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arXiv:2403.02968 · Quantum

Hamiltonian Property Testing

Andreas Blühm, Matthias C. Caro, Aadil Oufkir

Published Jan 21, 2026• 3 citations
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Abstract

Locality is a fundamental feature of many physical time evolutions. Assumptions on locality and related structural properties also underlie recently proposed procedures for learning an unknown Hamiltonian from access to the induced time evolution. However, no protocols to rigorously test whether an unknown Hamiltonian is local were known. We investigate Hamiltonian locality testing as a property testing problem, where the task is to determine whether an unknown n -qubit Hamiltonian H is k -local or ε -far from all k -local Hamiltonians, given access to the time evolution along H . First, we emphasize the importance of the chosen distance measure: With respect to the operator norm, a worst-case distance measure, incoherent quantum locality testers require Ω ~ ( 2 n ) many time evolution queries and an expected total evolution time of Ω ~ ( 2 n / ε ) , and even coherent testers need Ω ( 2 n / 2 ) many queries and Ω ( 2 n / 2 / ε ) total evolution time. In contrast, when distances are measured according to the normalized Frobenius norm, corresponding to an average-case distance, we give a sample-, time-, and computationally efficient incoherent Hamiltonian locality testing algorithm based on randomized measurements. In fact, our procedure can be used to simultaneously test a wide class of Hamiltonian properties beyond locality. Finally, we prove that learning a general Hamiltonian remains exponentially hard with this average-case distance, thereby establishing an exponential separation between Hamiltonian testing and learning. Our work initiates the study of property testing for quantum Hamiltonians, demonstrating that a broad class of Hamiltonian properties is efficiently testable even with limited quantum capabilities, and positioning Hamiltonian testing as an independent area of research alongside Hamiltonian learning.

