An upper limit to the velocity dispersion of relaxed stellar systems without massive black holes
M. Coleman Miller, Melvyn B. Davies

TL;DR
The paper proposes a critical velocity dispersion threshold (~40 km/s) above which massive black holes inevitably form in relaxed stellar systems due to core collapse and black hole mergers, explaining their presence in high-dispersion galaxies.
Contribution
It introduces a velocity dispersion threshold for black hole formation in stellar systems, linking core collapse dynamics to black hole growth across cosmic epochs.
Findings
Black holes form in systems with velocity dispersion above ~40 km/s.
Below this threshold, black hole mergers tend to eject black holes, preventing growth.
High accretion rates lead to rapid black hole growth via tidal disruption of stars.
Abstract
Massive black holes have been discovered in all closely examined galaxies with high velocity dispersion. The case is not as clear for lower-dispersion systems such as low-mass galaxies and globular clusters. Here we suggest that above a critical velocity dispersion of roughly 40 km/s, massive central black holes will form in relaxed stellar systems at any cosmic epoch. This is because above this dispersion primordial binaries cannot support the system against deep core collapse. If, as previous simulations show, the black holes formed in the cluster settle to produce a dense subcluster, then given the extremely high densities reached during core collapse the holes will merge with each other. For low velocity dispersions and hence low cluster escape speeds, mergers will typically kick out all or all but one of the holes due to three-body kicks or the asymmetric emission of gravitational…
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