Abstract
We investigate the gauge/gravity duality between the mathcal{N} = 6 mass-deformed ABJM theory with hbox {U}_k(N)times hbox {U}_{-k}(N) gauge symmetry and the 11-dimensional supergravity on LLM geometries with SO(2,1)times SO(4)/{mathbb {Z}}_ktimes SO(4)/{mathbb {Z}}_k isometry, in terms of a KK holography, which involves quadratic order field redefinitions. We establish the quadratic order KK mappings for various gauge invariant fields in order to obtain the canonical 4-dimensional gravity equations of motion and to reduce the LLM solutions to an asymptotically AdS_4 gravity solutions. The non-linearity of the KK maps indicates that we can observe the true purpose of the non-linear KK holography of the LLM solutions. We read the vacuum expectation value of conformal dimension two operator from the asymptotically AdS_4 gravity solutions. For the LLM solutions which are represented by square-shaped Young diagrams, we compare the vacuum expectation value obtained from the holographic procedure with the result obtained from the field theory, which is given by langle mathcal{O}^{(Delta =2)}rangle =sqrt{k}N^{frac{3}{2}}f_{(Delta =2)}+mathcal{O}(N), where f_{Delta } is independent of N. Based on this result, we examine the gauge/gravity duality in the large N limit and finite k. We also show that the vacuum expectation values of the massive KK graviton modes are vanishing as expected by the supersymmetry.
Highlights
=2) + O(N ), where f is is given by independent of N
We obtained the vevs of gauge invariant operators up to μ20-order in terms of the holographic renormalization in the mABJM theory
We found that the vevs of gauge invariant operators are vanishing up to μ20-order expect for the case of the CPOs with conformal dimension = 1, 2
Summary
We discuss the compactification of 11dimensional gravity on S7/Zk. The compactification involves expansion of the 11-dimensional fluctuations in terms of the spherical harmonics on S7/Zk and projecting the equations of motions on those spherical harmonics to obtain the equations of motion for various KK modes. The resulting equations contain higher derivatives of those KK modes and the necessary KK maps are introduced for obtaining the canonical equations of motion of the 4-dimensional dynamical fields. The non-linear KK maps established are used in Sect. 4 to obtain the asymptotically AdS4 solutions of 4-dimensional gravity equations of motion from the KK reduction of the LLM solutions. The vev of the CPO of conformal dimension = 2 is read from such asymptotic solutions
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