DOI
10.22331/q-2026-01-21-1979

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Locality is a fundamental feature of many physical time evolutions. Assumptions on locality and related structural properties also underlie recently proposed procedures for learning an unknown Hamiltonian from access to the induced time evolution. However, no protocols to rigorously test whether an unknown Hamiltonian is local were known. We investigate Hamiltonian locality testing as a property testing problem, where the task is to determine whether an unknown n -qubit Hamiltonian H is k -local or ε -far from all k -local Hamiltonians, given access to the time evolution along H . First, we emphasize the importance of the chosen distance measure: With respect to the operator norm, a worst-case distance measure, incoherent quantum locality testers require Ω ~ ( 2 n ) many time evolution queries and an expected total evolution time of Ω ~ ( 2 n / ε ) , and even coherent testers need Ω ( 2 n / 2 ) many queries and Ω ( 2 n / 2 / ε ) total evolution time. In contrast, when distances are measured according to the normalized Frobenius norm, corresponding to an average-case distance, we give a sample-, time-, and computationally efficient incoherent Hamiltonian locality testing algorithm based on randomized measurements. In fact, our procedure can be used to simultaneously test a wide class of Hamiltonian properties beyond locality. Finally, we prove that learning a general Hamiltonian remains exponentially hard with this average-case distance, thereby establishing an exponential separation between Hamiltonian testing and learning. Our work initiates the study of property testing for quantum Hamiltonians, demonstrating that a broad class of Hamiltonian properties is efficiently testable even with limited quantum capabilities, and positioning Hamiltonian testing as an independent area of research alongside Hamiltonian learning.
We establish lower bounds for Hamiltonian property testing with access to the time-evolution operator but not its inverse. Each experiment may query the time-evolution operator multiple times, and distances between Hamiltonians are measured in the normalized Frobenius norm. In this model, we show that testing whether a Hamiltonian is kkk-local or ε\varepsilonε-far from every kkk-local Hamiltonian requires Ω(1/ε2)Ω(1/\varepsilon^2)Ω(1/ε2) total evolution time, matching the upper bound of Kallaugher and Liang (TQC'25). We also prove that testing whether an unknown Hamiltonian equals a target Hamiltonian or is ε\varepsilonε-far from it requires Ω(1/ε2)Ω(1/\varepsilon^2)Ω(1/ε2) total evolution time, matching the upper bound of Sinha and Tong (2025). These are the first lower bounds for natural problems in Hamiltonian learning and testing that rule out Heisenberg-limited scaling of 1/ε1/\varepsilon1/ε. As a third result, we show that amplitude estimation to precision ε\varepsilonε requires Ω(1/ε2)Ω(1/\varepsilon^2)Ω(1/ε2) total time evolution, recovering the result of Tang and Wright (QIP'26) in the continuous-time query model. All three results follow from the hardness of distinguishing the zero Hamiltonian from a suitably chosen ensemble of random Hamiltonians. We establish this hardness by adapting the continuous-time adversary method to forward Hamiltonian evolution.
We consider the problems of testing and learning an unknown n -qubit quantum Hamiltonian H =∑ x λ x σ x expressed in its Pauli basis, from queries to its evolution operator e − iHt under the normalized Frobenius norm. To this end, we prove the following results (with and without quantum memory) for Hamiltonians whose Pauli spectrum involves only k -local terms or has sparsity at most s : (1) Local Hamiltonians : We give a tolerant testing protocol to decide if a Hamiltonian is ε 1 -close to k -local or ε 2 -far from k -local, with O (1/(ε 2 −ε 1 ) 4 ) queries, thereby solving two open questions posed in a recent work by Bluhm, Caro and Oufkir [BCO’24]. For learning a k -local Hamiltonian up to error ε, we give a protocol with query complexity and total time evolution exp( O ( k 2 + k log(1/ε))). Our algorithm leverages the non-commutative Bohnenblust-Hille inequality in order to get a complexity independent of n . (2) Sparse Hamiltonians : We give a protocol for testing whether a Hamiltonian is ε 1 -close to being s -sparse or ε 2 -far from being s -sparse, with O ( s 6 /(ε 2 2 −ε 1 2 ) 6 ) queries. For learning up to error ε, we show that O ( s 4 /ε 8 ) queries suffices. (3) Learning without quantum memory : The learning results stated above have no dependence on the system size n , but require n -qubit quantum memory. We give subroutines that allow us to reproduce all the above learning results without quantum memory; increasing the query complexity by a (log n )-factor in the local case and an n -factor in the sparse case. (4) Testing without quantum memory : We give a new subroutine called Pauli hashing , which allows one to tolerantly test s -sparse Hamiltonians using Õ( s 14 /(ε 2 2 −ε 1 2 ) 18 ) query complexity. A key ingredient is showing that s -sparse Pauli channels can be tested in a tolerant fashion as being ε 1 -close to being s -sparse or ε 2 -far under the diamond norm, using Õ( s 2 /(ε 2 −ε 1 ) 6 ) queries via Pauli hashing. In order to prove these results, we prove new structural theorems for local Hamiltonians, sparse Pauli channels and sparse Hamiltonians. We complement our learning algorithms with lower bounds that are polynomially weaker. Furthermore, our algorithms use short time evolutions and do not assume prior knowledge of the terms on which the Pauli spectrum is supported on, i.e., we do not require prior knowledge about the support of the Hamiltonian terms.
