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Taking the imaginary part of the second gives the asymptotic series for G>(ω,q=0) =2ImGret(ω) 1−e−βω, which is the same, up to corrections∼e−βωthat are nonperturbative at largeω, as that for2ImG ret(ω): G>(ω)∼ ∞∑ n=0 anω2ν−ndβ−nd Γ(1 + · 2048 · arXiv 2047.99999

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Imprint of the black hole singularity on thermal two-point functions

hep-th · 2025-10-24 · unverdicted · novelty 6.0

Thermal two-point functions in holographic AdS black holes receive exponentially small non-perturbative corrections controlled by null geodesics bouncing off the singularity.

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Imprint of the black hole singularity on thermal two-point functions hep-th · 2025-10-24 · unverdicted · none · ref 42
Thermal two-point functions in holographic AdS black holes receive exponentially small non-perturbative corrections controlled by null geodesics bouncing off the singularity.

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