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Non-relativistic holography

7 Pith papers cite this work. Polarity classification is still indexing.

7 Pith papers citing it
abstract

We consider holography for d-dimensional scale invariant but non-Lorentz invariant field theories, which do not admit the full Schrodinger symmetry group. We find new realizations of the corresponding (d+1)-dimensional gravity duals, engineered with a variety of matter Lagrangians, and their finite temperature generalizations. The thermodynamic properties of the finite temperature backgrounds are precisely those expected for anisotropic, scale invariant field theories. The brane and string theory realizations of such backgrounds are briefly discussed, along with their holographic interpretation in terms of marginal but non Lorentz invariant deformations of conformal field theories. We initiate discussion of holographic renormalization in these backgrounds, and note that such systematic renormalization is necessary to obtain the correct behavior of correlation functions.

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hep-th 6 gr-qc 1

years

2026 6 2025 1

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background 2

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representative citing papers

Non-Relativistic Chern-Simons Supergravity with Torsion

hep-th · 2026-04-27 · unverdicted · novelty 7.0

A parameterized family of non-relativistic supergravity theories with torsion is obtained in three dimensions from the semigroup expansion of an N=2 supersymmetric Mielke-Baekler algebra.

Minisuperspace Double Copy in Lifshitz Spacetimes

hep-th · 2026-04-23 · unverdicted · novelty 6.0

A radial operator extracted from the reduced gravitational dynamics in Lifshitz spacetimes directly reproduces the Maxwell operator for the temporal single-copy field without using equations of motion.

Weyl double copy in Lifshitz spacetimes

hep-th · 2025-11-01 · unverdicted · novelty 5.0

The regularization prescription for the Weyl double copy restores consistency with the Kerr-Schild double copy across three distinct Lifshitz black hole examples.

Quintic Modification to Lifshitz Quasi-topological Black Holes

gr-qc · 2026-06-23 · unverdicted · novelty 4.0

Numerical solutions for quintic quasi-topological Lifshitz black holes in 5D with massive vector field are built via near-horizon expansion and shooting, yielding positive heat capacity for representative parameters across z=1,2 and k=-1,0,1.

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Showing 7 of 7 citing papers.