Abstract

The “pole-skipping” phenomenon reflects that the retarded Green’s function is not unique at a pole-skipping point in momentum space (ω, k). We explore the universality of pole-skipping in different geometries. In holography, near horizon analysis of the bulk equation of motion is a more straightforward way to derive a pole-skipping point. We use this method in Lifshitz, AdS2 and Rindler geometries. We also study the complex hydrodynamic analyses and find that the dispersion relations in terms of dimensionless variables frac{omega }{2pi T} and frac{left|kright|}{2pi T} pass through pole-skipping points left(frac{omega_n}{2pi T},frac{left|{k}_nright|}{2pi T}right) at small ω and k in the Lifshitz background. We verify that the position of the pole-skipping points does not depend on the standard quantization or alternative quantization of the boundary theory in AdS2× ℝd−1 geometry. In the Rindler geometry, we cannot find the corresponding Green’s function to calculate pole-skipping points because it is difficult to impose the boundary condition. However, we can still obtain “special points” near the horizon where bulk equations of motion have two incoming solutions. These “special points” correspond to the nonuniqueness of the Green’s function in physical meaning from the perspective of holography.

Highlights

  • The “pole-skipping” phenomenon reflects that the retarded Green’s function is not unique at a pole-skipping point in momentum space (ω, k)

  • We study the complex hydrodynamic analyses and find that the dispersion relations in terms of dimensionless variables ω 2πT

  • We show that near horizon analysis applies to AdS spacetime and to Lifshitz and Rindler geometry

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Summary

Anisotropic system near Lifshitz points

We can calculate a Taylor series solution to the tensor mode hxy, Maxwell vector mode Ay equations of motion when the matrix equation (2.21) is satisfied. For the convenience of numerical calculation, we set the horizon radius r+ = 1 and L = 1. The first few elements of this matrix are shown below. For the perturbation along x-direction of tensor mode hxy in equation (2.28) with a = 0, the first few elements of this matrix are

Tensor-type perturbations
Maxwell vector mode
Maxwell scalar mode
Rindler geometry
Scalar field
Discussion and conclusion
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