Holographic complexity equals which action?
Abstract We revisit the complexity = action proposal for charged black holes. We investigate the complexity for a dyonic black hole, and we find the surprising feature that the late-time growth is sensitive to the ratio between electric and magnetic charges. In particular, the late-time growth rate...
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Online Access: | http://link.springer.com/article/10.1007/JHEP02(2019)160 |
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doaj-415e0386074243d993326637eeb752a02020-11-25T01:24:54ZengSpringerOpenJournal of High Energy Physics1029-84792019-02-012019215710.1007/JHEP02(2019)160Holographic complexity equals which action?Kanato Goto0Hugo Marrochio1Robert C. Myers2Leonel Queimada3Beni Yoshida4The University of TokyoPerimeter Institute for Theoretical PhysicsPerimeter Institute for Theoretical PhysicsPerimeter Institute for Theoretical PhysicsPerimeter Institute for Theoretical PhysicsAbstract We revisit the complexity = action proposal for charged black holes. We investigate the complexity for a dyonic black hole, and we find the surprising feature that the late-time growth is sensitive to the ratio between electric and magnetic charges. In particular, the late-time growth rate vanishes when the black hole carries only a magnetic charge. If the dyonic black hole is perturbed by a light shock wave, a similar feature appears for the switchback effect, e.g. it is absent for purely magnetic black holes. We then show how the inclusion of a surface term to the action can put the electric and magnetic charges on an equal footing, or more generally change the value of the late-time growt rate. Next, we investigate how the causal structure influences the late-time growth with and without the surface term for charged black holes in a family of Einstein-Maxwell-Dilaton theories. Finally, we connect the previous discussion to the complexity=action proposal for the two-dimensional Jackiw-Teitelboim theory. Since the two-dimensional theory is obtained by a dimensional reduction from Einstein-Maxwell theory in higher dimensions in a near-extremal and near-horizon limit, the choices of parent action and parent background solution determine the behaviour of holographic complexity in two dimensions.http://link.springer.com/article/10.1007/JHEP02(2019)160AdS-CFT CorrespondenceBlack HolesBlack Holes in String Theory |
collection |
DOAJ |
language |
English |
format |
Article |
sources |
DOAJ |
author |
Kanato Goto Hugo Marrochio Robert C. Myers Leonel Queimada Beni Yoshida |
spellingShingle |
Kanato Goto Hugo Marrochio Robert C. Myers Leonel Queimada Beni Yoshida Holographic complexity equals which action? Journal of High Energy Physics AdS-CFT Correspondence Black Holes Black Holes in String Theory |
author_facet |
Kanato Goto Hugo Marrochio Robert C. Myers Leonel Queimada Beni Yoshida |
author_sort |
Kanato Goto |
title |
Holographic complexity equals which action? |
title_short |
Holographic complexity equals which action? |
title_full |
Holographic complexity equals which action? |
title_fullStr |
Holographic complexity equals which action? |
title_full_unstemmed |
Holographic complexity equals which action? |
title_sort |
holographic complexity equals which action? |
publisher |
SpringerOpen |
series |
Journal of High Energy Physics |
issn |
1029-8479 |
publishDate |
2019-02-01 |
description |
Abstract We revisit the complexity = action proposal for charged black holes. We investigate the complexity for a dyonic black hole, and we find the surprising feature that the late-time growth is sensitive to the ratio between electric and magnetic charges. In particular, the late-time growth rate vanishes when the black hole carries only a magnetic charge. If the dyonic black hole is perturbed by a light shock wave, a similar feature appears for the switchback effect, e.g. it is absent for purely magnetic black holes. We then show how the inclusion of a surface term to the action can put the electric and magnetic charges on an equal footing, or more generally change the value of the late-time growt rate. Next, we investigate how the causal structure influences the late-time growth with and without the surface term for charged black holes in a family of Einstein-Maxwell-Dilaton theories. Finally, we connect the previous discussion to the complexity=action proposal for the two-dimensional Jackiw-Teitelboim theory. Since the two-dimensional theory is obtained by a dimensional reduction from Einstein-Maxwell theory in higher dimensions in a near-extremal and near-horizon limit, the choices of parent action and parent background solution determine the behaviour of holographic complexity in two dimensions. |
topic |
AdS-CFT Correspondence Black Holes Black Holes in String Theory |
url |
http://link.springer.com/article/10.1007/JHEP02(2019)160 |
work_keys_str_mv |
AT kanatogoto holographiccomplexityequalswhichaction AT hugomarrochio holographiccomplexityequalswhichaction AT robertcmyers holographiccomplexityequalswhichaction AT leonelqueimada holographiccomplexityequalswhichaction AT beniyoshida holographiccomplexityequalswhichaction |
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1725116396994560000 |