<< Cosmo.WebHome %TOC% ---- %INCLUDE{"BenasqueNotes2008Head"}% ---+ Jordi Miralde-Escudé ArXiv:0710.4488 Self-Consistent Models of the AGN and Black Hole Populations: Duty Cycles, Accretion Rates, and the Mean Radiative Efficiency See ArXiv:0710.4488 Some random comments: * Sołtan argument (1982?) * the X-ray background is now accepted as being mostly from AGNs * the Silk & Rees 1998 feedback mechanism has problems, so there's also a feeding mechanism * problems remain with matching all the observational parameters to the models * there's a new model with Kollmeier being prepared * BH evolution is closely tied with stellar spheroid evolution
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04 Aug 2008,
BoudRoukema
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