Consequences of Gravitational Radiation Recoil

Authors

David Merritt, Rochester Institute of Technology
Miloš Milosavljević, California Institute of Technology
Marc Favata, Montclair State UniversityFollow
Scott A. Hughes, Kavli Institute for Cosmological Physics
Daniel E. Holz, University of Chicago

Document Type

Article

Publication Date

5-20-2004

Journal / Book Title

The Astrophysical Journal

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.

DOI

10.1086/421551

MSU Digital Commons Citation

Merritt, David; Milosavljević, Miloš; Favata, Marc; Hughes, Scott A.; and Holz, Daniel E., "Consequences of Gravitational Radiation Recoil" (2004). Department of Physics and Astronomy Faculty Scholarship and Creative Works. 27.
https://digitalcommons.montclair.edu/physics-astron-facpubs/27

Published Citation

Merritt, D., Milosavljević, M., Favata, M., Hughes, S. A., & Holz, D. E. (2004). Consequences of gravitational radiation recoil. The Astrophysical Journal, 607(1), L9.