Anomalies in the gravitational recoil of eccentric black-hole mergers with unequal mass ratios
@inproceedings{Radia2021AnomaliesIT, title={Anomalies in the gravitational recoil of eccentric black-hole mergers with unequal mass ratios}, author={Miren Radia and Ulrich Sperhake and Emanuele Berti and Rupert Croft}, year={2021} }
Miren Radia,1, ∗ Ulrich Sperhake,1, 2, † Emanuele Berti,3, ‡ and Robin Croft1 Department of Applied Mathematics and Theoretical Physics, Centre for Mathematical Sciences, University of Cambridge, Wilberforce Road, Cambridge CB3 0WA, United Kingdom California Institute of Technology, Pasadena, California 91125, USA Department of Physics and Astronomy, Johns Hopkins University, 3400 N. Charles Street, Baltimore, Maryland, 21218, USA (Dated: January 28, 2021)
Figures and Tables from this paper
2 Citations
Hierarchical mergers of stellar-mass black holes and their gravitational-wave signatures
- PhysicsNature Astronomy
- 2021
We review theoretical findings, astrophysical modeling, and current gravitational-wave evidence of hierarchical stellar-mass black-hole mergers. While most of the compact binary mergers detected by…
GRChombo: An adaptable numerical relativity code for fundamental physics
- Computer Science, PhysicsJ. Open Source Softw.
- 2021
Tomas Andrade1, Llibert Areste Salo2, Josu C. Aurrekoetxea3, Jamie Bamber4, Katy Clough4, Robin Croft5, Eloy de Jong3, Amelia Drew5, Alejandro Duran6, Pedro G. Ferreira4, Pau Figueras2, Hal Finkel7,…
References
SHOWING 1-10 OF 102 REFERENCES
Gravitational-Radiation Recoil and Runaway Black Holes
- Physics
- 1973
In the nonspherical gavitational collapse of a stellar core to a black hole, linear momentum will in general be radiated with gravitational waves. As a result the black hole will recoil. Here we make…
Gravitational Recoil Velocities from Eccentric Binary Black Hole Mergers
- Physics
- 2006
The formation and growth of supermassive black holes is a key issue to unveil the secrets of galaxy formation. In particular, the gravitational recoil produced in the merger of unequal mass black…
Gravitational-Wave Recoil from the Ringdown Phase of Coalescing Black Hole Binaries
- Physics
- 2009
The gravitational recoil or "kick" of a black hole formed from the merger of two orbiting black holes, and caused by the anisotropic emission of gravitational radiation, is an astrophysically…
The Distribution of Recoil Velocities from Merging Black Holes
- Physics
- 2007
We calculate the linear momentum flux from merging black holes (BHs) with arbitrary masses and spin orientations, using the effective-one-body (EOB) model. This model includes an analytic description…
On the Assembly Rate of Highly Eccentric Binary Black Hole Mergers
- Physics
- 2017
In this {\it Letter} we calculate the fraction of highly eccentric binary black hole (BBH) mergers resulting from binary-single interactions. Using an $N$-body code that includes post-Newtonian…
Consequences of Gravitational Radiation Recoil
- Physics
- 2004
Coalescing binary black holes experience an impulsive kick due to anisotropic emission of gravitational waves. We discuss the dynamical consequences of the recoil accompanying massive black hole…
Gravitational recoil of inspiraling black hole binaries to second post-newtonian order
- Physics
- 2005
The loss of linear momentum by gravitational radiation and the resulting gravitational recoil of black hole binary systems may play an important role in the growth of massive black holes in early…
Post-Newtonian evolution of massive black hole triplets in galactic nuclei – IV. Implications for LISA
- PhysicsMonthly Notices of the Royal Astronomical Society
- 2019
Coalescing massive black hole binaries (MBHBs) of $10^{4-7} \rm M_{\odot}$, forming in the aftermath of galaxy mergers, are primary targets of the space mission LISA, the {\it Laser Interferometer…
11-orbit inspiral of a mass ratio 4:1 black-hole binary
- Physics
- 2011
We analyse an 11-orbit inspiral of a non-spinning black-hole binary with mass ratio q ≡ M_(1)/M_(2) = 4. The numerically obtained gravitational waveforms are compared with post-Newtonian (PN)…
The eccentric behavior of inspiralling compact binaries
- PhysicsClassical and Quantum Gravity
- 2018
Eccentricity of binary systems is not a gauge invariant quantity, but has an important impact on the observed gravitational wave signal of such systems, generating power in all possible harmonics of…