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dc.contributor.authorAnninos, Den_US
dc.contributor.authorAnous, Ten_US
dc.contributor.authorD’Agnolo, RTen_US
dc.date.accessioned2024-03-26T08:18:28Z
dc.date.issued2017-12-01en_US
dc.identifier.issn1126-6708en_US
dc.identifier.urihttps://qmro.qmul.ac.uk/xmlui/handle/123456789/95699
dc.description.abstractMotivated by the near-horizon geometry of four-dimensional extremal black holes, we study a disordered quantum mechanical system invariant under a global SU(2) symmetry. As in the Sachdev-Ye-Kitaev model, this system exhibits an approximate SL(2, ℝ) symmetry at low energies, but also allows for a continuous family of SU(2) breaking marginal deformations. Beyond a certain critical value for the marginal coupling, the model exhibits a quantum phase transition from the gapless phase to a gapped one and we calculate the critical exponents of this transition. We also show that charged, rotating extremal black holes exhibit a transition when the angular velocity of the horizon is tuned to a certain critical value. Where possible we draw parallels between the disordered quantum mechanics and charged, rotating black holes.en_US
dc.relation.ispartofJournal of High Energy Physicsen_US
dc.rightsThis article is distributed under the terms of the Creative Commons Attribution 4.0 International License (https://creativecommons.org/licenses/by/4.0), which permits use, duplication, adaptation, distribution, and reproduction in any medium or format, as long as you give appropriate credit to the original author(s) and the source, provide a link to the Creative Commons license, and indicate if changes were made.
dc.titleMarginal deformations & rotating horizonsen_US
dc.typeArticle
dc.identifier.doi10.1007/JHEP12(2017)095en_US
pubs.issue12en_US
pubs.notesNot knownen_US
pubs.publication-statusPublisheden_US
pubs.volume2017en_US
rioxxterms.funderDefault funderen_US
rioxxterms.identifier.projectDefault projecten_US


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