Space number density of bright quasars in the halo model of galaxy formation

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We analyse the redshift dependence of space number density of quasars assuming that they are the short-lived active stages of the massive galaxies and arise immediately after the collapse of homogeneous central part of protogalaxy clouds. Obtained dependence fits the observational data ChaMP+CDF+ROSAT (Silverman et al. 2005) very well for protogalaxy clouds of mass M≈ 8· 10¹¹ h⁻¹M and ellipticity e<0.4. The lifetime of bright X-ray AGNs or QSOs with Lₓ>10⁴⁴.⁵ erg· s⁻¹ in the range of energies 0.3-8 keV is τQSO 6·10⁶ years when the mass of supermassive black hole is MSMBH 10⁹ M and the values of other quasar parameters are reasonable. The analysis and all calculations were carried out in the framework of ΛCDM-model with parameters determined from 5-years WMAP, SNIa and large scale structure data (Komatsu et al. 2009). It is concluded, that the halo model of galaxy formation in the ΛCDM cosmological model matches well observational data on AGNs and QSOs number density coming from current optical and X-ray surveys.