2011
DOI: 10.1007/jhep08(2011)140
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Holographic striped phases

Abstract: We discuss new types of instabilities of D = 4 electrically charged AdSReissner-Nordström black branes that involve neutral pseudo-scalars. The instabilities spontaneously break translational invariance and are associated with the dual three-dimensional CFTs, at finite temperature and fixed chemical potential with respect to a global abelian symmetry, acquiring striped phases. We show that such instabilities are present for the infinite class of skew-whiffed AdS 4 ×SE 7 solutions of D = 11 supergravity, albeit… Show more

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Cited by 172 publications
(300 citation statements)
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“…This instability leads to a modulated phase where translation invariance in one of the spatial directions is broken. (The study of a three space-time dimensional analogue of this instability can be found in, for example, [44,45]. )…”
Section: Introductionmentioning
confidence: 99%
“…This instability leads to a modulated phase where translation invariance in one of the spatial directions is broken. (The study of a three space-time dimensional analogue of this instability can be found in, for example, [44,45]. )…”
Section: Introductionmentioning
confidence: 99%
“…Field theory models of non Fermi liquids often have relevant operators and suffer from symmetry-breaking instabilities as the temperature is lowered. Similar issues are encountered in the gravity side, for instance with superconducting [21][22][23] or translation-breaking [24] instabilities. While these instabilities can lead to interesting broken phases, it is important to develop tools to stabilize symmetric…”
Section: Jhep10(2013)126mentioning
confidence: 98%
“…To establish this, it is important that KK modes decouple. There could also be inhomogeneous instabilities, like the one found in [24], but our analysis so far shows that there can be stable solutions [72].…”
Section: Ads 2 × R 2 Fixed Pointmentioning
confidence: 99%
“…4 In summary, from solutions (19) and (20) we note that these TsT spacetimes supported by nontrivial string fields would have a Lifshitz (a = 3) or asymptotic Schroedinger symmetries (a = 2) depending upon the presence of B field in them. Particularly background (20) is a nontrivial solitonic configuration with B-field for which as we go from IR region to the UV region, it basically flows to a Schrödinger spacetime (with a = 2). The corresponding holographic dual will be a nonrelativistic CFT at zero temperature with suitable operater deformation giving rise to this flow.…”
Section: Vanishing Horizon Limits Of Tst Backgroundmentioning
confidence: 99%
“…These solutions require nontrivial dilaton field as well as metric deformations. Such solutions are further generalised in [20]. These recent Lifshitz solutions do avoid the early 'no-go' results of [24] because the field ansätze are some what less restrictive.…”
Section: Introductionmentioning
confidence: 99%