Repairing the linearization radius in shadow estimation

A published lemma that does not close as printed, and the bound that fixes it.

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Background

Shadow tomography asks for the expectation values of m observables on an unknown d-dimensional state to accuracy ε, using as few copies as possible [1]. Classical shadows [2] made it practical, and the conjectured optimum is Θ(log m/ε²) copies with no poly(d) overhead.

Chen, Li and Liu [3] prove this in the high-precision regime. Their argument linearizes around the maximally mixed state, and the linearization is controlled only for ‖EF ≤ (0.01/t)⁴, with the supporting moment lemma in [4]. That fourth power is what confines the result to ε ≤ d⁻¹², and closing the gap down to ε ∼ d⁻¹ was the stated open problem.

The problem

The tail of the linearization error is bounded in [3] by

Σj≥2 2j C(t,j)² (8j)8jE2j ≤ (100t)⁴‖E‖⁴,

valid inside that radius. How large can the radius be made — and is the inequality correct as printed?

The lemma does not close as printed

The j = 2 term alone exceeds the claimed bound by a factor of order 1.8 × 10¹¹, and the excess is independent of ‖E‖ — shrinking the radius does not rescue it. So the replacement below repairs the lemma rather than sharpening it, which matters for anyone citing the step.

The repaired radius

Using the exact identity expressing the operator norm of the t-th Haar moment as a maximum of Schur functions over partitions divided by the dimension of the corresponding irreducible, the per-term constant collapses and the tail resums under

EF ≤ 1/(4et)

in place of (0.01/t)⁴ — fourth power to first, with a better constant besides. Downstream the precision exponent falls from 12 to 5/2 for balanced and structured observables and to 11/2 in general, with copy complexity unchanged at O(log(1/δ)/ε²).

Verification, and an exposition slip

The Murnaghan–Nakayama table was rebuilt from scratch and cross-checked against the power-sum and bialternant formulas; the logical link held on 40k signed traceless spectra; the tail ratio stays below 0.78 uniformly out to t = 5000. Two accounting gaps found adversarially were closed, both exponent-neutral. One is an exposition slip in [3], where a median bound is used as though it were a mean — recoverable from an exact Schur–Weyl second moment, so nothing downstream breaks.

What remains open — and where this now sits

The honest placement matters more than the result. All of this lives inside the linearization framework, and that framework has since been bypassed: Pelecanos, Spilecki and Wright [5] give an exactly unbiased estimator, which has no bias radius to respect, reaches ε ≲ d⁻¹ directly, and disproves the conjectured optimal scaling of [3]. So this entry is of interest for the technique and for the record on the lemma — not for the state of the art.

Genuinely open: matching lower bounds showing [5] optimal across the range, which those authors conjecture but do not prove; and the low-accuracy regime ε ≳ d⁻¹, where the d2/34/3 term dominates and no lower bound is known.

References

  1. S. Aaronson, Shadow tomography of quantum states, arXiv:1711.01053.
  2. H.-Y. Huang, R. Kueng and J. Preskill, Predicting many properties of a quantum system from very few measurements, arXiv:2002.08953.
  3. S. Chen, J. Li and A. Liu, Optimal high-precision shadow estimation, arXiv:2407.13874.
  4. S. Chen, J. Li and A. Liu, An optimal tradeoff between entanglement and copy complexity for state tomography, arXiv:2402.16353.
  5. A. Pelecanos, J. Spilecki and J. Wright, The debiased Keyl’s algorithm: a new unbiased estimator for full state tomography, arXiv:2510.07788.