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Krylov Shadow Tomography for QFI Estimation

Updated 5 July 2026
  • KST is a hybrid framework that combines Krylov subspace methods with shadow tomography to efficiently estimate the quantum Fisher information.
  • It constructs a strict hierarchy of non-polynomial lower bounds that converge exponentially fast to the exact QFI, outperforming traditional polynomial approximations.
  • KST leverages classical shadows from local randomized measurements, making QFI estimation experimentally feasible for large or low-rank quantum systems.

Searching arXiv for papers on Krylov shadow tomography and QFI estimation. Krylov shadow tomography (KST) is a hybrid framework for estimating the quantum Fisher information (QFI) of an unknown quantum state by combining the Krylov subspace method with shadow tomography. It was introduced as a way to make QFI estimation experimentally feasible for large quantum systems, where direct evaluation is difficult because the QFI depends on the density operator in a highly nonlinear manner (Zhang et al., 3 Mar 2025). Subsequent work established that KST yields a strict hierarchy of non-polynomial lower bounds on the QFI, that these bounds converge exponentially fast with Krylov order, that they are tighter than state-of-the-art polynomial lower bounds at comparable resource level, and that for certain low-rank states the hierarchy terminates at the exact QFI already at low order (Wang et al., 19 Feb 2026).

1. QFI estimation problem and the motivation for KST

For a quantum state ρ=kpkkk\rho=\sum_k p_k |k\rangle\langle k| and Hermitian generator HH, the QFI is given by

FQ=2pk+pl>0(pkpl)2pk+plkHl2.F_Q = 2\sum_{p_k+p_l>0}\frac{(p_k-p_l)^2}{p_k+p_l}\, |\langle k|H|l\rangle|^2.

This quantity is central in quantum metrology because it determines the ultimate precision limit in parameter estimation, and it is also used in entanglement detection and related tasks (Zhang et al., 3 Mar 2025). The difficulty is that FQF_Q is highly nonlinear in ρ\rho, so it is not directly accessible through the low-order polynomial observables naturally handled by modern randomized-measurement methods.

Earlier work therefore concentrated on experimentally accessible lower bounds on the QFI, including Legendre-transform bounds, sub-QFI bounds, and Taylor-series-based bounds (Wang et al., 19 Feb 2026). These polynomial lower bounds are measurable, but they exhibit an unavoidable systematic gap: no polynomial lower bound can coincide with the QFI for all states (Wang et al., 19 Feb 2026). Previous asymptotic polynomial hierarchies can approach FQF_Q, but only at high order, with rapidly increasing measurement and postprocessing cost (Zhang et al., 3 Mar 2025).

KST addresses this limitation by replacing the polynomial-approximation viewpoint with a hierarchy of non-polynomial Krylov bounds. This shifts the task from approximating the QFI by polynomial surrogates to approximating an operator associated with the QFI inside a structured Krylov subspace. A plausible implication is that the central advantage of KST is not merely tighter lower bounds, but a qualitatively different approximation principle.

2. Operator-theoretic construction

The mathematical setup begins with the weighted inner product

X,Yρ=tr ⁣[ρ(XY+YX)/2],\langle X,Y\rangle_\rho = \operatorname{tr}\!\left[\rho(XY+YX)/2\right],

and the associated norm Xρ=X,Xρ\|X\|_\rho=\sqrt{\langle X,X\rangle_\rho}. The relevant superoperator is the symmetrization map

Rρ(X)=12(ρX+Xρ).\mathcal{R}_\rho(X)=\frac{1}{2}(\rho X+X\rho).

In the eigenbasis of ρ\rho, this acts as

HH0

with inverse on the relevant operator subspace

HH1

Defining

HH2

one obtains the compact representation

HH3

(Zhang et al., 3 Mar 2025).

KST then constructs the nested Krylov subspaces

HH4

Within each HH5, one chooses the best approximation HH6 to HH7 in the HH8-weighted norm, and defines the corresponding Krylov bound

HH9

Equivalently,

FQ=2pk+pl>0(pkpl)2pk+plkHl2.F_Q = 2\sum_{p_k+p_l>0}\frac{(p_k-p_l)^2}{p_k+p_l}\, |\langle k|H|l\rangle|^2.0

