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When did the large elliptical galaxies form?... The commonly discussed structure formation theory, ΛCDM, 1 certainly deserves careful attention because of its dramatic success in the interpretation of the temperature anisotropy of the 3K thermal cosmic background radiation....
général - core.ac.uk - PDF: citeseerx.ist.psu.edu
Noninteracting dark matter... We use the bounds on the present dark mass density and the measured large-scale fluctuations in the thermal cosmic background radiation to constrain the two parameters in a self-interaction potential that is a sum of quadratic and quartic terms in a single scalar dark matter...
Noninteracting dark matter...inflation.We use the bounds on the present dark mass density and the measured large-scalefluctuations in the thermal cosmic background radiation to constrain the twoparameters in a self-interaction potential that is a sum of quadratic andquartic terms in a single scalar dark matter field...
 PDF: arxiv.org
Small-scale anisotropy of the cosmic background radiation and scattering by cloudy plasmaIf the first stars formed soon after decoupling of baryons from the thermal cosmic background radiation (CBR), the radiation may have been last scattered in a cloudy plasma....
 PDF: core.ac.uk

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