Erasure Thresholds for Hyperbolic and Semi-Hyperbolic Surface Codes

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1. Verfasser: Galimova, Aygul Azatovna
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Veröffentlicht: 2026
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author Galimova, Aygul Azatovna
author_facet Galimova, Aygul Azatovna
contents We extend the circuit-level erasure noise model and Wang et al.\ quadratic expansion fitting of Chang et al.\ from planar surface codes to hyperbolic CSS surface codes. Under Chang et al.'s noise models, the $\{8,3\}$ Bolza fine-grained family threshold reaches $3.6\%$ under the general-Pauli models (which coincide at temporal resolution $η= 1$) and $4.7\%$ under the tailored spatially perfect model at $R_e = 1$ (pure erasure). The corresponding erasure-to-Pauli ratios ($5.0\times$ and $6.5\times$) match the surface code values to within $5\%$. Per-observable crossing-point analysis at $R_e = 1$ (Models 1--3) independently yields an erasure-to-Pauli ratio of $5.3\times$. These results establish that the erasure advantage extends to hyperbolic codes.
format Preprint
id arxiv_https___arxiv_org_abs_2602_10423
institution arXiv
publishDate 2026
record_format arxiv
spellingShingle Erasure Thresholds for Hyperbolic and Semi-Hyperbolic Surface Codes
Galimova, Aygul Azatovna
Quantum Physics
We extend the circuit-level erasure noise model and Wang et al.\ quadratic expansion fitting of Chang et al.\ from planar surface codes to hyperbolic CSS surface codes. Under Chang et al.'s noise models, the $\{8,3\}$ Bolza fine-grained family threshold reaches $3.6\%$ under the general-Pauli models (which coincide at temporal resolution $η= 1$) and $4.7\%$ under the tailored spatially perfect model at $R_e = 1$ (pure erasure). The corresponding erasure-to-Pauli ratios ($5.0\times$ and $6.5\times$) match the surface code values to within $5\%$. Per-observable crossing-point analysis at $R_e = 1$ (Models 1--3) independently yields an erasure-to-Pauli ratio of $5.3\times$. These results establish that the erasure advantage extends to hyperbolic codes.
title Erasure Thresholds for Hyperbolic and Semi-Hyperbolic Surface Codes
topic Quantum Physics
url https://arxiv.org/abs/2602.10423