Information flows in strongly coupled ABJM theory
| dc.contributor.affiliation | Universidade de Santiago de Compostela. Departamento de Física de Partículas | gl |
| dc.contributor.affiliation | Universidade de Santiago de Compostela. Instituto Galego de Física de Altas Enerxías (IGFAE) | gl |
| dc.contributor.author | Balasubramanian, Vijay | |
| dc.contributor.author | Jokela, Niko | |
| dc.contributor.author | Ponni, Arttu | |
| dc.contributor.author | Vázquez Ramallo, Alfonso | |
| dc.date.accessioned | 2020-04-09T07:27:08Z | |
| dc.date.available | 2020-04-09T07:27:08Z | |
| dc.date.issued | 2019 | |
| dc.description.abstract | We use holographic methods to characterize the RG flow of quantum information in a Chern-Simons theory coupled to massive fermions. First, we use entanglement entropy and mutual information between strips to derive the dimension of the RG-driving operator and a monotonic c-function. We then display a scaling regime where, unlike in a CFT, the mutual information between strips changes non-monotonically with strip width, vanishing in both IR and UV but rising to a maximum at intermediate scales. The associated information transitions also contribute to non-monotonicity in the conditional mutual information which characterizes the independence of neighboring strips after conditioning on a third. Finally, we construct a measure of extensivity which tests to what extent information that region A shares with regions B and C is additive. In general, mutual information is super-extensive in holographic theories, and we might expect super-extensivity to be maximized in CFTs since they are scale-free. Surprisingly, our massive theory is more super-extensive than a CFT in a range of scales near the UV limit, although it is less super-extensive than a CFT at all lower scales. Our analysis requires the full ten-dimensional dual gravity background, and the extremal surfaces computing entanglement entropy explore all of these dimensions | gl |
| dc.description.peerreviewed | SI | gl |
| dc.description.sponsorship | A. V. R. is funded by the Spanish grants FPA2014- 52218-P and FPA2017-84436-P by Xunta de Galicia (GRC2013-024), by FEDER and by the Maria de Maeztu Unit of Excellence MDM-2016-0692. V. B. was supported in part by the Simons Foundation (# 385592, V. B.) through the It From Qubit Simons Collaboration, and the US Department of Energy grant FG02-05ER-41367. V. B. also acknowledges the hospitality of the Aspen Center for Physics which is supported by National Science Foundation grant PHY-1607611 | gl |
| dc.identifier.citation | Balasubramanian, V., Jokela, N., Pönni, A. et al. Information flows in strongly coupled ABJM theory. J. High Energ. Phys. 2019, 232 (2019). https://doi.org/10.1007/JHEP01(2019)232 | gl |
| dc.identifier.doi | 10.1007/JHEP01(2019)232 | |
| dc.identifier.essn | 1029-8479 | |
| dc.identifier.uri | http://hdl.handle.net/10347/21289 | |
| dc.language.iso | eng | gl |
| dc.publisher | Springer | gl |
| dc.relation.projectID | info:eu-repo/grantAgreement/AEI/Plan Estatal de Investigación Científica y Técnica y de Innovación 2017-2020/FPA2017-84436-P/ES/HOLOGRAFIA, GRAVITACION Y TEORIAS GAUGE | |
| dc.relation.publisherversion | https://doi.org/10.1007/JHEP01(2019)232 | gl |
| dc.rights | © 2019 The Authors. Open Access. This article is distributed under the terms of the Creative Commons Attribution License (CC-BY 4.0), which permits any use, distribution and reproduction in any medium, provided the original author(s) and source are credited. | gl |
| dc.rights.accessRights | open access | gl |
| dc.rights.uri | https://creativecommons.org/licenses/by/4.0/ | |
| dc.subject | AdS-CFT correspondence | gl |
| dc.subject | D-branes | gl |
| dc.title | Information flows in strongly coupled ABJM theory | gl |
| dc.type | journal article | gl |
| dc.type.hasVersion | VoR | gl |
| dspace.entity.type | Publication | |
| relation.isAuthorOfPublication | b74f5b8d-b125-4ddf-864f-737bd61efc6e | |
| relation.isAuthorOfPublication.latestForDiscovery | b74f5b8d-b125-4ddf-864f-737bd61efc6e |
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