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arXiv:2602.04952

Instance-optimal high-precision shadow tomography with few-copy measurements: A metrological approach

Senrui Chen, Weiyuan Gong, Sisi Zhou

quant-phcs.ITcs.LGSubmitted Feb 4, 2026• Announced Feb 6, 2026• 0 citations
v1 · Feb 4, 2026v2 · Sep 27, 2026
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Abstract

We study the sample complexity of shadow tomography in the high-precision regime under realistic measurement constraints. Given an unknown $d$-dimensional quantum state $ρ$ and a known set of observables $\{O_i\}_{i=1}^m$, the goal is to estimate expectation values $\{\mathrm{tr}(O_iρ)\}_{i=1}^m$ to accuracy $ε$ in $L_p$-norm, using possibly adaptive measurements that act on $O(\mathrm{polylog}(d))$ number of copies of $ρ$ at a time. We focus on the regime where $ε$ is below an instance-dependent threshold. Our main contribution is an instance-optimal characterization of the sample complexity as $\tildeΘ(Γ_p/ε^2)$, where $Γ_p$ is a function of $\{O_i\}_{i=1}^m$ defined via an optimization formula involving the inverse Fisher information matrix. Previously, tight bounds were known only in special cases, e.g. Pauli shadow tomography with $L_\infty$-norm error. Concretely, we first analyze a simpler oblivious variant where the goal is to estimate an observable of the form $\sum_{i=1}^m α_i O_i$ with $\|α\|_q = 1$ (where $q$ is dual to $p$) revealed after the measurement. For single-copy measurements, we obtain a sample complexity of $Θ(Γ^{\mathrm{ob}}_p/ε^2)$. We then show $\tildeΘ(Γ_p/ε^2)$ is necessary and sufficient for the original problem, with the lower bound applying to unbiased, bounded estimators. Our upper bounds rely on a two-step algorithm combining coarse tomography with local estimation. Notably, $Γ^{\mathrm{ob}}_\infty = Γ_\infty$. In both cases, allowing $c$-copy measurements improves the sample complexity by at most $Ω(1/c)$. Our results establish a quantitative correspondence between quantum learning and metrology, unifying asymptotic metrological limits with finite-sample learning guarantees.

Journal reference
Proceedings of Thirty Ninth Conference on Learning Theory, PMLR 336:1115-1185, 2026
Comments
67 pages

