Built on

T. Johannsen and D. Psaltis, Astrophys. J. 718
Original
1931
Earlier work this paper cites.
D. G. Boulware and S. Deser, Phys. Rev. D6
1972
Earlier work this paper cites.
A. C. Fabian, M. J. Rees, L. Stella, and N. E. White, Mon. Not. Roy. Astron. Soc. 238
1989
Earlier work this paper cites.
L. S. Finn and P. J. Sutton, Phys. Rev. D65
2002
Earlier work this paper cites.
C. Bambi and E. Barausse, Astrophys. J. 731
Original
2007
Earlier work this paper cites.
P. Amaro-Seoane, J. R. Gair, M. Freitag, M. Coleman Miller, I. Mandel, C. J. Cutler, and S. Babak, Class. Quant. Grav. 24
2007
Earlier work this paper cites.
C. de Rham and G. Gabadadze, Phys. Rev. D82
Original
2010
Earlier work this paper cites.
C. de Rham, G. Gabadadze, and A. J. Tolley, Phys. Rev. Lett. 106
Original
2011
Earlier work this paper cites.
L. Berezhiani, G. Chkareuli, C. de Rham, G. Gabadadze, and A. J. Tolley, Phys. Rev. D85
Original
2012
Earlier work this paper cites.

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2017

Can the graviton have a large mass near black holes?

Zhang, Jun, Zhou, Shuang-Yong

Understand

The mass of the graviton, if nonzero, is usually considered to be very small, e.g.

of the Hubble scale, from several observational constraints.
In this paper, we propose a gravity model where the graviton mass is very small in the usual weak gravity environments, below all the current graviton mass bounds, but becomes much larger in the strong gravity regime such as a black hole's vicinity.
For black holes in this model, significant deviations from general relativity emerge very close to the black hole horizon and alter the black hole quasi-normal modes, which can be extracted from the ringdown waveform of black hole binary mergers.

Built on

T. Johannsen and D. Psaltis, Astrophys. J. 718
Original
1931
Earlier work this paper cites.
D. G. Boulware and S. Deser, Phys. Rev. D6
1972
Earlier work this paper cites.
A. C. Fabian, M. J. Rees, L. Stella, and N. E. White, Mon. Not. Roy. Astron. Soc. 238
1989
Earlier work this paper cites.
L. S. Finn and P. J. Sutton, Phys. Rev. D65
2002
Earlier work this paper cites.
C. Bambi and E. Barausse, Astrophys. J. 731
Original
2007
Earlier work this paper cites.
P. Amaro-Seoane, J. R. Gair, M. Freitag, M. Coleman Miller, I. Mandel, C. J. Cutler, and S. Babak, Class. Quant. Grav. 24
2007
Earlier work this paper cites.
C. de Rham and G. Gabadadze, Phys. Rev. D82
Original
2010
Earlier work this paper cites.
C. de Rham, G. Gabadadze, and A. J. Tolley, Phys. Rev. Lett. 106
Original
2011
Earlier work this paper cites.
L. Berezhiani, G. Chkareuli, C. de Rham, G. Gabadadze, and A. J. Tolley, Phys. Rev. D85
Original
2012
Earlier work this paper cites.

Similar

Q.-G. Huang, Y.-S. Piao, and S.-Y. Zhou, Phys. Rev. D86
Original
2012
Cited alongside, same era.
C. Bambi, JCAP 1209
Original
2012
Cited alongside, same era.
C. de Rham, Living Rev. Rel. 17
Original
2014
Cited alongside, same era.
M. S. Volkov, Lect. Notes Phys. 892
Original
2015
Cited alongside, same era.
A. J. Tolley, D.-J. Wu, and S.-Y. Zhou, Phys. Rev. D92
Original
2015
Cited alongside, same era.

Then

C. de Rham, A. J. Tolley, and S.-Y. Zhou, JHEP 04
Original
2016
Later among the works it cites.
K. Aoki and S. Mizuno, Phys. Rev. D94
Original
2016
Later among the works it cites.
J. Abedi, H. Dykaar, and N. Afshordi, (2017), arXiv:1701.03485 [gr-qc]
Original
2017
Closest in time.
R. H. Price and G. Khanna, (2017), arXiv:1702.04833 [gr-qc]
Original
2017
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V. Cardoso and P. Pani, (2017), arXiv:1707.03021 [gr-qc]
Original
2017
Closest in time.

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The precise definition of a particle mass in curved space is a subtle issue. Here we simply take the size of coefficients of the quadratic perturbative potential as an effective measure

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