Quantum algorithms enable Heisenberg-limited scaling across many tasks in sensing and learning, achieving precision ε\varepsilonε using O(1/ε)O(1/\varepsilon)O(1/ε) total evolution time. However, in Hamiltonian property testing, the best known algorithms have O(1/ε2)O(1/\varepsilon^2)O(1/ε2) total evolution time, unless it is possible to reverse\textit{reverse}reverse the flow of time under the Hamiltonian. In this work, we prove that time reversal is necessary to close this gap. We establish evolution time lower bounds for Hamiltonian certification and locality testing, for a continuous family of error metrics ranging from average- to worst-case. We also prove matching upper bounds for Hamiltonian certification in all cases, both with and without time reversal, showing that the advantage from time reversal persists. Our results follow from a new Fourier-analytic approach to quantum lower bounds in continuous time, which is sensitive to time reversal and applicable beyond Hamiltonian property testing. This gives an alternative proof that inverses are required for amplitude amplification and estimation, improving the lower bounds of Tang and Wright and extending to fractional queries. We also show that, for unstructured search, uncertainty in the phase of the oracle destroys the quantum speedup without inverse queries, even when the oracle is fixed and coherent. Our work rigorously establishes time reversal as a resource governing both the precision of quantum measurement and the robustness of quantum algorithms.
We study the problem of certifying local Hamiltonians from real-time access to their dynamics. Given oracle access to e−itHe^{-itH}e−itH for an unknown kkk-local Hamiltonian HHH and a fully specified target Hamiltonian H0H_0H0​, the goal is to decide whether HHH is exactly equal to H0H_0H0​ or differs from H0H_0H0​ by at least ε\varepsilonε in normalized Frobenius norm, while minimizing the total evolution time. We introduce the first intolerant Hamiltonian certification protocol that achieves optimal performance for all constant-locality Hamiltonians. For general nnn-qubit, kkk-local, traceless Hamiltonians, our procedure uses O(ck/ε)O(c^k/\varepsilon)O(ck/ε) total evolution time for a universal constant ccc, and succeeds with high probability. In particular, for O(1)O(1)O(1)-local Hamiltonians, the total evolution time becomes Θ(1/ε)Θ(1/\varepsilon)Θ(1/ε), matching the known Ω(1/ε)Ω(1/\varepsilon)Ω(1/ε) lower bounds and achieving the gold-standard Heisenberg-limit scaling. Prior certification methods either relied on implementing inverse evolution of HHH, required controlled access to e−itHe^{-itH}e−itH, or achieved near-optimal guarantees only in restricted settings such as the Ising case (k=2k=2k=2). In contrast, our algorithm requires neither inverse evolution nor controlled operations: it uses only forward real-time dynamics and achieves optimal intolerant certification for all constant-locality Hamiltonians.
We consider the problems of testing and learning an unknown nnn-qubit Hamiltonian HHH from queries to its evolution operator e−iHte^{-iHt}e−iHt under the normalized Frobenius norm. We prove: 1. Local Hamiltonians: We give a tolerant testing protocol to decide if HHH is ε1ε_1ε1​-close to kkk-local or ε2ε_2ε2​-far from kkk-local, with O(1/(ε2−ε1)4)O(1/(ε_2-ε_1)^{4})O(1/(ε2​−ε1​)4) queries, solving open questions posed in a recent work by Bluhm et al. For learning a kkk-local HHH up to error εεε, we give a protocol with query complexity exp⁡(O(k2+klog⁡(1/ε)))\exp(O(k^2+k\log(1/ε)))exp(O(k2+klog(1/ε))) independent of nnn, by leveraging the non-commutative Bohnenblust-Hille inequality. 2. Sparse Hamiltonians: We give a protocol to test if HHH is ε1ε_1ε1​-close to being sss-sparse (in the Pauli basis) or ε2ε_2ε2​-far from being sss-sparse, with O(s6/(ε22−ε12)6)O(s^{6}/(ε_2^2-ε_1^2)^{6})O(s6/(ε22​−ε12​)6) queries. For learning up to error εεε, we show that O(s4/ε8)O(s^{4}/ε^{8})O(s4/ε8) queries suffice. 3. Learning without memory: The learning results stated above have no dependence on nnn, but require nnn-qubit quantum memory. We give subroutines that allow us to learn without memory; increasing the query complexity by a (log⁡n)(\log n)(logn)-factor in the local case and an nnn-factor in the sparse case. 4. Testing without memory: We give a new subroutine called Pauli hashing, which allows one to tolerantly test sss-sparse Hamiltonians with O(s14/(ε22−ε12)18)O(s^{14}/(ε_2^2-ε_1^2)^{18})O(s14/(ε22​−ε12​)18) queries. A key ingredient is showing that sss-sparse Pauli channels can be tolerantly tested under the diamond norm with O(s2/(ε2−ε1)6)O(s^2/(ε_2-ε_1)^6)O(s2/(ε2​−ε1​)6) queries. Along the way, we prove new structural theorems for local and sparse Hamiltonians. We complement our learning results with polynomially weaker lower bounds. Furthermore, our algorithms use short time evolutions and do not assume prior knowledge of the terms in the support of the Pauli spectrum.
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