Anisotropies of the cosmic microwave background in nonstandard cold dark matter models

Statistics – Computation

Scientific paper

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Anisotropy, Astronomical Models, Cosmology, Dark Matter, Microwaves, Relic Radiation, Computational Astrophysics, Density Distribution, Galactic Evolution, Power Spectra

Scientific paper

Small angular scale cosmic microwave anisotropies in flat, vacuum-dominated, cold dark matter cosmological models which fit large-scale structure observations and are consistent with a high value for the Hubble constant are reexamined. New predictions for CDM models in which the large-scale power is boosted via a high baryon content and low H(0) are presented. Both classes of models are consistent with current limits: an improvement in sensitivity by a factor of about 3 for experiments which probe angular scales between 7 arcmin and 1 deg is required, in the absence of very early reionization, to test boosted CDM models for large-scale structure formation.

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