Exponentially small high-frequency corrections to holographic thermal correlators are computed from null geodesics reflecting at the black hole singularity, with numerically verified reflection coefficients.
At orderϵ0, the solution to (A1) are Bessel/Hankel func- tions
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Imprint of the black hole singularity on thermal two-point functions
Exponentially small high-frequency corrections to holographic thermal correlators are computed from null geodesics reflecting at the black hole singularity, with numerically verified reflection coefficients.