Built on

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E. Berti, V. Cardoso, and C. M. Will, Phys. Rev. D 73
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M. Campanelli, C. O. Lousto, Y. Zlochower, and D. Merritt, Physical Review Letters 98
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A. Sesana, MNRAS 382
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M. Koppitz, D. Pollney, C. Reisswig, L. Rezzolla, J. Thornburg, P. Diener, and E. Schnetter, Physical Review Letters 99
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M. J. Valtonen, H. J. Lehto, K. Nilsson, J. Heidt, L. O. Takalo, A. Sillanpää, C. Villforth, M. Kidger, G. Poyner, Pursimo, et al. , Nature 452
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C. O. Lousto and Y. Zlochower, Phys. Rev. D 77
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2016

Black hole kicks as new gravitational wave observables

Gerosa, Davide, Moore, Christopher J.

Understand

Generic black hole binaries radiate gravitational waves anisotropically, imparting a recoil, or kick, velocity to the merger remnant.

If a component of the kick along the line of sight is present, gravitational waves emitted during the final orbits and merger will be gradually Doppler shifted as the kick builds up.
We develop a simple prescription to capture this effect in existing waveform models, showing that future gravitational wave experiments will be able to perform direct measurements, not only of the black hole kick velocity, but also of its accumulation profile.
In particular, the eLISA space mission will measure supermassive black hole kick velocities as low as ~500 km/s, which are expected to be a common outcome of black hole binary coalescence following galaxy mergers.

Built on

C. O. Lousto, Y. Zlochower, M. Dotti, and M. Volonteri, Phys. Rev. D 85
Original
1923
Earlier work this paper cites.
S. Komossa, Advances in Astronomy 2012
Original
1977
Earlier work this paper cites.
A. Krolak and B. F. Schutz, General Relativity and Gravitation 19
1987
Earlier work this paper cites.
I. H. Redmount and M. J. Rees, Comments on Astrophysics 14
1989
Earlier work this paper cites.
L. E. Kidder, Phys. Rev. D 52
1995
Earlier work this paper cites.
D. Merritt, M. Milosavljević, M. Favata, S. A. Hughes, and D. E. Holz, ApJ 607
2004
Earlier work this paper cites.
J. D. Schnittman, Phys. Rev. D 70
2004
Earlier work this paper cites.
C. Rodriguez, G. B. Taylor, R. T. Zavala, A. B. Peck, L. K. Pollack, and R. W. Romani, ApJ 646
2006
Earlier work this paper cites.
E. Berti, V. Cardoso, and C. M. Will, Phys. Rev. D 73
2006
Earlier work this paper cites.
M. Campanelli, C. O. Lousto, Y. Zlochower, and D. Merritt, Physical Review Letters 98
2007
Earlier work this paper cites.
A. Sesana, MNRAS 382
Original
2007
Earlier work this paper cites.
M. Koppitz, D. Pollney, C. Reisswig, L. Rezzolla, J. Thornburg, P. Diener, and E. Schnetter, Physical Review Letters 99
2007
Earlier work this paper cites.
M. J. Valtonen, H. J. Lehto, K. Nilsson, J. Heidt, L. O. Takalo, A. Sillanpää, C. Villforth, M. Kidger, G. Poyner, Pursimo, et al. , Nature 452
Original
2008
Earlier work this paper cites.
A. Gualandris and D. Merritt, ApJ 678
Original
2008
Earlier work this paper cites.
S. Komossa and D. Merritt, ApJ 689
Original
2008
Earlier work this paper cites.
B. Brügmann, J. A. González, M. Hannam, S. Husa, and U. Sperhake, Phys. Rev. D 77
Original
2008
Earlier work this paper cites.
C. O. Lousto and Y. Zlochower, Phys. Rev. D 77
Original
2008
Earlier work this paper cites.