R. Durrer, ANISOTROPIES IN THE COSMIC MICROWAVE BACKGROUND - THEORETICAL FOUNDATIONS, International journal of theoretical physics, 36(11), 1997, pp. 2469-2487
The analysis of anisotropies in the cosmic microwave background (CMB)
has become an extremely valuable tool for cosmology. There is even hop
e that planned CMB anisotropy experiments may revolutionize cosmology.
Together with determinations of the CMB spectrum, they represent the
first precise cosmological measurements. The value of CMB anisotropies
lies in large part in the simplicity of the theoretical analysis. Flu
ctuations in the CMB can be determined almost fully within linear cosm
ological perturbation theory and are not severely influenced by compli
cated nonlinear physics. In this contribution the different physical p
rocesses causing or influencing anisotropies in the CMB are discussed:
the geometry perturbations at and after last scattering, the acoustic
oscillations in the baryon-photon plasma prior to recombination, and
the diffusion damping during the process of recombination. The perturb
ations due to the fluctuating gravitational field, the so-called Sachs
-Wolfe contribution, is described in a very general form using the Wey
l tensor of the perturbed geometry.