Flowing to Higher Dimensions: A New Strongly-Coupled Phase on M2 Branes

preprint2015arXivOpen access

Abstract

We describe a one-parameter family of new holographic RG flows that start from AdS4×S7AdS_4 \times S^7 and go to AdS5^×B6\widehat{AdS_5} \times {\cal B}_6, where B6{\cal B}_6 is conformal to a Kähler manifold and AdS5^\widehat{AdS_5} is Poincaré AdS5AdS_5 with one spatial direction compactified and fibered over B6{\cal B}_6. The new solutions "flow up dimensions," going from the (2+1)(2+1)-dimensional conformal field theory on M2 branes in the UV to a (3+1)(3+1)-dimensional field theory on intersecting M5 branes in the infra-red. The M2 branes completely polarize into M5 branes along the flow and the Poincaré sections of the AdS5^\widehat{AdS_5} are the (3+1)(3+1)-dimensional common intersection of the M5 branes. The emergence of the extra dimension in the infra-red suggests a new strongly-coupled phase of the M2 brane and ABJM theories in which charged solitons are becoming massless. The flow solution is first analyzed by finding a four-dimensional N ⁣= ⁣2N \! = \! 2 supersymmetric flow in N ⁣= ⁣8N \! = \! 8 gauged supergravity. This is then generalized to a one parameter family of non-supersymmetric flows. The infra-red limit of the solutions appears to be quite singular in four dimensions but the uplift to eleven-dimensional supergravity is remarkable and regular (up to orbifolding). Our construction is a non-trivial application of the recently derived uplift formulae for fluxes, going well beyond the earlier constructions of stationary points solutions. The eleven-dimensional supersymmetry is also analyzed and shows how, for the supersymmetric flow, the M2-brane supersymmetry in the UV is polarized entirely into M5-brane supersymmetry in the infra-red.

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