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M. Giesler, M. Isi, M. Scheel, and S. Teukolsky, “Black hole ringdown: the importance of overtones,” (2019), arXiv:1903.08284 [gr-qc]
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2019

Testing the no-hair theorem with GW150914

Isi, Maximiliano, Giesler, Matthew, Farr, Will M. et al.

Understand

We analyze gravitational-wave data from the first LIGO detection of a binary black-hole merger (GW150914) in search of the ringdown of the remnant black hole.

Using observations beginning at the peak of the signal, we find evidence of the fundamental quasinormal mode and at least one overtone, both associated with the dominant angular mode ($\ell=m=2$), with $3.6\sigma$ confidence.
A ringdown model including overtones allows us to measure the final mass and spin magnitude of the remnant exclusively from postinspiral data, obtaining an estimate in agreement with the values inferred from the full signal.
The mass and spin values we measure from the ringdown agree with those obtained using solely the fundamental mode at a later time, but have smaller uncertainties.

Built on

G. Carullo, W. Del Pozzo, and J. Veitch, Phys. Rev. D99
Original
1902
Earlier work this paper cites.
M. Giesler, M. Isi, M. Scheel, and S. Teukolsky, “Black hole ringdown: the importance of overtones,” (2019), arXiv:1903.08284 [gr-qc]
Original
1903
Earlier work this paper cites.
N. Levinson, Journal of Mathematics and Physics 25
1946
Earlier work this paper cites.
J. Durbin, Revue de l’Institut International de Statistique / Review of the International Statistical Institute 28
1960
Earlier work this paper cites.
P. Welch, IEEE Transactions on audio and electroacoustics 15
1967
Earlier work this paper cites.
C. V. Vishveshwara, Phys. Rev. D 1
1970
Earlier work this paper cites.
W. H. Press, Astrophys. J. 170
1971
Earlier work this paper cites.
S. Teukolsky, Phys. Rev. Lett. 29
1972
Earlier work this paper cites.
S. A. Teukolsky, Astrophys. J. 185
1973
Earlier work this paper cites.
W. H. Press and S. A. Teukolsky, Astrophys. J. 185
1973
Earlier work this paper cites.
S. Chandrasekhar and S. Detweiler, Proc. R. Soc. A 344
1975
Earlier work this paper cites.
E. W. Leaver, Proc. Roy. Soc. Lond. A402
1985
Earlier work this paper cites.
F. Echeverria, Phys. Rev. D40
1989
Earlier work this paper cites.
I. Verdinelli and L. Wasserman, Journal of the American Statistical Association 90
1995
Earlier work this paper cites.
O. Dreyer, B. J. Kelly, B. Krishnan, L. S. Finn, D. Garrison, and R. Lopez-Aleman, Class. Quant. Grav. 21
2004
Earlier work this paper cites.
E. Berti, V. Cardoso, and C. M. Will, Phys. Rev. D73
2006
Earlier work this paper cites.
A. Buonanno, G. B. Cook, and F. Pretorius, Phys. Rev. D75
2007
Earlier work this paper cites.
E. Berti, V. Cardoso, and A. O. Starinets, Class. Quantum Grav. 26
Original
2009
Earlier work this paper cites.