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Supergravity Instabilities of Non-Supersymmetric Quantum Critical Points

High Energy Physics - Theory 2011-03-28 v1

Abstract

Motivated by the recent use of certain consistent truncations of M-theory to study condensed matter physics using holographic techniques, we study the SU(3)-invariant sector of four-dimensional, N=8 gauged supergravity and compute the complete scalar spectrum at each of the five non-trivial critical points. We demonstrate that the smaller SU(4)^- sector is equivalent to a consistent truncation studied recently by various authors and find that the critical point in this sector, which has been proposed as the ground state of a holographic superconductor, is unstable due to a family of scalars that violate the Breitenlohner-Freedman bound. We also derive the origin of this instability in eleven dimensions and comment on the generalization to other embeddings of this critical point which involve arbitrary Sasaki-Einstein seven manifolds. In the spirit of a resurging interest in consistent truncations, we present a formal treatment of the SU(3)-invariant sector as a U(1)xU(1) gauged N=2 supergravity theory coupled to one hypermultiplet.

Keywords

Cite

@article{arxiv.1006.2546,
  title  = {Supergravity Instabilities of Non-Supersymmetric Quantum Critical Points},
  author = {Nikolay Bobev and Nick Halmagyi and Krzysztof Pilch and Nicholas P. Warner},
  journal= {arXiv preprint arXiv:1006.2546},
  year   = {2011}
}

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46 pages