{ "id": "1512.09055", "version": "v1", "published": "2015-12-30T18:43:06.000Z", "updated": "2015-12-30T18:43:06.000Z", "title": "Holography as a highly efficient RG flow II: An explicit construction", "authors": [ "Nicolas Behr", "Ayan Mukhopadhyay" ], "comment": "1+51 pages; can be read independently of part 1 of this work, which has been revised recently to make a better interphase with this work", "categories": [ "hep-th", "gr-qc" ], "abstract": "We complete the reformulation of the holographic correspondence as a \\emph{highly efficient RG flow} that can also determine the UV data in the field theory in the strong coupling and large $N$ limit. We introduce a special way to define operators at any given scale in terms of appropriate coarse-grained collective variables, without requiring the use of the elementary fields. The Wilsonian construction is generalised by promoting the cut-off to a functional of these collective variables. We impose three criteria to determine the coarse-graining. The first criterion is that the effective Ward identities for local conservation of energy, momentum, etc. should preserve their standard forms, but in new scale-dependent background metric and sources which are functionals of the effective single trace operators. The second criterion is that the scale-evolution equations of the operators in the actual background metric should be state-independent, implying that the collective variables should not explicitly appear in them. The final required criterion is that the endpoint of the scale-evolution of the RG flow can be transformed to a fixed point corresponding to familiar non-relativistic equations with a finite number of parameters, such as incompressible non-relativistic Navier-Stokes, under a certain universal rescaling of the scale and of the time coordinate. Using previous work, we explicitly show that in the hydrodynamic limit each such highly efficient RG flow reproduces a unique classical gravity theory with precise UV data that satisfy our IR criterion and also lead to regular horizons in the dual geometries. We obtain the explicit coarse-graining which reproduces Einstein's equations. Finally, we show how our construction can be interpolated with the traditional Wilsonian RG flow at a suitable scale, and can be used to develop new non-perturbative frameworks for QCD-like theories.", "revisions": [ { "version": "v1", "updated": "2015-12-30T18:43:06.000Z" } ], "analyses": { "keywords": [ "explicit construction", "collective variables", "highly efficient rg flow reproduces", "uv data", "background metric" ], "note": { "typesetting": "TeX", "pages": 51, "language": "en", "license": "arXiv", "status": "editable", "adsabs": "2015arXiv151209055B", "inspire": 1411634 } } }