Built on

J. Gleyzes, D. Langlois, F. Piazza, and F. Vernizzi, JCAP 1502
Original
1952
Earlier work this paper cites.
T. Regge and J. A. Wheeler, Phys. Rev. 108
1957
Earlier work this paper cites.
C. Brans and R. H. Dicke, Phys. Rev. 124
1961
Earlier work this paper cites.
F. J. Zerilli, Phys. Rev. Lett. 24
1970
Earlier work this paper cites.
S. W. Hawking, Communications in Mathematical Physics 25
1972
Earlier work this paper cites.
S. A. Teukolsky, Astrophys. J. 185
1973
Earlier work this paper cites.
G. W. Horndeski, Int. J. Theor. Phys. 10
1974
Earlier work this paper cites.
S. Chandrasekhar and S. Detweiler, Proceedings of the Royal Society of London Series A 344
1975
Earlier work this paper cites.
E. W. Leaver, Proceedings of the Royal Society of London Series A 402
1985
Earlier work this paper cites.
O. J. Kwon, Y. D. Kim, Y. S. Myung, B. H. Cho, and Y. J. Park, Phys. Rev. D 34
1986
Earlier work this paper cites.
K. D. Kokkotas and B. G. Schmidt, Living Rev. Rel. 2
1999
Earlier work this paper cites.
H.-P. Nollert, Classical and Quantum Gravity 16
1999
Earlier work this paper cites.
L. Rezzolla, Astroparticle physics and cosmology. Proceedings: Summer School, Trieste, Italy, Jun 17-Jul 5 2002 , ICTP Lect. Notes Ser. 14
2003
Earlier work this paper cites.
E. Teo, General Relativity and Gravitation 35
2003
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.
R. A. Konoplya and A. V. Zhidenko, Phys. Lett. B609
2005
Earlier work this paper cites.
K. Martel and E. Poisson, Phys. Rev. D71
2005
Earlier work this paper cites.
E. Berti, V. Cardoso, and C. M. Will, Phys. Rev. D73
2006
Earlier work this paper cites.

Similar

R. A. Konoplya and A. V. Zhidenko, Phys. Rev. D 73
2006
Cited alongside, same era.
E. Berti, V. Cardoso, and A. O. Starinets, Class. Quant. Grav. 26
Original
2009
Cited alongside, same era.
S. R. Dolan and A. C. Ottewill, Classical and Quantum Gravity 26
Original
2009
Cited alongside, same era.
C. de Rham and L. Heisenberg, Phys. Rev. D84
Original
2011
Cited alongside, same era.
T. Clifton, P. G. Ferreira, A. Padilla, and C. Skordis, Physics Reports 513
2012
Cited alongside, same era.
T. Kobayashi, H. Motohashi, and T. Suyama, Phys. Rev. D85

Then

L. Lombriser and A. Taylor, JCAP 1603
Original
2016
Later among the works it cites.
B. P. Abbott, R. Abbott, T. D. Abbott, F. Acernese, K. Ackley, C. Adams, T. Adams, P. Addesso, R. X. Adhikari, V. B. Adya, and et al., Physical Review Letters 118
Original
2017
Later among the works it cites.
B. P. Abbott et al. (Virgo, LIGO Scientific), Phys. Rev. Lett. 119
Original
2017
Later among the works it cites.
Y. Gong, E. Papantonopoulos, and Z. Yi, (2017), arXiv:1711.04102 [gr-qc]
Original
2017
Later among the works it cites.
D. A. Coulter, R. J. Foley, C. D. Kilpatrick, M. R. Drout, A. L. Piro, B. J. Shappee, M. R. Siebert, J. D. Simon, N. Ulloa, D. Kasen, B. F. Madore, A. Murguia-Berthier, Y.-C. Pan, J. X. Prochaska, E. Ramirez-Ruiz, A. Rest, and C. Rojas-Bravo, Science 358

Beyond the bibliography

alphaXiv searches the wider corpus for related work and actual follow-ups.

Open on alphaXiv

alphaXiv is searching for related work…

Reading the bibliography…

2018

Quasi-normal modes of black holes in Horndeski gravity

Tattersall, Oliver J., Ferreira, Pedro G.

Understand

We study the perturbations to General Relativistic black holes (i.e.

those without scalar hair) in Horndeski scalar-tensor gravity.
First, we derive the equations of odd and even parity perturbations of both the metric and scalar field in the case of a Schwarzschild black hole, and show that the gravitational waves emitted from such a system contain a mixture of quasi-normal mode frequencies from the usual General Relativistic spectrum and those from the new scalar field spectrum, with the new scalar spectrum characterised by just two free parameters.
We then specialise to the sub-family of Horndeski theories in which gravitational waves propagate at the speed of light $c$ on cosmological backgrounds; the scalar quasi-normal mode spectrum of such theories is characterised by just a single parameter $\mu$ acting as an effective mass of the scalar field.

Built on

J. Gleyzes, D. Langlois, F. Piazza, and F. Vernizzi, JCAP 1502
Original
1952
Earlier work this paper cites.
T. Regge and J. A. Wheeler, Phys. Rev. 108
1957
Earlier work this paper cites.
C. Brans and R. H. Dicke, Phys. Rev. 124
1961
Earlier work this paper cites.
F. J. Zerilli, Phys. Rev. Lett. 24
1970
Earlier work this paper cites.
S. W. Hawking, Communications in Mathematical Physics 25
1972
Earlier work this paper cites.
S. A. Teukolsky, Astrophys. J. 185
1973
Earlier work this paper cites.
G. W. Horndeski, Int. J. Theor. Phys. 10
1974
Earlier work this paper cites.
S. Chandrasekhar and S. Detweiler, Proceedings of the Royal Society of London Series A 344
1975
Earlier work this paper cites.
E. W. Leaver, Proceedings of the Royal Society of London Series A 402
1985
Earlier work this paper cites.
O. J. Kwon, Y. D. Kim, Y. S. Myung, B. H. Cho, and Y. J. Park, Phys. Rev. D 34
1986
Earlier work this paper cites.
K. D. Kokkotas and B. G. Schmidt, Living Rev. Rel. 2
1999
Earlier work this paper cites.
H.-P. Nollert, Classical and Quantum Gravity 16
1999
Earlier work this paper cites.
L. Rezzolla, Astroparticle physics and cosmology. Proceedings: Summer School, Trieste, Italy, Jun 17-Jul 5 2002 , ICTP Lect. Notes Ser. 14
2003
Earlier work this paper cites.
E. Teo, General Relativity and Gravitation 35
2003
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.
R. A. Konoplya and A. V. Zhidenko, Phys. Lett. B609
2005
Earlier work this paper cites.
K. Martel and E. Poisson, Phys. Rev. D71
2005
Earlier work this paper cites.
E. Berti, V. Cardoso, and C. M. Will, Phys. Rev. D73
2006
Earlier work this paper cites.