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arXiv 2406.11533quant-ph
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使用 Classical Shadows 的高维子空间展开

High-Dimensional Subspace Expansion Using Classical Shadows

Gregory Boyd, Bálint Koczor, Zhenyu Cai

AI总结:

本文提出面向 classical shadow 数据的正则化高维子空间展开后处理方法,在不增加量子资源的前提下稳定降低基态能量估计误差,并证明其噪声鲁棒性与性能保证。

摘要:

我们提出了一种针对 classical shadow 测量数据的后处理技术,该技术通过高维子空间展开来提高基态估计的精度;其维度仅受经典后处理资源量的限制,而不受量子资源限制。我们方法的关键步骤是从 shadow 数据中高效识别有用的可观测量,随后采用我们的正则化子空间展开;该展开被设计为即使在使用含噪数据时也具有数值稳定性。我们以解析方式研究了方法内的噪声传播,并对 classical shadows 中因快照数量有限而产生的统计涨落给出了上界。在数值模拟中,我们的方法在许多情况下能够降低能量估计误差,有时降幅超过一个数量级。我们还证明,性能提升对相干误差(不良初始态)和态制备电路中的门噪声均具有鲁棒性。此外,在不使用额外量子资源的情况下,其性能保证至少与直接能量估计一样好,并且在许多情况下更好;因此,该方法是直接从 classical shadow 数据估计基态能量的一种非常自然的替代方案。

英文摘要:

We introduce a post-processing technique for classical shadow measurement data that enhances the precision of ground state estimation through high-dimensional subspace expansion; the dimensionality is only limited by the amount of classical post-processing resources rather than by quantum resources. Crucial steps of our approach are the efficient identification of useful observables from shadow data, followed by our regularised subspace expansion that is designed to be numerically stable even when using noisy data. We analytically investigate noise propagation within our method, and upper bound the statistical fluctuations due to the limited number of snapshots in classical shadows. In numerical simulations, our method can achieve a reduction in the energy estimation errors in many cases, sometimes by more than an order of magnitude. We also demonstrate that our performance improvements are robust against both coherent errors (bad initial state) and gate noise in the state-preparation circuits. Furthermore, performance is guaranteed to be at least as good - and in many cases better - than direct energy estimation without using additional quantum resources and the approach is thus a very natural alternative for estimating ground state energies directly from classical shadow data.

机构、总结、中文摘要均由AI分析而来,可能存在错误,请以论文正文为准。

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