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Similar

J. Wilms, A. Allen and R. McCray, Astrophys. J. 542
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S. M. Carroll, J. A. Harvey, V. A. Kostelecky, C. D. Lane and T. Okamoto, Phys. Rev. Lett. 87
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2022

Probing bumblebee gravity with black hole X-ray data

Gu, Jiale, Riaz, Shafqat, Abdikamalov, Askar B. et al.

Understand

Bumblebee gravity is one of the simplest gravity theories with spontaneous Lorentz symmetry breaking.

Since we know a rotating black hole solution in bumblebee gravity, we can potentially test this model with the available astrophysical observations of black holes.
In this work, we construct a reflection model in bumblebee gravity and we use our model to analyze the reflection features of a NuSTAR spectrum of the Galactic black hole EXO 1846-031 in order to constrain the Lorentz-violating parameter $\ell$.
We find that the analysis of the reflection features in the spectrum of EXO 1846-031 cannot constrain the parameter $\ell$ because of a very strong degeneracy between the estimates of $\ell$ and of the black hole spin parameter $a_*$.

Built on

P. G. Ferreira, Ann. Rev. Astron. Astrophys. 57
Original
1902
Earlier work this paper cites.
A. B. Abdikamalov, D. Ayzenberg, C. Bambi, T. Dauser, J. A. Garcia and S. Nampalliwar, Astrophys. J. 878
Original
1902
Earlier work this paper cites.
M. Zhou, A. B. Abdikamalov, D. Ayzenberg, C. Bambi, H. Liu and S. Nampalliwar, Phys. Rev. D 99
Original
1903
Earlier work this paper cites.
K. Akiyama et al
Original
1906
Earlier work this paper cites.
C. Ding, C. Liu, R. Casana and A. Cavalcante, Eur. Phys. J. C 80
Original
1910
Earlier work this paper cites.
A. Einstein, Annalen Phys. 49
1916
Earlier work this paper cites.
R. W. Lindquist, Annals Phys. 37
1966
Earlier work this paper cites.
I. D. Novikov and K. S. Thorne, Astrophysics of black holes
1973
Earlier work this paper cites.
D. N. Page and K. S. Thorne, Astrophys. J. 191
1974
Earlier work this paper cites.
C. T. Cunningham, Astrophys. J. 202
1975
Earlier work this paper cites.
A. N. Parmar and N. E.White, International Astronomical Union Circular 4051
1985
Earlier work this paper cites.
K. Makishima, Y. Maejima, K. Mitsuda, H. V. Bradt, R. A. Remillard, I. R. Tuohy, R. Hoshi and M. Nakagawa, Astrophys. J. 308
1986
Earlier work this paper cites.
V. A. Kostelecky and S. Samuel, Phys. Rev. D 39
1989
Earlier work this paper cites.
V. A. Kostelecky and S. Samuel, Phys. Rev. D 40
1989
Earlier work this paper cites.
A. N. Parmar, L. Angelini, P. Roche and N. E. White, Astron. Astrophys. 279
1993
Earlier work this paper cites.
K. A. Arnaud, in Astronomical Data Analysis Software and Systems V
1996
Earlier work this paper cites.
R. Gambini and J. Pullin, Phys. Rev. D 59
1999
Earlier work this paper cites.
J. R. Ellis, N. E. Mavromatos and D. V. Nanopoulos, Gen. Rel. Grav. 32
2000
Earlier work this paper cites.