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Accretion-Driven Evolution of Black Holes: Eddington Ratios, Duty Cycles, and Active Galaxy Fractions

Monthly Notices of the Royal Astronomical Society, no. 1 (2013): 421-446

Cited: 53|Views26
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Abstract

We develop semi-empirical models of the supermassive black hole and active galactic nucleus (AGN) populations, which incorporate the black hole growth implied by the observed AGN luminosity function assuming a radiative efficiency ϵ and a distribution of Eddington ratios λ. By generalizing these continuity-equation models to allow a distr...More

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