Consequences of gravitational radiation recoil

David Merritt, Miloš Milosavljević, Marc Favata, Scott A. Hughes, Daniel E. Holz

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Abstract

Coalescing binary black holes experience an impulsive kick from anisotropic emission of gravitational waves. Recoil velocities are sufficient to eject most coalescing black holes from dwarf galaxies and globular clusters, which may explain the apparent absence of massive black holes in these systems. Ejection from giant elliptical galaxies would be rare, but coalescing black holes are displaced from the center and fall back on a timescale of order the half-mass crossing time. Displacement of the black holes transfers energy to the stars in the nucleus and can convert a steep density cusp into a core. Radiation recoil calls into question models that grow supermassive black holes from hierarchical mergers of stellar-mass precursors.

Original languageEnglish
Pages (from-to)L9-L12
JournalAstrophysical Journal
Volume607
Issue number1 II
DOIs
StatePublished - 20 May 2004

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Keywords

  • Black hole physics
  • Galaxies: nuclei
  • Gravitation
  • Gravitational waves

Cite this

Merritt, D., Milosavljević, M., Favata, M., Hughes, S. A., & Holz, D. E. (2004). Consequences of gravitational radiation recoil. Astrophysical Journal, 607(1 II), L9-L12. https://doi.org/10.1086/421551