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We study the sample complexity of shadow tomography in the high-precision regime under realistic measurement constraints. Given an unknown ddd-dimensional quantum state ρρρ and a known set of observables {Oi}i=1m\{O_i\}_{i=1}^m{Oi​}i=1m​, the goal is to estimate expectation values {tr(Oiρ)}i=1m\{\mathrm{tr}(O_iρ)\}_{i=1}^m{tr(Oi​ρ)}i=1m​ to accuracy εεε in LpL_pLp​-norm, using possibly adaptive measurements that act on O(polylog(d))O(\mathrm{polylog}(d))O(polylog(d)) number of copies of ρρρ at a time. We focus on the regime where εεε is below an instance-dependent threshold.
Our main contribution is an instance-optimal characterization of the sample complexity as Θ~(Γp/ε2)\tildeΘ(Γ_p/ε^2)Θ~(Γp​/ε2), where ΓpΓ_pΓp​ is a function of {Oi}i=1m\{O_i\}_{i=1}^m{Oi​}i=1m​ defined via an optimization formula involving the inverse Fisher information matrix. Previously, tight bounds were known only in special cases, e.g. Pauli shadow tomography with L∞L_\inftyL∞​-norm error. Concretely, we first analyze a simpler oblivious variant where the goal is to estimate an observable of the form ∑i=1mαiOi\sum_{i=1}^m α_i O_i∑i=1m​αi​Oi​ with ∥α∥q=1\|α\|_q = 1∥α∥q​=1 (where qqq is dual to ppp) revealed after the measurement. For single-copy measurements, we obtain a sample complexity of Θ(Γpob/ε2)Θ(Γ^{\mathrm{ob}}_p/ε^2)Θ(Γpob​/ε2). We then show Θ~(Γp/ε2)\tildeΘ(Γ_p/ε^2)Θ~(Γp​/ε2) is necessary and sufficient for the original problem, with the lower bound applying to unbiased, bounded estimators. Our upper bounds rely on a two-step algorithm combining coarse tomography with local estimation. Notably, Γ∞ob=Γ∞Γ^{\mathrm{ob}}_\infty = Γ_\inftyΓ∞ob​=Γ∞​. In both cases, allowing ccc-copy measurements improves the sample complexity by at most Ω(1/c)Ω(1/c)Ω(1/c).
Our results establish a quantitative correspondence between quantum learning and metrology, unifying asymptotic metrological limits with finite-sample learning guarantees.
Shadow Tomography is a fundamental problem in quantum information theory. Given multiple copies of an unknown ddd-dimensional quantum state ρρρ and a known collection of observables E1,…,EME_1,\ldots,E_ME1​,…,EM​, the goal is to estimate all expectation values {Tr(ρEi)}i=1M\{\text{Tr}(ρE_i)\}_{i=1}^M{Tr(ρEi​)}i=1M​ to additive accuracy ε\varepsilonε with probability at least 1−δ1-δ1−δ. An elusive open question from the seminal shadow tomography work of Aaronson is whether this task admits a dimension-independent sample complexity with only polylogarithmic dependence on MMM, as suggested by the best-known lower bounds. In this work, we propose two different quantum protocols for shadow tomography with the best sample complexity O(log⁡(M)log⁡(M/δ)ε2), O\left( \frac{\log(M)\log(M/δ)}{\varepsilon^2} \right), O(ε2log(M)log(M/δ)​), which is polylogarithmic in the number of observables and independent of the dimension of the unknown state, thereby answering Aaronson's original question while also providing an exponential improvement in the prior best dimension independent sample complexity of shadow tomography from Sinha (STOC 2025) and, more recently, Chen, O'Donnell, Pelecanos, and Wright. Our approach first reduces the general shadow tomography problem to a finite-ensemble estimation problem via a minimax argument. We then develop an observable-independent protocol that repeatedly applies the pretty-good measurement while updating the prior distribution over the finite ensemble according to the measurement outcomes. A tail analysis of the resulting estimation error yields simultaneous accuracy guarantees for all observables and a cubic-logarithmic upper bound. We also introduce a refined recovery-label measurement for the same finite ensemble, which yields the bound in our main theorem.
We study the problems of quantum tomography and shadow tomography using measurements performed on individual, identical copies of an unknown d -dimensional state. We first revisit known lower bounds [ 23 ] on quantum tomography with accuracy ε in trace distance, when the measurement choices are independent of previously observed outcomes, i.e., they are nonadaptive. We give a succinct proof of these results through the χ 2 -divergence between suitable distributions. Unlike prior work, we do not require that the measurements be given by rank-one operators. This leads to stronger lower bounds when the learner uses measurements with a constant number of outcomes (e.g., two-outcome measurements). In particular, this rigorously establishes the optimality of the folklore “Pauli tomography” algorithm in terms of its sample complexity. We also derive novel bounds of Ω(r2d/ϵ2)\Omega (r^2 d/\epsilon ^2)Ω(r2d/ϵ2) and Ω(r2d2/ϵ2)\Omega (r^2 d^2/\epsilon ^2)Ω(r2d2/ϵ2) for learning rank r states using arbitrary and constant-outcome measurements, respectively, in the nonadaptive case. In addition to the sample complexity, a resource of practical significance for learning quantum states is the number of unique measurement settings required (i.e., the number of different measurements used by an algorithm, each possibly with an arbitrary number of outcomes). Motivated by this consideration, we employ concentration of measure of χ 2 -divergence of suitable distributions to extend our lower bounds to the case where the learner performs possibly adaptive measurements from a fixed set of exp⁡(O(d))\exp (O(d))exp(O(d)) possible measurements. This implies in particular that adaptivity does not give us any advantage using single-copy measurements that are efficiently implementable. We also obtain a similar bound in the case where the goal is to predict the expectation values of a given sequence of observables, a task known as shadow tomography. Finally, in the case of adaptive, single-copy measurements implementable with polynomial-size circuits, we prove that a straightforward strategy based on computing sample means of the given observables is optimal.
