Energy-selective quantum search with Ising Hamiltonian phase oracles

A. S. Plyashechnik, A. A. Zhukov, A. V. Lebedev, W. V. Pogosov · arXiv:2606.03380 · new submission, announced 2026-06-03 · score 9/10 (HIGH)

Abstract

Ising Hamiltonians are basic models of disordered magnets and a standard language for quantum and classical optimization. We study an energy-selective quantum search primitive in which the physical evolution exp(-iTH) is used directly as a Hamiltonian phase oracle. Unlike a Boolean oracle, this oracle marks configurations continuously by their phases and selects a finite resonance band rather than a preassigned marked set. We show that alternating it with the Grover diffusion operator nevertheless produces a Grover-type amplification peak. An exact spectral recurrence and a generating-function representation determine the peak position, width, and height. For an annealed Gaussian density of states, target energies in a high-density tail require Θ(√(2n/M)) oracle calls when the resonance contains M configurations. For random Ising spectra, overlap-induced correlations shift and distort the peak; spectral symmetrization and iterative calibration remove this detuning for prescribed-energy targeting.

Executive summary

The authors replace Grover's Boolean phase oracle with the continuous-phase operator U_T = exp(-iTH) of an Ising Hamiltonian itself, then prove that alternating U_T with the standard Grover diffuser still yields a quadratic-speedup amplification peak — at a target energy E* = π/T selected by the operator's free parameter T. The selected subspace is generated self-consistently by the local spectral density (not specified externally as in Boolean Grover), and reaches it in Θ(√(2n/M)) oracle calls, with each call costing only the O(n²) commuting ZZ rotations needed to Trotter-implement exp(-iTH) exactly. For Yuan this is directly load-bearing: it is the closest possible methodological neighbour to Y4 (Grover × cardinality-structured search), and the √(2n/M) scaling matches Y4's √(C(n,k)/M) when the energy resonance band plays the role of the cardinality-feasible subspace.

Main contribution

The paper develops a complete spectral theory of an "Ising Grover" iterate W_T = D_ξ U_T with D_ξ = 2|ξ⟩⟨ξ| - I the diffuser about the uniform state. The amplitudes a_K(E) satisfy an exact one-dimensional recurrence (Eq. 11) in energy, whose generating-function solution (Eq. 19) factorises into a resonance kernel and a spectral susceptibility C_r(φ) = 2G(-re^{iφ}) - 1, where G is the generating function of the characteristic-function samples g_m = 2-n Tr exp(-imTH) — the partition function at imaginary inverse temperature β = imT. The local zero of Im C_r determines the resonance position; its slope and real part determine width and saturation height. For the annealed Gaussian density of states this gives K_peak ~ nμ-3/2 2n/2 and resonance cardinality M_peak ~ n3-2μ, recovering Grover scaling. For correlated random-Ising spectra (overlap-correlated levels rather than independent random energies), spin-glass correlations shift the resonance by φ_0 = O(n-3) rms and can also depress the peak height — both effects are fixed analytically and corrected via either (i) ancilla-based spectral symmetrization or (ii) an iteratively self-calibrating evolution time.

Key theorems / lemmas / algorithms

Detailed walkthrough

Section II frames the setup. The Ising Hamiltonian H = ∑i hiZi + 2∑i<j JijZiZj is diagonal in the computational basis, so U_T = exp(-iTH) assigns a configuration-dependent phase exp(-iTE_s) — a continuous spectral oracle rather than a Boolean one. The key conceptual move is to ask whether alternating this with the Grover diffuser D_ξ still produces coherent amplification when no sharply marked subspace exists. The answer is yes, under a condition: a configuration becomes resonant when TE_s ≈ π (mod 2π), and the diffusion step couples energies only through their spectral average, so a finite phase neighbourhood around TE = π is amplified collectively.

Section III is the analytic heart. Equation 11 is the recurrence for energy-resolved amplitudes; Eq. 19 expresses a_{K-1}(E) as a contour integral of a "resonance kernel" divided by C_r(φ) = 2G(-re^{iφ}) - 1 where G(z) = ∑ g_m z^m. The radius r is an auxiliary parameter (the authors later fix 1-r = O(1/K)). The local linearisation C_r(φ) ≈ ε_eff + iκ_C(φ - φ_0) immediately gives the peak position (where Im C_r vanishes), the phase width ε_eff/|κ_C|, and the saturation height |κ_C|/ε_eff. This is a clean, very general susceptibility framework: any spectrum that gives g_m compatible with a singular response near φ = 0 yields Grover-type behaviour.