Because FQ=2pk+pl>0(pkpl)2pk+plkHl2.F_Q = 2\sum_{p_k+p_l>0}\frac{(p_k-p_l)^2}{p_k+p_l}\, |\langle k|H|l\rangle|^2.1 is the orthogonal projection of FQ=2pk+pl>0(pkpl)2pk+plkHl2.F_Q = 2\sum_{p_k+p_l>0}\frac{(p_k-p_l)^2}{p_k+p_l}\, |\langle k|H|l\rangle|^2.2 onto FQ=2pk+pl>0(pkpl)2pk+plkHl2.F_Q = 2\sum_{p_k+p_l>0}\frac{(p_k-p_l)^2}{p_k+p_l}\, |\langle k|H|l\rangle|^2.3, the exact decomposition

FQ=2pk+pl>0(pkpl)2pk+plkHl2.F_Q = 2\sum_{p_k+p_l>0}\frac{(p_k-p_l)^2}{p_k+p_l}\, |\langle k|H|l\rangle|^2.4

holds, and therefore

FQ=2pk+pl>0(pkpl)2pk+plkHl2.F_Q = 2\sum_{p_k+p_l>0}\frac{(p_k-p_l)^2}{p_k+p_l}\, |\langle k|H|l\rangle|^2.5

(Zhang et al., 3 Mar 2025).

The operator space is restricted to

FQ=2pk+pl>0(pkpl)2pk+plkHl2.F_Q = 2\sum_{p_k+p_l>0}\frac{(p_k-p_l)^2}{p_k+p_l}\, |\langle k|H|l\rangle|^2.6

so that the weighted inner product is positive definite even when FQ=2pk+pl>0(pkpl)2pk+plkHl2.F_Q = 2\sum_{p_k+p_l>0}\frac{(p_k-p_l)^2}{p_k+p_l}\, |\langle k|H|l\rangle|^2.7 is singular. The nontrivial case assumes FQ=2pk+pl>0(pkpl)2pk+plkHl2.F_Q = 2\sum_{p_k+p_l>0}\frac{(p_k-p_l)^2}{p_k+p_l}\, |\langle k|H|l\rangle|^2.8; otherwise FQ=2pk+pl>0(pkpl)2pk+plkHl2.F_Q = 2\sum_{p_k+p_l>0}\frac{(p_k-p_l)^2}{p_k+p_l}\, |\langle k|H|l\rangle|^2.9 (Zhang et al., 3 Mar 2025).

3. Hierarchy, strict improvement, and finite termination

A defining feature of KST is that it yields not a single bound but a strict hierarchy of increasingly tight lower bounds. The Krylov subspaces satisfy

FQF_Q0

for some finite stopping index FQF_Q1, and the exact operator FQF_Q2 belongs to FQF_Q3 but not to any smaller FQF_Q4 with FQF_Q5 (Zhang et al., 3 Mar 2025). Consequently,

FQF_Q6

This strict hierarchy is one of the principal structural results of the framework (Wang et al., 19 Feb 2026).

The highest Krylov bound is exact because once the Krylov subspace contains FQF_Q7, the projection error vanishes. In this sense, KST is not limited to asymptotic approximation: at finite Krylov dimension it can reproduce the exact QFI (Zhang et al., 3 Mar 2025). This directly differentiates it from previously studied polynomial lower-bound schemes, which cannot coincide with the QFI for all states (Wang et al., 19 Feb 2026).

A common misconception is to regard KST as simply another polynomial lower-bound construction. That characterization is inaccurate. The bound FQF_Q8 is non-polynomial in FQF_Q9, even though it is assembled from polynomial moments. The distinction is essential because the exactness and finite termination properties of KST lie beyond the reach of polynomial lower bounds in general (Zhang et al., 3 Mar 2025).

4. Convergence properties and comparison with polynomial bounds

The 2026 analysis established that low-order Krylov bounds are already practically effective. Its central quantitative result is an exponential convergence theorem for the relative error

ρ\rho0

namely

ρ\rho1

Here ρ\rho2 is a condition-number-like quantity determined by the spectrum of ρ\rho3; for full rank it is essentially the ratio of largest to smallest eigenvalue, with an appropriate modification for non-full-rank states (Wang et al., 19 Feb 2026). The theorem implies exponential convergence of the Krylov hierarchy to the exact QFI as the Krylov order increases, with faster convergence for more mixed states.

The same work proved a direct superiority statement against the Taylor hierarchy ρ\rho4:

ρ\rho5

This comparison is described as resource-fair because ρ\rho6 and ρ\rho7 require estimating polynomial functions of ρ\rho8 of comparable degree (Wang et al., 19 Feb 2026). The result shows that, at essentially the same estimation cost, the Krylov bound is generally tighter than the corresponding Taylor bound.

