peculiar velocity field

Details Scale-invariant density perturbations, anisotropy of the cosmic microwave background, and large-scale peculiar velocity field Scale-invariant density perturbations, anisotropy of the cosmic microwave background, and large-scale peculiar velocity field

Jun 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985apj...293l...1v&link_type=abstract

Astrophysical Journal, Part 2 - Letters to the Editor (ISSN 0004-637X), vol. 293, June 1, 1985, p. L1-L5. NASA-supported researc

Astronomy and Astrophysics

Astrophysics

46

Anisotropy, Background Radiation, Cosmology, Density Distribution, Relic Radiation, Galactic Clusters, Microwaves, Missing Mass (Astrophysics), Velocity Distribution

Scientific paper

The large-scale peculiar velocity field and the large- and intermediate-angular scale anisotropy of the cosmic microwave background are studied in inflationary cosmological models of critical density and containing primordial scale-invariant adiabatic density perturbations. Comparison with recent observations by de Vaucouleurs and Peters provides tentative support for a cold dark matter scenario in which the dark matter is not appreciably less clustered than the luminous galaxy distribution.

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