AdS3×S2 in IIB with small N $$ \mathcal{N} $$ = (4, 0) supersymmetry

Abstract We consider warped AdS3×S2×M5 backgrounds in type II supergravity preserving small N $$ \mathcal{N} $$ = (4, 0) supersymmetry. We show that imposing N $$ \mathcal{N} $$ = (4, 0) supersymmetry imposes between 0 and 3 a priori isometries in the internal M5. In this work we focus on classes of...

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Main Authors: Niall T. Macpherson, Anayeli Ramirez
Format: Article
Language:English
Published: SpringerOpen 2022-04-01
Series:Journal of High Energy Physics
Subjects:
Online Access:https://doi.org/10.1007/JHEP04(2022)143
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author Niall T. Macpherson
Anayeli Ramirez
author_facet Niall T. Macpherson
Anayeli Ramirez
author_sort Niall T. Macpherson
collection DOAJ
description Abstract We consider warped AdS3×S2×M5 backgrounds in type II supergravity preserving small N $$ \mathcal{N} $$ = (4, 0) supersymmetry. We show that imposing N $$ \mathcal{N} $$ = (4, 0) supersymmetry imposes between 0 and 3 a priori isometries in the internal M5. In this work we focus on classes of solution where M5 exhibits no a priori isometry which imposes additional constraints. Solving these in IIA forces M5 to support an SU(2)-structure, a class already studied in [10], while in IIB one arrives at two broad new classes with identity-structure that we reduce to local expressions for the physical fields and PDEs.
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spelling doaj.art-aac851288aed462a84f1de0b24a47b7b2023-03-22T10:10:18ZengSpringerOpenJournal of High Energy Physics1029-84792022-04-012022413510.1007/JHEP04(2022)143AdS3×S2 in IIB with small N $$ \mathcal{N} $$ = (4, 0) supersymmetryNiall T. Macpherson0Anayeli Ramirez1Departamento de Física de Partículas Universidade de Santiago de Compostela, and Instituto Galego de Física de Altas Enerxías (IGFAE)Department of Physics, University of OviedoAbstract We consider warped AdS3×S2×M5 backgrounds in type II supergravity preserving small N $$ \mathcal{N} $$ = (4, 0) supersymmetry. We show that imposing N $$ \mathcal{N} $$ = (4, 0) supersymmetry imposes between 0 and 3 a priori isometries in the internal M5. In this work we focus on classes of solution where M5 exhibits no a priori isometry which imposes additional constraints. Solving these in IIA forces M5 to support an SU(2)-structure, a class already studied in [10], while in IIB one arrives at two broad new classes with identity-structure that we reduce to local expressions for the physical fields and PDEs.https://doi.org/10.1007/JHEP04(2022)143Flux CompactificationsAdS-CFT CorrespondenceExtended Supersymmetry
spellingShingle Niall T. Macpherson
Anayeli Ramirez
AdS3×S2 in IIB with small N $$ \mathcal{N} $$ = (4, 0) supersymmetry
Journal of High Energy Physics
Flux Compactifications
AdS-CFT Correspondence
Extended Supersymmetry
title AdS3×S2 in IIB with small N $$ \mathcal{N} $$ = (4, 0) supersymmetry
title_full AdS3×S2 in IIB with small N $$ \mathcal{N} $$ = (4, 0) supersymmetry
title_fullStr AdS3×S2 in IIB with small N $$ \mathcal{N} $$ = (4, 0) supersymmetry
title_full_unstemmed AdS3×S2 in IIB with small N $$ \mathcal{N} $$ = (4, 0) supersymmetry
title_short AdS3×S2 in IIB with small N $$ \mathcal{N} $$ = (4, 0) supersymmetry
title_sort ads3 s2 in iib with small n mathcal n 4 0 supersymmetry
topic Flux Compactifications
AdS-CFT Correspondence
Extended Supersymmetry
url https://doi.org/10.1007/JHEP04(2022)143
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