The significance of this comparison is methodological as well as numerical. Polynomial lower bounds approximate the nonlinear QFI through polynomial surrogates and therefore retain a systematic bias. KST instead constructs a hierarchy of non-polynomial approximants through projection in Krylov space. This suggests that the observed superiority is structurally rooted in the approximation scheme rather than in a favorable choice of constants.

5. Exactness for low-rank states

KST has a particularly sharp exactness theory for low-rank states. Let

ρ\rho9

be the set of sums of distinct eigenvalue pairs. The stopping order satisfies

FQF_Q0

where FQF_Q1 denotes the number of distinct values in FQF_Q2 (Wang et al., 19 Feb 2026). Since FQF_Q3 for a rank-FQF_Q4 state,

FQF_Q5

Thus low-rank structure can force exact recovery of the QFI at very small Krylov order.

The Methods section further refines this by giving the exact formula

FQF_Q6

where FQF_Q7 consists of those eigenvalue sums FQF_Q8 for which all relevant matrix elements of FQF_Q9 vanish between the corresponding eigenspaces (Wang et al., 19 Feb 2026). This characterizes when the Krylov sequence terminates earlier than the generic rank-based upper bound would suggest.

The original KST paper presented explicit examples with X,Yρ=tr ⁣[ρ(XY+YX)/2],\langle X,Y\rangle_\rho = \operatorname{tr}\!\left[\rho(XY+YX)/2\right],0. For the pseudo-pure state

X,Yρ=tr ⁣[ρ(XY+YX)/2],\langle X,Y\rangle_\rho = \operatorname{tr}\!\left[\rho(XY+YX)/2\right],1

it showed that X,Yρ=tr ⁣[ρ(XY+YX)/2],\langle X,Y\rangle_\rho = \operatorname{tr}\!\left[\rho(XY+YX)/2\right],2 for any X,Yρ=tr ⁣[ρ(XY+YX)/2],\langle X,Y\rangle_\rho = \operatorname{tr}\!\left[\rho(XY+YX)/2\right],3, any pure state X,Yρ=tr ⁣[ρ(XY+YX)/2],\langle X,Y\rangle_\rho = \operatorname{tr}\!\left[\rho(XY+YX)/2\right],4, and any X,Yρ=tr ⁣[ρ(XY+YX)/2],\langle X,Y\rangle_\rho = \operatorname{tr}\!\left[\rho(XY+YX)/2\right],5, so that

X,Yρ=tr ⁣[ρ(XY+YX)/2],\langle X,Y\rangle_\rho = \operatorname{tr}\!\left[\rho(XY+YX)/2\right],6

For the bound entangled state

X,Yρ=tr ⁣[ρ(XY+YX)/2],\langle X,Y\rangle_\rho = \operatorname{tr}\!\left[\rho(XY+YX)/2\right],7

with X,Yρ=tr ⁣[ρ(XY+YX)/2],\langle X,Y\rangle_\rho = \operatorname{tr}\!\left[\rho(XY+YX)/2\right],8, it likewise proved X,Yρ=tr ⁣[ρ(XY+YX)/2],\langle X,Y\rangle_\rho = \operatorname{tr}\!\left[\rho(XY+YX)/2\right],9, hence again Xρ=X,Xρ\|X\|_\rho=\sqrt{\langle X,X\rangle_\rho}0 (Zhang et al., 3 Mar 2025).

The broader relevance of these results follows from the observation that low-rank and nearly low-rank states are common in quantum information processing, for example when ideal pure states are weakly corrupted by noise (Wang et al., 19 Feb 2026). In such settings, low-order Krylov bounds can eliminate the systematic error that affects polynomial approximations.

6. Estimation by classical shadows, practical behavior, and limitations

KST becomes experimentally accessible because each bound can be expressed through quantities

Xρ=X,Xρ\|X\|_\rho=\sqrt{\langle X,X\rangle_\rho}1

which are polynomial functionals of Xρ=X,Xρ\|X\|_\rho=\sqrt{\langle X,X\rangle_\rho}2 (Wang et al., 19 Feb 2026). Writing

Xρ=X,Xρ\|X\|_\rho=\sqrt{\langle X,X\rangle_\rho}3

the bound is computed as

Xρ=X,Xρ\|X\|_\rho=\sqrt{\langle X,X\rangle_\rho}4

Equivalently, the original derivation formulates Xρ=X,Xρ\|X\|_\rho=\sqrt{\langle X,X\rangle_\rho}5 as a positive-definite Hankel matrix for Xρ=X,Xρ\|X\|_\rho=\sqrt{\langle X,X\rangle_\rho}6, so the matrix inverse is well defined (Zhang et al., 3 Mar 2025). The non-polynomial character of Xρ=X,Xρ\|X\|_\rho=\sqrt{\langle X,X\rangle_\rho}7 thus enters through the inverse of a moment matrix built from polynomial data.

