%0 Journal Article %1 Guica2010Holography %A Guica, Monica %A Skenderis, Kostas %A Taylor, Marika %A van Rees, Balt %D 2010 %K 3dgravity, arxiv, schrodinger, warped-bh %T Holography for Schrodinger backgrounds %U http://arxiv.org/abs/1008.1991 %X We discuss holography for Schrodinger solutions of both topologically massive gravity in three dimensions and massive vector theories in (d+1) dimensions. In both cases the dual field theory can be viewed as a d-dimensional conformal field theory (two dimensional in the case of TMG) deformed by certain operators that respect the Schrodinger symmetry. These operators are irrelevant from the viewpoint of the relativistic conformal group but they are exactly marginal with respect to the non-relativistic conformal group. The spectrum of linear fluctuations around the background solutions corresponds to operators that are labeled by their scaling dimension and the lightcone momentum k\_v. We set up the holographic dictionary and compute 2-point functions of these operators both holographically and in field theory using conformal perturbation theory and find agreement. The counterterms needed for holographic renormalization are non-local in the v lightcone direction.

@article{Guica2010Holography, abstract = {{We discuss holography for Schrodinger solutions of both topologically massive gravity in three dimensions and massive vector theories in (d+1) dimensions. In both cases the dual field theory can be viewed as a d-dimensional conformal field theory (two dimensional in the case of TMG) deformed by certain operators that respect the Schrodinger symmetry. These operators are irrelevant from the viewpoint of the relativistic conformal group but they are exactly marginal with respect to the non-relativistic conformal group. The spectrum of linear fluctuations around the background solutions corresponds to operators that are labeled by their scaling dimension and the lightcone momentum k\_v. We set up the holographic dictionary and compute 2-point functions of these operators both holographically and in field theory using conformal perturbation theory and find agreement. The counterterms needed for holographic renormalization are non-local in the v lightcone direction.}}, added-at = {2019-02-26T10:37:35.000+0100}, archiveprefix = {arXiv}, author = {Guica, Monica and Skenderis, Kostas and Taylor, Marika and van Rees, Balt}, biburl = {https://www.bibsonomy.org/bibtex/2b6412e5347ee991490b4815f6903c0c3/acastro}, citeulike-article-id = {7631284}, citeulike-linkout-0 = {http://arxiv.org/abs/1008.1991}, citeulike-linkout-1 = {http://arxiv.org/pdf/1008.1991}, day = 11, eprint = {1008.1991}, interhash = {a502fb1bf410bfa7254e8a3ed38cc5ac}, intrahash = {b6412e5347ee991490b4815f6903c0c3}, keywords = {3dgravity, arxiv, schrodinger, warped-bh}, month = aug, posted-at = {2010-08-13 15:14:43}, priority = {2}, timestamp = {2019-02-26T10:37:35.000+0100}, title = {{Holography for Schrodinger backgrounds}}, url = {http://arxiv.org/abs/1008.1991}, year = 2010 }