AdS nonlinear instability: moving beyond spherical symmetry
AdS nonlinear instability: moving beyond spherical symmetry
Anti-de Sitter (AdS) is conjectured to be nonlinear unstable to a weakly turbulent mechanism that develops a cascade towards high frequencies, leading to black hole formation. We give evidence that the gravitational sector of perturbations behaves differently from the scalar one studied by Bizon and Rostworowski. In contrast with Bizon and Rostworowski, we find that not all gravitational normal modes of AdS can be nonlinearly extended into periodic horizonless smooth solutions of the Einstein equation. In particular, we show that even seeds with a single normal mode can develop secular resonances, unlike the spherically symmetric scalar field collapse studied by Bizon and Rostworowski. Moreover, if the seed has two normal modes, more than one resonance can be generated at third order, unlike the spherical collapse of Bizon and Rostworowski. We also show that weak turbulent perturbative theory predicts the existence of direct and inverse cascades, with the former dominating the latter for equal energy two-mode seeds.
Dias, Oscar J. C.
f01a8d9b-9597-4c32-9226-53a6e5500a54
Santos, Jorge E.
6e5a1703-a14c-4ef6-bfe4-7e4c5177c274
8 November 2016
Dias, Oscar J. C.
f01a8d9b-9597-4c32-9226-53a6e5500a54
Santos, Jorge E.
6e5a1703-a14c-4ef6-bfe4-7e4c5177c274
Dias, Oscar J. C. and Santos, Jorge E.
(2016)
AdS nonlinear instability: moving beyond spherical symmetry.
Classical and Quantum Gravity, 33 (23), [23LT01].
(doi:10.1088/0264-9381/33/23/23LT01).
Abstract
Anti-de Sitter (AdS) is conjectured to be nonlinear unstable to a weakly turbulent mechanism that develops a cascade towards high frequencies, leading to black hole formation. We give evidence that the gravitational sector of perturbations behaves differently from the scalar one studied by Bizon and Rostworowski. In contrast with Bizon and Rostworowski, we find that not all gravitational normal modes of AdS can be nonlinearly extended into periodic horizonless smooth solutions of the Einstein equation. In particular, we show that even seeds with a single normal mode can develop secular resonances, unlike the spherically symmetric scalar field collapse studied by Bizon and Rostworowski. Moreover, if the seed has two normal modes, more than one resonance can be generated at third order, unlike the spherical collapse of Bizon and Rostworowski. We also show that weak turbulent perturbative theory predicts the existence of direct and inverse cascades, with the former dominating the latter for equal energy two-mode seeds.
Text
TurbulenceCascadeLetter_CQG_v2.pdf
- Accepted Manuscript
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Accepted/In Press date: 20 October 2016
e-pub ahead of print date: 8 November 2016
Published date: 8 November 2016
Organisations:
Applied Mathematics
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Local EPrints ID: 405796
URI: http://eprints.soton.ac.uk/id/eprint/405796
ISSN: 0264-9381
PURE UUID: 9ff74a6a-56e6-4be2-bdcb-25be3a2e3892
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Date deposited: 18 Feb 2017 00:21
Last modified: 16 Mar 2024 05:02
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Author:
Jorge E. Santos
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