Ultraspinning instability: the missing link
Ultraspinning instability: the missing link
We study linearized perturbations of Myers-Perry black holes in d = 7, with two of the three angular momenta set to be equal, and show that instabilities always appear before extremality. Analogous results are expected for all higher odd d. We determine numerically the stationary perturbations that mark the onset of instability for the modes that preserve the isometries of the background. The onset is continuously connected between the previously studied sectors of solutions with a single angular momentum and solutions with all angular momenta equal. This shows that the near-extremality instabilities are of the same nature as the ultraspinning instability of d ≥ 6 singly-spinning solutions, for which the angular momentum is unbounded. Our results raise the question of whether there are any extremal Myers-Perry black holes which are stable in d ≥ 6.
Dias, Oscar J.C.
f01a8d9b-9597-4c32-9226-53a6e5500a54
Monteiro, Ricardo
1dfb2954-9861-425f-82c5-75185a088b60
Santos, Jorge E.
88cca86d-9e1e-40a7-acba-f7986bd7f84b
30 August 2011
Dias, Oscar J.C.
f01a8d9b-9597-4c32-9226-53a6e5500a54
Monteiro, Ricardo
1dfb2954-9861-425f-82c5-75185a088b60
Santos, Jorge E.
88cca86d-9e1e-40a7-acba-f7986bd7f84b
Dias, Oscar J.C., Monteiro, Ricardo and Santos, Jorge E.
(2011)
Ultraspinning instability: the missing link.
JHEP, 2011 (08), [139].
(doi:10.1007/JHEP08(2011)139).
Abstract
We study linearized perturbations of Myers-Perry black holes in d = 7, with two of the three angular momenta set to be equal, and show that instabilities always appear before extremality. Analogous results are expected for all higher odd d. We determine numerically the stationary perturbations that mark the onset of instability for the modes that preserve the isometries of the background. The onset is continuously connected between the previously studied sectors of solutions with a single angular momentum and solutions with all angular momenta equal. This shows that the near-extremality instabilities are of the same nature as the ultraspinning instability of d ≥ 6 singly-spinning solutions, for which the angular momentum is unbounded. Our results raise the question of whether there are any extremal Myers-Perry black holes which are stable in d ≥ 6.
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Published date: 30 August 2011
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Copyright: SISSA 2011
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Local EPrints ID: 468067
URI: http://eprints.soton.ac.uk/id/eprint/468067
PURE UUID: c4edb7c9-4a0b-43b6-b725-9fdc4a264e72
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Date deposited: 29 Jul 2022 16:41
Last modified: 17 Mar 2024 03:35
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Author:
Ricardo Monteiro
Author:
Jorge E. Santos
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