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S. Borhanian, K. G. Arun, H. P. Pfeiffer, and B. S. Sathyaprakash, (2019), arXiv:1901.08516 [gr-qc]
Original
1901
Earlier work this paper cites.
V. Cardoso and P. Pani, Living Rev. Rel. 22
Original
1904
Earlier work this paper cites.
V. Varma, S. E. Field, M. A. Scheel, J. Blackman, D. Gerosa, L. C. Stein, L. E. Kidder, and H. P. Pfeiffer, Phys. Rev. Research. 1
Original
1905
Earlier work this paper cites.
B. P. Abbott et al. (LIGO Scientific, Virgo), Astrophys. J. 883
Original
1907
Earlier work this paper cites.
S. Bhagwat, X. J. Forteza, P. Pani, and V. Ferrari, Phys. Rev. D101
Original
1910
Earlier work this paper cites.
M. Okounkova, L. C. Stein, J. Moxon, M. A. Scheel, and S. A. Teukolsky, Phys. Rev. D 101
Original
1911
Earlier work this paper cites.
I. Ota and C. Chirenti, Phys. Rev. D 101
Original
1911
Earlier work this paper cites.
M. Maggiore et al. , JCAP 03
Original
1912
Earlier work this paper cites.
B. Carter, Phys. Rev. Lett. 26
1971
Earlier work this paper cites.
S. W. Hawking, Phys. Rev. Lett. 26
1971
Earlier work this paper cites.
S. W. Hawking and J. B. Hartle, Commun. Math. Phys. 27
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.
J. D. Bekenstein, Phys. Rev. D7
1973
Earlier work this paper cites.
S. A. Teukolsky and W. H. Press, Astrophys. J. 193
1974
Earlier work this paper cites.
S. Chandrasekhar and S. L. Detweiler, Proc. Roy. Soc. Lond. A344
1975
Earlier work this paper cites.
V. Ferrari and B. Mashhoon, Phys. Rev. D 30
1984
Earlier work this paper cites.
S. Chandrasekhar, The mathematical theory of black holes (Oxford Classic Texts in the Physical Sciences, 1985)
1985
Earlier work this paper cites.
K. D. Kokkotas and B. G. Schmidt, Living Rev. Rel. 2
1999
Earlier work this paper cites.
M. Okounkova, Phys. Rev. D 102
Original
2001
Earlier work this paper cites.
V. Baibhav, E. Berti, and V. Cardoso, Phys. Rev. D 101
Original
2001
Earlier work this paper cites.

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2022

A novel ringdown amplitude-phase consistency test

Forteza, Xisco Jiménez, Bhagwat, Swetha, Kumar, Sumit et al.

Understand

The ringdown signal emitted during a binary black hole coalescence can be modeled as a linear superposition of the characteristic damped modes of the remnant black hole that get excited during the merger phase.

While checking the consistency of the measured frequencies and damping times against the Kerr BH spectrum predicted by General Relativity (GR) is a cornerstone of strong-field tests of gravity, the consistency of measured excitation amplitudes and phases have been largely left unexplored.
For a nonprecessing, quasi-circular binary black hole merger, we find that GR predicts a narrow region in the space of mode amplitude ratio and phase difference, independently of the spin of the binary components.
% Using this unexpected result, we develop a new null test of strong-field gravity which demands that the measured amplitudes and phases of different ringdown modes should lie within this narrow region predicted by GR.

Built on

S. Borhanian, K. G. Arun, H. P. Pfeiffer, and B. S. Sathyaprakash, (2019), arXiv:1901.08516 [gr-qc]
Original
1901
Earlier work this paper cites.
V. Cardoso and P. Pani, Living Rev. Rel. 22
Original
1904
Earlier work this paper cites.
V. Varma, S. E. Field, M. A. Scheel, J. Blackman, D. Gerosa, L. C. Stein, L. E. Kidder, and H. P. Pfeiffer, Phys. Rev. Research. 1
Original
1905
Earlier work this paper cites.
B. P. Abbott et al. (LIGO Scientific, Virgo), Astrophys. J. 883
Original
1907
Earlier work this paper cites.
S. Bhagwat, X. J. Forteza, P. Pani, and V. Ferrari, Phys. Rev. D101
Original
1910
Earlier work this paper cites.
M. Okounkova, L. C. Stein, J. Moxon, M. A. Scheel, and S. A. Teukolsky, Phys. Rev. D 101
Original
1911
Earlier work this paper cites.
I. Ota and C. Chirenti, Phys. Rev. D 101
Original
1911
Earlier work this paper cites.
M. Maggiore et al. , JCAP 03
Original
1912
Earlier work this paper cites.
B. Carter, Phys. Rev. Lett. 26
1971
Earlier work this paper cites.
S. W. Hawking, Phys. Rev. Lett. 26
1971
Earlier work this paper cites.
S. W. Hawking and J. B. Hartle, Commun. Math. Phys. 27
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.
J. D. Bekenstein, Phys. Rev. D7
1973
Earlier work this paper cites.
S. A. Teukolsky and W. H. Press, Astrophys. J. 193
1974
Earlier work this paper cites.
S. Chandrasekhar and S. L. Detweiler, Proc. Roy. Soc. Lond. A344
1975
Earlier work this paper cites.
V. Ferrari and B. Mashhoon, Phys. Rev. D 30
1984
Earlier work this paper cites.
S. Chandrasekhar, The mathematical theory of black holes (Oxford Classic Texts in the Physical Sciences, 1985)
1985
Earlier work this paper cites.
K. D. Kokkotas and B. G. Schmidt, Living Rev. Rel. 2
1999
Earlier work this paper cites.
M. Okounkova, Phys. Rev. D 102
Original
2001
Earlier work this paper cites.
V. Baibhav, E. Berti, and V. Cardoso, Phys. Rev. D 101
Original
2001
Earlier work this paper cites.