Section IV instantiates the framework for the annealed Gaussian density f_G(E) with variance Σ_n² = 2n(n-1)σ_J² + nσ_h². The characteristic-function samples are g_m = exp[-(mΣ_nT)²/2]; with the natural dimensionless tail parameter a = (Σ_nT)²/2 << 1 one obtains ε_G = 2√(π/a) exp(-π²/(4a)). The "high-density tail" regime is defined by parametrising the local mean spacing as Δ_n ~ nμ 2-n/2, which forces the target energy E* = O(n3/2). The arithmetic collapses to K_peak ~ √(2n/M_peak) with M_peak ~ n3-2μ — Grover scaling for a target band whose cardinality is determined by spectral physics rather than by user choice. For μ = 3/2 one selects O(1) levels; for smaller μ the resonance band grows polynomially.

Section V is where the spin-glass physics becomes load-bearing. The independent-energy approximation (random-energy model) gets the average density right but misses overlap-induced level correlations. Equation 27 gives the exact two-point covariance E[g_m g_ℓ*] = 2-n exp{-αn[(n-1)(m²+ℓ²) + 2mℓ]} ∑q C(n,q) exp[2αmℓ(n-2q)²] with q the Hamming distance between configurations. The q = 0, n terms give a persistent O(2-n/2) noise floor in the g_m sequence that propagates into C_r near the unit circle. The upshot (Eq. 32-34) is that the resonance centre φ_0 is displaced by an O(n-3) rms phase — small on spectral scales but large compared with the exponentially narrow resonance width.

Section VI addresses prescribed-energy targeting. The symmetrization trick (Eq. 41-42) adds an ancilla and replaces H by Z_a ⊗ H, doubling the spectrum to ±E_j and making g̃_m manifestly real — hence φ_0 = 0 exactly. The cost is three-body Z_aZ_iZ_j terms. Alternatively the time calibration T ← (π + φ_0(T))/E* is shown (Eq. 47-49) to converge in O(n/ln n) updates using only the measured bit string and its classical Ising energy — natural for an experimental loop. Section VII assembles total cost: each oracle call is O(n²) commuting ZZ rotations, so the gate cost of producing a resonance state is O(n² √(2n/M_peak)).

Section VIII shows numerics for n = 24. Figure 1 verifies the Gaussian local-response approximation. Figure 2 compares the discrete random Ising response with the annealed Gaussian: both show resonances near ET = ±π, but the Ising peak is shifted and distorted. Figure 3 zooms in on the resonance for two target energies, showing the predicted scaling of width and height with μ. The n = 18,...,36 scan in Fig. 4 verifies √⟨φ_0²⟩ = O(n-3).

Figures

Gaussian resonance profile
Figure 1. Amplification profile for an annealed Gaussian spectrum near the principal phase resonance ET = π. Horizontal axis is dimensionless phase ET/π; panels show amplitude magnitude after K = 2, 8, 16 iterations. Solid: exact spectral recurrence. Dashed: local resonant approximation. Parameters give ΣT ≈ 0.72. Agreement near ET/π = 1 illustrates that the local response captures the growth and narrowing of the Gaussian resonance.
Ising vs Gaussian energy-space amplification
Figure 2. Energy-space amplification profile for a single zero-field random Ising instance (n = 24, h_i = 0, J_ij ~ N(0,1)) compared with the annealed Gaussian prediction. Red: discrete Ising spectrum. Blue: annealed Gaussian. Both develop resonances near ET = ±π, but the discrete Ising response is shifted and distorted by spectral correlations.
Zoom of positive-energy resonance
Figure 3. Zoom of the positive-energy resonance at n = 24. Blue: annealed Gaussian. Red points: amplitudes on the discrete Ising energy levels. Dashed line: Gaussian target energy E* = π/T. Panel (a): denser tail (μ ≈ 0.6), broader/lower peak. Panel (b): sparser tail (μ ≈ 1.2), sharper/higher peak. In both, the discrete Ising peak is displaced from the Gaussian target — the realization-dependent shift φ_0.
phi0 scaling with system size
Figure 4. Scaling of the correlation-induced resonance displacement in the zero-field random Ising ensemble. σ_J = 1, J_ij ~ N(0,1), h_i = 0, μ = 3/2, truncated characteristic function with m ≤ 15. (a) Disorder-averaged ⟨φ_0²⟩ for n = 18,...,36; circles are Monte Carlo, squares are the finite-n covariance sum, dashed line is the asymptotic n-6 law. (b) Scaled quantity n6⟨φ_0²⟩ showing finite-size drift toward the asymptotic plateau. RMS displacement obeys √⟨φ_0²⟩ = O(n-3).

Citations to Yuan's papers

No direct citation to any of Y1–Y6 found in bibliography.

Overlap with Y1–Y6

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