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The sheer range of scales in the Universe makes it impossible to model all atonce. It is necessary, therefore, when conducting numerical experiments, thatwe employ sub-resolution prescriptions that can represent the scales we areunable to model directly. In this article we present a prescription for blackhole growth that incorporates a different accretion regime from the standardapproach used in the literature, and discuss the results of dedicatedsimulations of intermediate processes between small-scale accretion flows andlarge-scale cosmological volumes that can strongly enhance the accretion rateonto the black hole at the centre of a galaxy.

Growing supermassive black holes: sub-grid modelling and intermediate-scale processes