We study single-copy shadow tomography in the adversarial robust setting, where the goal is to learn the expectation values of MMM observables O1,…,OMO_1, \ldots, O_MO1​,…,OM​ with ε\varepsilonε accuracy, but γγγ-fraction of the outcomes can be arbitrarily corrupted by an adversary. We show that all non-adaptive shadow tomography algorithms must incur an error of ε=Ω~(γmin⁡{M,d})\varepsilon=\tildeΩ(γ\min\{\sqrt{M}, \sqrt{d}\})ε=Ω~(γmin{M​,d​}) for some choice of observables, even with unlimited copies. Unfortunately, the classical shadows algorithm by [HKP20] and naive algorithms that directly measure each observable suffer even more. We design an algorithm that achieves an error of ε=O~(γmax⁡i∈[M]∥Oi∥HS)\varepsilon=\tilde{O}(γ\max_{i\in[M]}\|O_i\|_{HS})ε=O~(γmaxi∈[M]​∥Oi​∥HS​), which nearly matches our worst-case error lower bound for M≥dM\ge dM≥d and guarantees better accuracy when the observables have stronger structure. Remarkably, the algorithm only needs n=1γ2log⁡(M/δ)n=\frac{1}{γ^2}\log(M/δ)n=γ21​log(M/δ) copies to achieve that error with probability at least 1−δ1-δ1−δ, matching the sample complexity of the classical shadows algorithm that achieves the same error without corrupted measurement outcomes. Our algorithm is conceptually simple and easy to implement. Classical simulation for fidelity estimation shows that our algorithm enjoys much stronger robustness than [HKP20] under adversarial noise. Finally, based on a reduction from full-state tomography to shadow tomography, we prove that for rank rrr states, both the near-optimal asymptotic error of ε=O~(γr)\varepsilon=\tilde{O}(γ\sqrt{r})ε=O~(γr​) and copy complexity O~(dr2/ε2)=O~(dr/γ2)\tilde{O}(dr^2/\varepsilon^2)=\tilde{O}(dr/γ^2)O~(dr2/ε2)=O~(dr/γ2) can be achieved for adversarially robust state tomography, closing the large gap in [ABCL25] where optimal error can only be achieved using pseudo-polynomial number of copies in ddd.
Shadow tomography addresses the task of efficiently predicting many expectation values of an unknown quantum state from randomized measurements on comparatively few copies. Existing analyses promise large scaling advantages, but the optimal strategies realizing these guarantees are not always known, and the required measurements are potentially challenging to implement on current hardware. We address this gap for Pauli observables by computing optimal sample-complexity parameters and constructing optimal measurement strategies under realistic resource constraints. We focus on memoryless protocols, where each copy is measured only once, and on measurements with bounded interaction range. Our approach reduces the problem to the analysis of graph parameters of the frustration graph encoding the Pauli anticommutation relations. We provide efficient numerical methods for the general case and analytically prove that Clifford measurements are optimal in many situations. This includes all perfect graphs, all single-qubit, all two-qubit measurement scenarios, and more. Applied to Hamiltonian energy estimation, our framework yields constructive strategies and improved variance bounds for molecular benchmarks.
We give the first tight sample complexity bounds for shadow tomography and classical shadows in the regime where the target error is below some sufficiently small inverse polynomial in the dimension of the Hilbert space. Formally we give a protocol that, given any m∈Nm\in\mathbb{N}m∈N and ε≤O(d−12)ε\le O(d^{-12})ε≤O(d−12), measures O(log⁡(m)/ε2)O(\log(m)/ε^2)O(log(m)/ε2) copies of an unknown mixed state ρ∈Cd×dρ\in\mathbb{C}^{d\times d}ρ∈Cd×d and outputs a classical description of ρρρ which can then be used to estimate any collection of mmm observables to within additive accuracy εεε. Previously, even for the simpler task of shadow tomography -- where the mmm observables are known in advance -- the best known rates either scaled benignly but suboptimally in all of m,d,εm, d, εm,d,ε, or scaled optimally in ε,mε, mε,m but had additional polynomial factors in ddd for general observables. Intriguingly, we also show via dimensionality reduction, that we can rescale εεε and ddd to reduce to the regime where ε≤O(d−1/2)ε\le O(d^{-1/2})ε≤O(d−1/2). Our algorithm draws upon representation-theoretic tools recently developed in the context of full state tomography.
We revisit the problem of Pauli shadow tomography: given copies of an unknown n-qubit quantum stateρ\rhoρ, estimate Tr(Pρ)(P\rho)(Pρ)for some set of Pauli operatorsFFFto within additive errorϵ\epsilonϵ. This has been a popular testbed for exploring the advantage of protocols with quantum memory over those without: with enough memory to measure two copies at a time, one can use Bell sampling to estimate∣Tr(Pρ)\vert \text{Tr}(P\rho)∣Tr(Pρ)for allPPPusingO(n/ϵ4)O(n/\epsilon^{4})O(n/ϵ4)copies, but withk≤nk\leq nk≤nqubits of memory,Ω(2(n−k)/3)\Omega(2^{(n-k)/3})Ω(2(n−k)/3)copies are needed. These results leave open several natural questions. How does this picture change in the physically relevant setting where one only needs to estimate a certain subset of Paulis? What is the optimal dependence onϵ?\epsilon ?ϵ?What is the optimal tradeoff between quantum memory and sample complexity? We answer all of these questions: •For any subsetAAAof Paulis and any family of measurement strategies, we completely characterize the optimal sample complexity, up tolog⁡∣A∣\log\vert A\vertlog∣A∣factors. •We show any protocol that makes poly(n)(n)(n)-copy measure-ments must makeΩ(1/ϵ4)\Omega(1/\epsilon^{4})Ω(1/ϵ4)measurements. •For any protocol that makes poly(n)(n)(n)-copy measurements and only hask<nk < nk<nqubits of memory, we show thatΘ~(min⁡{2n/ϵ2,2n−k/ϵ4})\tilde{\Theta}(\min\{2^{n}/\epsilon^{2},2^{n-k}/\epsilon^{4}\})Θ~(min{2n/ϵ2,2n−k/ϵ4})copies are necessary and sufficient. The protocols we propose can also estimate the actual valuesTr(Pρ)\text{Tr}(P\rho)Tr(Pρ), rather than just their absolute values as in prior work. Additionally, as a byproduct of our techniques, we establish tight bounds for the task of purity testing and show that it exhibits an intriguing phase transition not present in the memory-sample tradeoff for Pauli shadow tomography.