Cookies

We use cookies to ensure that we give you the best experience on our website. You can change your cookie settings at any time. Otherwise, we'll assume you're OK to continue.

Durham University

Department of Physics

Staff profile

Publication details for Prof Richard Bower

McAlpine, Stuart, Bower, Richard G., Rosario, David J., Crain, Robert A., Schaye, Joop & Theuns, Tom (2018). The rapid growth phase of supermassive black holes. Monthly Notices of the Royal Astronomical Society 481(3): 3118-3128.

Author(s) from Durham

Abstract

We investigate the rapid growth phase of supermassive black holes (BHs) within the hydrodynamical cosmological EAGLE simulation. This non-linear phase of BH growth occurs within ∼L* galaxies, embedded between two regulatory states of the galaxy host: in sub L* galaxies efficient stellar feedback regulates the gas inflow on to the galaxy and significantly reduces the growth of the central BH, while in galaxies more massive than L* efficient AGN feedback regulates the gas inflow on to the galaxy and curbs further non-linear BH growth. We find evolving critical galaxy and halo mass scales at which rapid BH growth begins. Galaxies in the low-redshift Universe transition into the rapid BH growth phase in haloes that are approximately an order of magnitude more massive than their high-redshift counterparts (M200  ≈1012.4 M⊙ at z ≈ 0 decreasing to M200  ≈1011.2 M⊙ at z ≈ 6). Instead, BHs enter the rapid growth phase at a fixed critical halo virial temperature (Tvir ≈ 105.6 K). We additionally show that major galaxy–galaxy interactions ( μ≥14 , where μ is the stellar mass ratio) play a substantial role in triggering the rapid growth phase of BHs in the low-redshift Universe, whilst potentially having a lower influence at high redshift. Approximately 40 per cent of BHs that initiate the rapid BH growth phase at z ≈ 0 do so within ±0.5 dynamical times of a major galaxy–galaxy merger, a fourfold increase above what is expected from the background merger rate. We find that minor mergers ( 110≤μ<14 ) have a substantially lower influence in triggering the rapid growth phase at all epochs.