2018
DOI: 10.1007/jhep04(2018)134
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Membrane paradigm and RG flows for anomalous holographic theories

Abstract: Holographic RG flows can be better understood with the help of radially conserved charges. It was shown by various authors that the bulk gauge and diffeomorphism symmetries lead to the conservation of the zero mode of the holographic U (1) current and, if the spacetime is stationary, to that of the holographic heat current. In describing dual theories with 't Hooft anomalies the bulk gauge invariance is broken by Chern-Simons terms. We show that conservation laws can still be derived and used to characterize t… Show more

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Cited by 5 publications
(3 citation statements)
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“…We note that there are additional terms in energy-momentum tensor proportional to the gravitational anomaly that were calculated in [54,55]. These terms contribute to the chiral magnetic conductivity in holographic model with momentum relaxation.…”
Section: Jhep08(2021)007mentioning
confidence: 75%
“…We note that there are additional terms in energy-momentum tensor proportional to the gravitational anomaly that were calculated in [54,55]. These terms contribute to the chiral magnetic conductivity in holographic model with momentum relaxation.…”
Section: Jhep08(2021)007mentioning
confidence: 75%
“…Therefore, Dirichlet boundary conditions can be fixed either to the metric or to the gauge field, but not simultaneously to both. This fact resemble the case in AdS 5 with the mixed gauge-gravitational Chern-Simons term [57][58][59], where a Gibbons-Hawking like term can be added but nonetheless, the regularity of the variational problem is not resolved. From a practical point of view, and in the context that concerns us, adding or not δS GH does not affect the observables because the near boundary behaviour of the fields in an asymptotically locally AdS space is such that this boundary term always vanishes, as we discuss below.…”
Section: Discussionmentioning
confidence: 97%
“…the extrinsic curvature acts like an external source conjugate to the operator u µν . We will define the holographic energy-momentum tensor as [19,22] T µ…”
Section: Holographic Energy-momentum Tensormentioning
confidence: 99%