The measurement protocol is local. One samples

Xρ=X,Xρ\|X\|_\rho=\sqrt{\langle X,X\rangle_\rho}8

where each Xρ=X,Xρ\|X\|_\rho=\sqrt{\langle X,X\rangle_\rho}9 is drawn independently from a suitable single-qubit ensemble such as the single-qubit Clifford group or Rρ(X)=12(ρX+Xρ).\mathcal{R}_\rho(X)=\frac{1}{2}(\rho X+X\rho).0, applies Rρ(X)=12(ρX+Xρ).\mathcal{R}_\rho(X)=\frac{1}{2}(\rho X+X\rho).1 to Rρ(X)=12(ρX+Xρ).\mathcal{R}_\rho(X)=\frac{1}{2}(\rho X+X\rho).2, measures in the computational basis, and records a bitstring Rρ(X)=12(ρX+Xρ).\mathcal{R}_\rho(X)=\frac{1}{2}(\rho X+X\rho).3 (Zhang et al., 3 Mar 2025). Repeating this procedure yields classical shadows

Rρ(X)=12(ρX+Xρ).\mathcal{R}_\rho(X)=\frac{1}{2}(\rho X+X\rho).4

with Rρ(X)=12(ρX+Xρ).\mathcal{R}_\rho(X)=\frac{1}{2}(\rho X+X\rho).5. The moments Rρ(X)=12(ρX+Xρ).\mathcal{R}_\rho(X)=\frac{1}{2}(\rho X+X\rho).6 can be estimated simultaneously from the same shadow data using Rρ(X)=12(ρX+Xρ).\mathcal{R}_\rho(X)=\frac{1}{2}(\rho X+X\rho).7-statistics, and the batch-shadow method can accelerate post-processing (Wang et al., 19 Feb 2026). The estimator in the original proposal uses a median-of-means construction and finally computes

Rρ(X)=12(ρX+Xρ).\mathcal{R}_\rho(X)=\frac{1}{2}(\rho X+X\rho).8

(Zhang et al., 3 Mar 2025).

The formal guarantee states that for

Rρ(X)=12(ρX+Xρ).\mathcal{R}_\rho(X)=\frac{1}{2}(\rho X+X\rho).9

and ρ\rho0 chosen according to an explicit bound depending on the operator norms or variances of the relevant ρ\rho1, the final estimate satisfies

ρ\rho2

with probability at least ρ\rho3 (Zhang et al., 3 Mar 2025). The papers emphasize that the protocol uses only single-qubit gates and local measurements, and that its measurement cost is comparable to the best existing randomized-measurement approaches for QFI lower bounds (Zhang et al., 3 Mar 2025).

At the same time, the resource cost grows exponentially with Krylov order, which is why the practical emphasis falls on low-order bounds (Wang et al., 19 Feb 2026). This is the main limitation of current KST implementations. The method is therefore most attractive precisely in the regimes highlighted by the theory: moderate Krylov order, rapid convergence, or low-rank structure yielding early exactness. Numerical simulations support this picture: low-order Krylov bounds are close to ρ\rho4 already for moderate mixed states, outperform Taylor bounds in direct comparisons, and for rank-2 examples the highest relevant Krylov bound matches the QFI exactly (Wang et al., 19 Feb 2026). The original benchmarks further reported that ρ\rho5 for pseudo-pure states obtained from ρ\rho6 classical shadows tracks ρ\rho7 well, with sample complexity for relative error ρ\rho8 scaling like ρ\rho9, while for the bound entangled example numerical results using HH00 classical shadows showed sample cost scaling like HH01 (Zhang et al., 3 Mar 2025).

KST is therefore best understood as a framework for QFI estimation that combines three features: a Krylov-subspace approximation to the SLD-related operator HH02, a strict hierarchy of non-polynomial lower bounds HH03, and shadow-based estimation of the polynomial moments required to evaluate those bounds (Zhang et al., 3 Mar 2025). In quantum metrology, entanglement detection, sensing, variational algorithms, and resource quantification, its importance lies in reducing or removing the systematic error inherent to polynomial lower-bound methods while preserving experimental accessibility (Wang et al., 19 Feb 2026).

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