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High-density cusps of compact remnants are expected to form around supermassive black holes (SMBHs) in galactic nuclei via dynamical friction and two-body relaxation.
Trani, A. A., Spera, M., Leigh, N. W. C., and Fujii, M. S.: 2019, · 1904
Earlier work this paper cites.
MNRAS 310
Mikkola, S. and Tanikawa, K.: 1999, · 1999
Earlier work this paper cites.
ApJ 757(1)
Antonini, F. and Perets, H. B.: 2012, · 2012
Cited alongside, same era.
Monthly Notices of the Royal Astronomical Society
Leigh, N. W. C., Antonini, F., Stone, N. C., Shara, M. M., and Merritt, D.: 2016, · 2016
Cited alongside, same era.
Nature 556
Hailey, C. J., Mori, K., Bauer, F. E., Berkowitz, M. E., Hong, J., and Hord, B. J.: 2018, · 2018
Later among the works it cites.
The Astrophysical Journal
Trani, A. A., Fujii, M. S., and Spera, M.: 2019, · 2019
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