On the influence of X-ray galaxy clusters in the fluctuations of the cosmic microwave background

The negative evolution found in X–ray clusters of galaxies limits the amount of available hot gas for the inverse Compton scattering of the Cosmic Microwave Background (the Sunyaev–Zel’dovich effect). Using a parametrisation of the X-ray luminosity function and its evolution in terms of a coalescence model (as presented in the analysis of a flux limited X-ray cluster sample by Edge et al. 1990), as well as a simple virialised structure for the clusters (which requires a gas to total mass fraction � 0.1 in order to reproduce observed properties of nearby clusters) we show that the Compton distortion y parameter is about two orders of magnitude below the current FIRAS upper limits. Concerning the anisotropies imprinted on arcmin scales they are dominated by the hottest undetected objects. We show that they are negligible ( �T T � 10 −7 ) at wavelengths λ � 1 mm. At shorter wavelengths they become more important ( �T T � 10