We develop a systematic analytic method for studying high-order pole skipping in near-extremal holographic black holes. In the near-extremal regime, approaching the limit $T\to 0$, the near-horizon geometry develops an approximately ${\mathrm{AdS}}_2\times {\mathbb{R}}^{d-1}$ structure; we show that the mode index $q$ labeling pole skipping points is identified with the IR conformal dimension ${\mathrm{\Delta }}_{\mathrm{IR}}=q$ in the emergent ${\mathrm{AdS}}_2/{\mathrm{CFT}}_1$ correspondence, providing a concrete physical interpretation of the subleading pole skipping tower. The method reorganizes the near-horizon Frobenius expansion according to powers of temperature. This reveals a temperature-graded hierarchical structure that reduces the $n$th-order pole skipping condition to a factorized algebraic equation: each pole skipping momentum depends only on the mode index $q$, not on the order $n$. This $n$-independence produces a high degeneracy as $T\to 0$, where pole skipping momenta at all orders collapse onto a discrete set of values determined by near-horizon geometry and the scalar field mass; these values can be expressed in terms of thermodynamic quantities such as entropy density and specific heat. In the limit $n\gg 1$ (with $nT$ remaining small), the leading pole skipping momenta grow asymptotically as $k_{n,n}\propto n$. We compute leading temperature corrections and verify our predictions through numerical analysis of the dyonic Gubser-Rocha model. The results confirm that high-order pole skipping at low temperature is governed by near-horizon physics. This provides analytic access to pole-skipping points well beyond those accessible by standard determinant methods and clarifies the structure of holographic Green’s functions in the low-temperature regime.

Close

PrevNext

View figure in article

• General relativity
• Quantum aspects of black holes
• Quantum fields in curved spacetime
• Quantum gravity