dc.contributor.author | Ganchev, B | |
dc.contributor.author | Giusto, S | |
dc.contributor.author | Houppe, A | |
dc.contributor.author | Russo, R | |
dc.contributor.author | Warner, NP | |
dc.date.accessioned | 2023-12-05T15:52:20Z | |
dc.date.available | 2023-12-05T15:52:20Z | |
dc.date.issued | 2023-10-01 | |
dc.identifier.uri | https://qmro.qmul.ac.uk/xmlui/handle/123456789/92638 | |
dc.description.abstract | Microstrata are the non-extremal analogues of superstrata: they are smooth, non-extremal (non-BPS) solitonic solutions to IIB supergravity whose deep-throat limits approximate black holes. Using perturbation theory and numerical methods, we construct families of solutions using a consistent truncation to three-dimensional supergravity. The most general families presented here involve two continuous parameters, or amplitudes, and four quantized parameters that set the angular momenta and energy levels. Our solutions are asymptotic to the vacuum of the D1-D5 system: AdS3 × S 3 × T4. Using holography, we show that the they are dual to multi-particle states in the D1-D5 CFT involving a large number of mutually non-BPS supergravitons and we determine the anomalous dimensions of these states from the binding energies in supergravity. These binding energies are uniformly negative and depend non-linearly on the amplitudes of the states. In one family of solutions, smoothness restricts some of the fields to lie on a special locus of the parameter space. Using precision holography we show that this special locus can be identified with the multi-particle states constructed via the standard OPE of the single-particle constituents. Our numerical analysis shows that microstrata are robust at large amplitudes and the solutions can be obtained to very high precision. | en_US |
dc.publisher | Springer Nature | en_US |
dc.relation.ispartof | Journal of High Energy Physics | |
dc.rights | 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. | |
dc.rights | Attribution 3.0 United States | * |
dc.rights.uri | http://creativecommons.org/licenses/by/3.0/us/ | * |
dc.title | Microstrata | en_US |
dc.type | Article | en_US |
dc.rights.holder | © 2023 The Author(s). Published by Springer Nature | |
dc.identifier.doi | 10.1007/JHEP10(2023)163 | |
pubs.issue | 10 | en_US |
pubs.notes | Not known | en_US |
pubs.publication-status | Published | en_US |
pubs.volume | 2023 | en_US |
rioxxterms.funder | Default funder | en_US |
rioxxterms.identifier.project | Default project | en_US |
qmul.funder | Amplitudes, Strings and Duality::Science and Technology Facilities Council | en_US |
qmul.funder | Amplitudes, Strings and Duality::Science and Technology Facilities Council | en_US |
qmul.funder | Amplitudes, Strings and Duality::Science and Technology Facilities Council | en_US |