The cosmic microwave background: from the spectrum to the anisotropies

The spectrum and the temperature anisotropies of the cosmic microwave backg ound (CMB) are both essential, quantitative tools for cosmology. The former contains a record of the thermal history of the Universe back to a tempera ture T similar to1 keV. In this context, I discuss the process of thermaliz ation, i.e., the establishment of a Planck spectrum, as well as the Compton and mu -distortions. The fundamental ingredients necessary for understandi ng the angular power spectrum of the temperature anisotropies are then pres ented. The first generation anisotropy data is shown to be consistent with the basic expectations of Inflation: a flat Universe with scale-invariant p erturbations. This data set also prefers a rather large baryon density. The recent BOOMERanG and MAXIMA-1 data confirm these first indications with hi gher precision. (C) 2001 Elsevier Science B.V. All rights reserved.