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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Main Authors: Kanato Goto, Hugo Marrochio, Robert C. Myers, Leonel Queimada, Beni Yoshida
Format: Article
Language:English
Published: SpringerOpen 2019-02-01
Series:Journal of High Energy Physics
Subjects:
Online Access:http://link.springer.com/article/10.1007/JHEP02(2019)160
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spelling 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
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