Thermal chaos of a charged dilaton-AdS black hole in the extended phase space
Abstract We have studied thermal chaotic behavior in the extended phase space for a charged dilaton-AdS black hole by Melnikov method and present the effect of dilaton parameter on the thermal chaos. Our result show that for the temporal perturbation the thermal chaos in the charged dilaton-AdS blac...
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doaj-669ac025ecc04f12b61cf235af5df4582020-11-25T02:54:27ZengSpringerOpenEuropean Physical Journal C: Particles and Fields1434-60441434-60522020-03-0180311010.1140/epjc/s10052-020-7813-1Thermal chaos of a charged dilaton-AdS black hole in the extended phase spaceChaoqun Dai0Songbai Chen1Jiliang Jing2Institute of Physics and Department of Physics, Key Laboratory of Low Dimensional Quantum Structures and Quantum Control of Ministry of Education, Synergetic Innovation Center for Quantum Effects and Applications, Hunan Normal UniversityInstitute of Physics and Department of Physics, Key Laboratory of Low Dimensional Quantum Structures and Quantum Control of Ministry of Education, Synergetic Innovation Center for Quantum Effects and Applications, Hunan Normal UniversityInstitute of Physics and Department of Physics, Key Laboratory of Low Dimensional Quantum Structures and Quantum Control of Ministry of Education, Synergetic Innovation Center for Quantum Effects and Applications, Hunan Normal UniversityAbstract We have studied thermal chaotic behavior in the extended phase space for a charged dilaton-AdS black hole by Melnikov method and present the effect of dilaton parameter on the thermal chaos. Our result show that for the temporal perturbation the thermal chaos in the charged dilaton-AdS black hole occurs only if the perturbation amplitude is larger than certain a critical value, but for the spatially perturbation, the chaos always exists irrespective of perturbation amplitude. These behaviors are similar to those in other AdS black hole, which can be regarded as the common features of the static AdS black holes. Moreover, we also find that the critical temporal perturbation amplitude leading to chaos increases with the dilaton parameter and decreases with the charge. This means that under the temporal perturbation the presence of dilaton parameter makes the onset of chaos more difficult, which differs from that of the charge parameter.http://link.springer.com/article/10.1140/epjc/s10052-020-7813-1 |
collection |
DOAJ |
language |
English |
format |
Article |
sources |
DOAJ |
author |
Chaoqun Dai Songbai Chen Jiliang Jing |
spellingShingle |
Chaoqun Dai Songbai Chen Jiliang Jing Thermal chaos of a charged dilaton-AdS black hole in the extended phase space European Physical Journal C: Particles and Fields |
author_facet |
Chaoqun Dai Songbai Chen Jiliang Jing |
author_sort |
Chaoqun Dai |
title |
Thermal chaos of a charged dilaton-AdS black hole in the extended phase space |
title_short |
Thermal chaos of a charged dilaton-AdS black hole in the extended phase space |
title_full |
Thermal chaos of a charged dilaton-AdS black hole in the extended phase space |
title_fullStr |
Thermal chaos of a charged dilaton-AdS black hole in the extended phase space |
title_full_unstemmed |
Thermal chaos of a charged dilaton-AdS black hole in the extended phase space |
title_sort |
thermal chaos of a charged dilaton-ads black hole in the extended phase space |
publisher |
SpringerOpen |
series |
European Physical Journal C: Particles and Fields |
issn |
1434-6044 1434-6052 |
publishDate |
2020-03-01 |
description |
Abstract We have studied thermal chaotic behavior in the extended phase space for a charged dilaton-AdS black hole by Melnikov method and present the effect of dilaton parameter on the thermal chaos. Our result show that for the temporal perturbation the thermal chaos in the charged dilaton-AdS black hole occurs only if the perturbation amplitude is larger than certain a critical value, but for the spatially perturbation, the chaos always exists irrespective of perturbation amplitude. These behaviors are similar to those in other AdS black hole, which can be regarded as the common features of the static AdS black holes. Moreover, we also find that the critical temporal perturbation amplitude leading to chaos increases with the dilaton parameter and decreases with the charge. This means that under the temporal perturbation the presence of dilaton parameter makes the onset of chaos more difficult, which differs from that of the charge parameter. |
url |
http://link.springer.com/article/10.1140/epjc/s10052-020-7813-1 |
work_keys_str_mv |
AT chaoqundai thermalchaosofachargeddilatonadsblackholeintheextendedphasespace AT songbaichen thermalchaosofachargeddilatonadsblackholeintheextendedphasespace AT jiliangjing thermalchaosofachargeddilatonadsblackholeintheextendedphasespace |
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1724721141070692352 |