3D supergravity from wrapped M5-branes

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作者
Parinya Karndumri
Eoin Ó Colgáin
机构
[1] Chulalongkorn University,Department of Physics, Faculty of Science
[2] SUNY,C.N.Yang Institute for Theoretical Physics
[3] University of Surrey,Department of Mathematics
[4] Korea Institute for Advanced Study,Kavli Institute for Theoretical Physics China, Institute for Theoretical Physics
[5] Chinese Academy of Sciences,undefined
关键词
AdS-CFT Correspondence; Supergravity Models; Classical Theories of Gravity; M-Theory;
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摘要
Through consistent Kaluza-Klein reduction, we construct 3D N=2\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$ \mathcal{N}=2 $$\end{document} gauged supergravities corresponding to twisted compactifications of M5-branes on a product of constant curvature Riemann surfaces, including Kähler-Einstein four-manifolds. We extend the reduction to fermionic supersymmetry variations in order to determine the 3D Killing spinor equations and classify all timelike supersymmetric solutions. As a by-product, we identify an infinite class of new supersymmetric warped AdS3 (Gödel) and warped dS3 solutions. Moreover, we show that the superpotential T encodes the central charge and R symmetry of the dual N=0,2\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$ \mathcal{N}=\left(0,\;2\right) $$\end{document} SCFTs in the large N limit. We demonstrate that the R symmetry matches the canonical U(1) isometry from existing classifications of supersymmetric AdS3 solutions to 11D supergravity with N=0,2\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$ \mathcal{N}=\left(0,\;2\right) $$\end{document} supersymmetry.
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