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• W1866590555 abstract "In this work we investigate the accretion of cosmological fluids onto an intermediate-mass black hole at the centre of a globular cluster, focusing on the influence of the parent stellar system on the accretion flow. We show that the accretion of cosmic background radiation and the so-called dark energy onto an intermediate-mass black hole is negligible. On the other hand, if cold dark matter has a nonvanishing pressure, the accretion of dark matter is large enough to increase the black hole mass well beyond the present observed upper limits. We conclude that either intermediate-mass black holes do not exist, or dark matter does not exist, or it is not strictly collisionless. In the latter case, we set a lower limit for the parameter of the cold dark matter equation of state." @default.
• W1866590555 created "2016-06-24" @default.
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• W1866590555 date "2012-01-27" @default.
• W1866590555 modified "2023-09-25" @default.
• W1866590555 title "Dark matter and dark energy accretion on to intermediate-mass black holes" @default.
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• W1866590555 doi "https://doi.org/10.1111/j.1365-2966.2011.20252.x" @default.
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