Non-linear perturbation of black branes at large D
Abstract The Einstein equations describing the black-brane dynamics both in Minkowski and AdS background were recently recast in the form of coupled diffusion equations in the large-D(imension) limit. Using such results in the literature, we formulate a higher-order perturbation theory of black bran...
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doaj-274acfe515d14a2fbaa41bceb61878d42020-11-25T00:34:36ZengSpringerOpenJournal of High Energy Physics1029-84792017-06-012017612510.1007/JHEP06(2017)033Non-linear perturbation of black branes at large DUmpei Miyamoto0RECCS, Akita Prefectural UniversityAbstract The Einstein equations describing the black-brane dynamics both in Minkowski and AdS background were recently recast in the form of coupled diffusion equations in the large-D(imension) limit. Using such results in the literature, we formulate a higher-order perturbation theory of black branes in time domain and present the general form of solutions for arbitrary initial conditions. For illustrative purposes, the solutions up to the first or second order are explicitly written down for several kind of initial conditions, such as a Gaussian wave packet, shock wave, and rather general superposed sinusoidal waves. These could be the first examples describing the non-trivial evolution of black-brane horizons in time domain. In particular, we learn some interesting aspects of black-brane dynamics such as the Gregory-Laflamme (GL) instability and non-equilibrium steady state (NESS). The formalism presented here would be applicable to the analysis of various black branes and their holographically dual field theories.http://link.springer.com/article/10.1007/JHEP06(2017)033Black HolesAdS-CFT CorrespondenceClassical Theories of Gravityp-branes |
collection |
DOAJ |
language |
English |
format |
Article |
sources |
DOAJ |
author |
Umpei Miyamoto |
spellingShingle |
Umpei Miyamoto Non-linear perturbation of black branes at large D Journal of High Energy Physics Black Holes AdS-CFT Correspondence Classical Theories of Gravity p-branes |
author_facet |
Umpei Miyamoto |
author_sort |
Umpei Miyamoto |
title |
Non-linear perturbation of black branes at large D |
title_short |
Non-linear perturbation of black branes at large D |
title_full |
Non-linear perturbation of black branes at large D |
title_fullStr |
Non-linear perturbation of black branes at large D |
title_full_unstemmed |
Non-linear perturbation of black branes at large D |
title_sort |
non-linear perturbation of black branes at large d |
publisher |
SpringerOpen |
series |
Journal of High Energy Physics |
issn |
1029-8479 |
publishDate |
2017-06-01 |
description |
Abstract The Einstein equations describing the black-brane dynamics both in Minkowski and AdS background were recently recast in the form of coupled diffusion equations in the large-D(imension) limit. Using such results in the literature, we formulate a higher-order perturbation theory of black branes in time domain and present the general form of solutions for arbitrary initial conditions. For illustrative purposes, the solutions up to the first or second order are explicitly written down for several kind of initial conditions, such as a Gaussian wave packet, shock wave, and rather general superposed sinusoidal waves. These could be the first examples describing the non-trivial evolution of black-brane horizons in time domain. In particular, we learn some interesting aspects of black-brane dynamics such as the Gregory-Laflamme (GL) instability and non-equilibrium steady state (NESS). The formalism presented here would be applicable to the analysis of various black branes and their holographically dual field theories. |
topic |
Black Holes AdS-CFT Correspondence Classical Theories of Gravity p-branes |
url |
http://link.springer.com/article/10.1007/JHEP06(2017)033 |
work_keys_str_mv |
AT umpeimiyamoto nonlinearperturbationofblackbranesatlarged |
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