Spectrum universality properties of holographic Chern-Simons theories

被引:0
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作者
Yi Pang
Junchen Rong
Oscar Varela
机构
[1] Max-Planck-Institut für Gravitationsphysik (Albert-Einstein-Institut),Department of Physics
[2] Fields,Departmento de Fısica Teórica and Instituto de Física Teórica UAM/CSIC
[3] Gravity & Strings,undefined
[4] Center for Theoretical Physics of the Universe,undefined
[5] Institute for Basic Sciences,undefined
[6] Utah State University,undefined
[7] Universidad Autónoma de Madrid,undefined
关键词
AdS-CFT Correspondence; Chern-Simons Theories; Extended Supersymmetry; Supergravity Models;
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摘要
We give a master formula for the spin-2 spectrum of a class of three-dimensional Chern-Simons theories at large N , with flavour group containing SU(3), that arise as infrared fixed points of the D2-brane worldvolume field theory and have AdS4 duals in massive type IIA supergravity. We use this formula to compute the spin-2 spectrum of the individual theories, discuss its supermultiplet structure and, for an N\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$ \mathcal{N} $$\end{document} = 2 theory in this class, the spectrum of protected operators with spin 2. We also show that the trace of the Kaluza-Klein graviton mass matrix on the dual AdS4 solutions enjoys certain universality properties. These are shown to relate the class of AdS4 massive IIA solutions under consideration to a similar class of AdS4 solutions of D = 11 supergravity with the same symmetries. Finally, for the N\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$ \mathcal{N} $$\end{document} = 2 AdS4 solution in this class, we study the entire spectrum at lowest Kaluza-Klein level and relate it to an analogue solution in D = 11 supergravity.
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