Pith. sign in

AdS/CFT correspondence, quasinormal modes, and thermal correlators in N=4 SYM

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

4 Pith papers citing it
abstract

We use the Lorentzian AdS/CFT prescription to find the poles of the retarded thermal Green's functions of ${\cal N=4}$ SU(N) SYM theory in the limit of large N and large 't Hooft coupling. In the process, we propose a natural definition for quasinormal modes in an asymptotically AdS spacetime, with boundary conditions dictated by the AdS/CFT correspondence. The corresponding frequencies determine the dispersion laws for the quasiparticle excitations in the dual finite-temperature gauge theory. Correlation functions of operators dual to massive scalar, vector and gravitational perturbations in a five-dimensional AdS-Schwarzschild background are considered. We find asymptotic formulas for quasinormal frequencies in the massive scalar and tensor cases, and an exact expression for vector perturbations. In the long-distance, low-frequency limit we recover results of the hydrodynamic approximation to thermal Yang-Mills theory.

citation-role summary

background 2

citation-polarity summary

fields

hep-th 3 gr-qc 1

roles

background 2

polarities

background 2

representative citing papers

Analytic approaches to perturbations of strongly coupled Yang-Mills plasma

hep-th · 2026-06-10 · conditional · novelty 7.0

Scalar-channel quasinormal modes of the planar AdS5 black brane are captured across all wave numbers by exact WKB quantisation, transseries resummation, and Seiberg–Witten analytic continuation, with resummed large-q predictions matching independent numerics to ten to thirty decimal places.

Bouncing singularities and thermal correlators on line defects

hep-th · 2026-03-11 · accept · novelty 7.0

Retarded correlators of bulk scalars and Wilson-line displacement operators exhibit bouncing singularities at t_c=β/2(1+i) with matching WKB and asymptotic OPE data, implying a universal high-frequency factorization.

Quasinormal modes of black holes and black branes

gr-qc · 2009-05-19 · unverdicted · novelty 2.0

Quasinormal modes are eigenmodes of dissipative gravitational systems whose spectra encode near-equilibrium transport coefficients in dual quantum field theories and enable tests of general relativity through gravitational wave observations.

citing papers explorer

Showing 4 of 4 citing papers.

  • Analytic approaches to perturbations of strongly coupled Yang-Mills plasma hep-th · 2026-06-10 · conditional · none · ref 5 · internal anchor

    Scalar-channel quasinormal modes of the planar AdS5 black brane are captured across all wave numbers by exact WKB quantisation, transseries resummation, and Seiberg–Witten analytic continuation, with resummed large-q predictions matching independent numerics to ten to thirty decimal places.

  • Bouncing singularities and thermal correlators on line defects hep-th · 2026-03-11 · accept · none · ref 83 · internal anchor

    Retarded correlators of bulk scalars and Wilson-line displacement operators exhibit bouncing singularities at t_c=β/2(1+i) with matching WKB and asymptotic OPE data, implying a universal high-frequency factorization.

  • Effect of non-conformal deformation on the gapped quasi-normal modes and the holographic implications hep-th · 2025-06-11 · unverdicted · none · ref 83 · internal anchor

    Non-conformal deformation via Einstein-dilaton gravity increases the radius of convergence of the derivative expansion for gapped quasinormal modes of a scalar operator in the holographic dual.

  • Quasinormal modes of black holes and black branes gr-qc · 2009-05-19 · unverdicted · none · ref 101

    Quasinormal modes are eigenmodes of dissipative gravitational systems whose spectra encode near-equilibrium transport coefficients in dual quantum field theories and enable tests of general relativity through gravitational wave observations.