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On the Classical Shadow Nonparametric Bootstrap

Eric Ghysels, Jack Morgan

TL;DR

The paper addresses the limitations of Gaussian-based error characterizations for classical shadow estimators by applying nonparametric bootstrap to the shadow data, treating the shadow samples as a dataset and generating bootstrap replicates $T_N^{*,b}$. This approach reveals non-Gaussian, heavy-tailed tail behavior in general observables and shows that standard MoM error bounds are not tight, highlighting the value of bootstrap-based uncertainty quantification. By introducing tail risk measures such as Value-at-Risk and Expected Shortfall for quantum circuit predictions, the work demonstrates meaningful tail-risk differences compared to Gaussian approximations, underscoring the need for tail-focused analysis. The findings broaden the applicability of classical shadows, enabling risk-aware assessments for a range of tasks including entropies, correlators, and error mitigation, and pave the way for more robust, tail-conscious quantum state property estimation.

Abstract

Classical shadows are an efficient method for constructing an approximate classical description of a quantum state using very few measurements. In the paper we propose to enhance classical shadow methods using bootstrap resampling methods. We apply nonparametric bootstrapping to assess the variability and accuracy of estimators by repeatedly sampling with replacement from the observed data, i.e. in our case the classical shadow measurements. We show that the bootstrap distributions are very different from the Gaussian approximations. Likewise, the theoretical error bounds are not tight compared to the bootstrap percentiles. Finally, we suggest using resampling tools to make risk assessments.

On the Classical Shadow Nonparametric Bootstrap

TL;DR

The paper addresses the limitations of Gaussian-based error characterizations for classical shadow estimators by applying nonparametric bootstrap to the shadow data, treating the shadow samples as a dataset and generating bootstrap replicates . This approach reveals non-Gaussian, heavy-tailed tail behavior in general observables and shows that standard MoM error bounds are not tight, highlighting the value of bootstrap-based uncertainty quantification. By introducing tail risk measures such as Value-at-Risk and Expected Shortfall for quantum circuit predictions, the work demonstrates meaningful tail-risk differences compared to Gaussian approximations, underscoring the need for tail-focused analysis. The findings broaden the applicability of classical shadows, enabling risk-aware assessments for a range of tasks including entropies, correlators, and error mitigation, and pave the way for more robust, tail-conscious quantum state property estimation.

Abstract

Classical shadows are an efficient method for constructing an approximate classical description of a quantum state using very few measurements. In the paper we propose to enhance classical shadow methods using bootstrap resampling methods. We apply nonparametric bootstrapping to assess the variability and accuracy of estimators by repeatedly sampling with replacement from the observed data, i.e. in our case the classical shadow measurements. We show that the bootstrap distributions are very different from the Gaussian approximations. Likewise, the theoretical error bounds are not tight compared to the bootstrap percentiles. Finally, we suggest using resampling tools to make risk assessments.

Paper Structure

This paper contains 6 sections, 13 equations, 4 figures, 1 table.

Figures (4)

  • Figure 1: Gaussian distribution of median-of-mean estimator with $K$ = 10 for $N$ = 1000, for an observable $o_1$ of a 10-qubit circuit involving rotations detailed in the next section, using the estimator defined in equation (\ref{['eq:MoM']}) and its variance appearing in (\ref{['eq:S9']}).
  • Figure 2: Quantum circuit used to generate classical shadow observables. We use 10 qubit (only 4 displayed) circuit for classical shadows to estimate a set $O$ of 27 observables.
  • Figure 3: The three densities are: (a) the Gaussian appearing in Figure \ref{['fig:Gaussian']} representing the asymptotic representation, (b) the histogram of the $B$ = 1000 expectation value bootstrap estimates for the median-of-means, and (c) a Kernel density estimate (KDE) smoothed version of the histogram.
  • Figure 4: Theoretical error bound implied by equation and bootstrap distributions with $B$ = 1000 with $N$ appearing on the x-axis.