Abstract
In a previous work of ours, the most general family of Kerr deformations—admitting a Carter constant—has been presented. This time a simple, necessary and sufficient condition in order for the aforementioned family to have a separable Klein-Gordon equation is exhibited. In addition, we provide a solid theoretical foundation that the maximum number of free to be chosen radial functions is three.
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Notes
In [17] a misunderstanding of the results published in [1] is apparent. More specifically, it is mentioned that according to [1] the Kerr-Sen metric [18] cannot be mapped to the Johannsen metric [2] and that in [17] it is proven to be possible. The correct statement in [1] is that the Killing tensor of the Kerr-Sen metric, which is of Petrov type I, is not induced by a Yano tensor—and thus, it is somehow more general than the rest of the examples, which are of the Petrov type D. Never the less the Johannsen metric is—in priciple—of Petrov type I as well and contains much freedom so that the Kerr-Sen metric can be considered as a member of the this family.
The exact form of g is quite extended to be written here.
References
Papadopoulos, G.O., Kokkotas, K.D.: Class. Quant. Grav. 35, 185014 (2018)
Johannsen, T.: Phys. Rev. D 88, 044002 (2013)
Abbott, B.P., Abbott, R., Abbott, T.D., Abernathy, M.R., Acernese, F., Ackley, K., Adams, C., Adams, T., Addesso, P., Adhikari, R.X., et al.: Phys. Rev. Lett. 116, 061102 (2016a)
Abbott, B.P., Abbott, R., Abbott, T.D., Abernathy, M.R., Acernese, F., Ackley, K., Adams, C., Adams, T., Addesso, P., Adhikari, R.X., et al.: Phys. Rev. Lett. 116, 221101 (2016b)
Event Horizon Telescope Collaboration, K. Akiyama, A. Alberdi, W. Alef, K. Asada, R. Azulay, A.-K. Baczko, D. Ball, M. Baloković, J. Barrett, et al., ApJ 875, L1 (2019)
Medeiros, L., Psaltis, D., Özel, F.: ApJ 896, 7 (2020)
Barack, L., Cardoso, V., Nissanke, S., Sotiriou, T.P., Askar, A., Belczynski, C., Bertone, G., Bon, E., Blas, D., Brito, R., et al.: Class. Quant. Grav. 36, 143001 (2019)
E. Barausse, E. Berti, T. Hertog, S. A. Hughes, P. Jetzer, P. Pani, T. P. Sotiriou, N. Tamanini, H. Witek, K. Yagi, et al., arXiv e-prints arXiv:2001.09793 (2020)
Okounkova, M., Stein, L.C., Moxon, J., Scheel, M.A., Teukolsky, S.A.: Phys. Rev. D 101, 104016 (2020)
Carter, B.: Phys. Rev. 174, 1559 (1968)
Ryan, F.D.: Phys. Rev. D 52, 5707 (1995)
Glampedakis, K., Babak, S.: Class. Quant. Grav. 23, 4167 (2006)
Collins, N.A., Hughes, S.A.: Phys. Rev. D 69, 124022 (2004)
Johannsen, T., Psaltis, D.: Phys. Rev. D 83, 124015 (2011)
Konoplya, R.A., Stuchlík, Z., Zhidenko, A.: Phys. Rev. D 97, 084044 (2018)
Shaikh, R.: Phys. Rev. D 100, 024028 (2019)
Carson, Z., Yagi, K.: Phys. Rev. D 101, 084030 (2020)
Sen, A.: Phys. Rev. Lett. 69, 1006 (1992)
Suvorov, A.G.: Phys. Rev. D 99, 124026 (2019)
Brill, D.R., Chrzanowski, P.L., Pereira, C.M., Fackerell, E.D., Ipser, J.R.: Phys. Rev. D 5, 1913 (1972)
Teukolsky, S.A.: Phys. Rev. Lett. 29, 1114 (1972)
Chen, C.-Y., Chen, P.: Phys. Rev. D 100, 104054 (2019)
Landau, L.D., Lifshitz, E.M.: The classical theory of fields. Pergamon Press (1975)
Acknowledgements
The authors are grateful to K. Destounis, S. Nampalliwar, K. Yagi and A. G. Suvorov for useful discussions. This work was supported by the DAAD program “Hochschulpartnerschaften mit Griechenland 2016” (Projekt 57340132). Networking support by the COST Action CA16104 is also gratefully acknowledged
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Papadopoulos, G.O., Kokkotas, K.D. On Kerr black hole deformations admitting a Carter constant and an invariant criterion for the separability of the wave equation. Gen Relativ Gravit 53, 21 (2021). https://doi.org/10.1007/s10714-021-02795-2
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DOI: https://doi.org/10.1007/s10714-021-02795-2