Systematics of black hole binary inspiral kicks and the slowness approximation
During the inspiral and merger of black holes, the interaction of gravitational wave multipoles carries linear momentum away, thereby providing an astrophysically important recoil, or “kick” to the system and to the final black hole remnant. It has been found that linear momentum during the last sta...
Main Authors: | Price, Richard H., Khanna, Gaurav, Hughes, Scott A |
---|---|
Other Authors: | Massachusetts Institute of Technology. Department of Physics |
Format: | Article |
Language: | en_US |
Published: |
American Physical Society
2011
|
Online Access: | http://hdl.handle.net/1721.1/65946 https://orcid.org/0000-0001-6211-1388 |
Similar Items
-
Black hole binary inspiral and trajectory dominance
by: Price, Richard H., et al.
Published: (2014) -
Learning about Black Hole Binaries from their Ringdown Spectra
by: Hughes, Scott A, et al.
Published: (2022) -
Learning about Black Hole Binaries from their Ringdown Spectra
by: Hughes, Scott A, et al.
Published: (2021) -
Binary black hole merger gravitational waves and recoil in the large mass ratio limit
by: Sundararajan, Pranesh A., et al.
Published: (2010) -
Small mass plunging into a Kerr black hole: Anatomy of the inspiral-merger-ringdown waveforms
by: Taracchini, Andrea, et al.
Published: (2015)