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• W3097989181 startingPage "92" @default.
• W3097989181 abstract "We show that the MBH–Mbulge scaling relations observed from the local to the high-z universe can be largely or even entirely explained by a non-causal origin, i.e., they do not imply the need for any physically coupled growth of black hole (BH) and bulge mass, for example, through feedback by active galactic nuclei (AGNs). Provided some physics for the absolute normalization, the creation of the scaling relations can be fully explained by the hierarchical assembly of BH and stellar mass through galaxy merging, from an initially uncorrelated distribution of BH and stellar masses in the early universe. We show this with a suite of dark matter halo merger trees for which we make assumptions about (uncorrelated) BH and stellar mass values at early cosmic times. We then follow the halos in the presence of global star formation and BH accretion recipes that (1) work without any coupling of the two properties per individual galaxy and (2) correctly reproduce the observed star formation and BH accretion rate density in the universe. With disk-to-bulge conversion in mergers included, our simulations even create the observed slope of ∼1.1 for the MBH–Mbulge relation at z = 0. This also implies that AGN feedback is not a required (though still a possible) ingredient in galaxy evolution. In light of this, other mechanisms that can be invoked to truncate star formation in massive galaxies are equally justified." @default.
• W3097989181 created "2020-11-23" @default.
• W3097989181 creator A5006999794 @default.
• W3097989181 creator A5055026157 @default.
• W3097989181 date "2011-05-31" @default.
• W3097989181 modified "2023-10-16" @default.
• W3097989181 title "THE NON-CAUSAL ORIGIN OF THE BLACK-HOLE-GALAXY SCALING RELATIONS" @default.
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• W3097989181 doi "https://doi.org/10.1088/0004-637x/734/2/92" @default.
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