Tachyonic Kaluza-Klein modes and the AdS swampland conjecture

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作者
Emanuel Malek
Hermann Nicolai
Henning Samtleben
机构
[1] Max-Planck-Institut für Gravitationsphysik (Albert-Einstein-Institut),
[2] Univ Lyon,undefined
[3] Ens de Lyon,undefined
[4] Univ Claude Bernard,undefined
[5] CNRS,undefined
[6] Laboratoire de Physique,undefined
关键词
Flux compactifications; Supergravity Models; Superstring Vacua; Supersymmetry Breaking;
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摘要
We compute the Kaluza-Klein spectrum of the non-supersymmetric SO(3) × SO(3)-invariant AdS4 vacuum of 11-dimensional supergravity, whose lowest-lying Kaluza-Klein modes belong to a consistent truncation to 4-dimensional 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} = 8 supergravity and are stable. We show that, nonetheless, the higher Kaluza-Klein modes become tachyonic so that this non-supersymmetric AdS4 vacuum is perturbatively unstable within 11-dimensional supergravity. This represents the first example of unstable higher Kaluza-Klein modes and provides further evidence for the AdS swampland conjecture, which states that there are no stable non-supersymmetric AdS vacua within string theory. We also find 27 infinitesimal moduli amongst the Kaluza-Klein modes, which hints at the existence of a family of non-supersymmetric AdS4 vacua.
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