Random quantum circuits transform local noise into global white noise
Alexander M. Dalzell, Nicholas Hunter-Jones, Fernando G. S. L. Brandão
TL;DR
This work analyzes noisy random quantum circuits in the low-fidelity regime and proves that local unital noise is rapidly scrambled, effectively becoming white noise. It shows the noisy output distribution p_noisy is well approximated by a white-noise mixture p_wn = F p_ideal + (1−F) p_unif with F ≈ exp(−2sε), and provides an explicit bound on the average total-variation distance to p_wn that scales as O(Fε√s) under conditions s ≥ Ω(n log n) and ε^{-1} ≥ Ω(n). The study also proves exponential convergence of p_noisy to the uniform distribution for incoherent noise, and derives a quantitative bound on how close p_noisy is to p_wn (via δ and F) when the noise is incoherent; the latter supports the use of linear cross-entropy benchmarking and has implications for the hardness of sampling from noisy outputs. The methodology maps second-moment quantities to stochastic processes, enabling rigorous analysis of error scrambling, and numerical results for complete-graph architectures with parameters akin to recent experiments suggest a practical regime where the white-noise approximation is meaningful. Overall, the results provide a robust theoretical footing for salvaging signals from noisy random quantum circuits and for understanding the noise resilience of near-term quantum computational tasks.
Abstract
We study the distribution over measurement outcomes of noisy random quantum circuits in the low-fidelity regime. We show that, for local noise that is sufficiently weak and unital, correlations (measured by the linear cross-entropy benchmark) between the output distribution $p_{\text{noisy}}$ of a generic noisy circuit instance and the output distribution $p_{\text{ideal}}$ of the corresponding noiseless instance shrink exponentially with the expected number of gate-level errors, as $F=\text{exp}(-2sε\pm O(sε^2))$, where $ε$ is the probability of error per circuit location and $s$ is the number of two-qubit gates. Furthermore, if the noise is incoherent, the output distribution approaches the uniform distribution $p_{\text{unif}}$ at precisely the same rate and can be approximated as $p_{\text{noisy}} \approx Fp_{\text{ideal}} + (1-F)p_{\text{unif}}$, that is, local errors are scrambled by the random quantum circuit and contribute only white noise (uniform output). Importantly, we upper bound the total variation error (averaged over random circuit instance) in this approximation as $O(Fε\sqrt{s})$, so the "white-noise approximation" is meaningful when $ε\sqrt{s} \ll 1$, a quadratically weaker condition than the $εs\ll 1$ requirement to maintain high fidelity. The bound applies when the circuit size satisfies $s \geq Ω(n\log(n))$ and the inverse error rate satisfies $ε^{-1} \geq \tildeΩ(n)$. The white-noise approximation is useful for salvaging the signal from a noisy quantum computation; it was an underlying assumption in complexity-theoretic arguments that low-fidelity random quantum circuits cannot be efficiently sampled classically. Our method is based on a map from second-moment quantities in random quantum circuits to expectation values of certain stochastic processes for which we compute upper and lower bounds.
