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Linear-2 Eigenvector Quantization

Updated 27 January 2026
  • Eigenvector quantization using the Linear-2 method approximates the ground-state eigenvector of real symmetric matrices with nonpositive off-diagonals by exploiting a linear relationship with the row-sum vector.
  • It employs a one-parameter variational optimization to minimize the Rayleigh quotient, achieving errors below 10⁻³ and dramatically lowering computational complexity compared to full diagonalization.
  • The method is validated on diverse systems—including RRSMs, Hubbard models, and transverse-field Ising models—demonstrating robust performance across matrix sizes and configurations.

Eigenvector quantization in the form of the Linear-2 method provides an explicit, computationally efficient approach to directly approximate the ground-state eigenvector of real symmetric matrices with non-positive off-diagonal entries—commonly referred to as real random symmetric matrices (RRSM) of this specific type. The procedure leverages an observed linear relationship between the ground-state eigenvector and the row-sums of the matrix, allowing ground-state properties to be captured without full diagonalization. This approach is particularly significant for large-scale quantum and statistical systems modeled in condensed matter physics and related fields (Pan et al., 2019).

1. Class of Matrices and Assumptions

The Linear-2 method applies to N×NN \times N real symmetric matrices HH where all off-diagonal elements satisfy Hij0H_{ij} \leq 0 for iji \neq j, with diagonal entries HiiH_{ii} arbitrary. The target is the unique ground-state eigenvector G=(g1,,gN)TG = (g_1, \ldots, g_N)^T associated with the smallest eigenvalue; uniqueness is guaranteed by the Perron–Frobenius theorem under these conditions. No further structure is required: the method applies to both dense and sparse matrices, with random (uniform or Gaussian) or model-derived entries, including systems such as the Hubbard and transverse-field Ising models (Pan et al., 2019).

2. Linear Scaling Law and Ansatz

Define the row-sum vector SS (sometimes denoted SME) by

Si=j=1NHijS_i = \sum_{j=1}^N H_{ij}

for i=1,,Ni=1, \ldots, N. Empirically, after normalizing SS and the ground-state eigenvector GG to unit Euclidean norm (G2=S2=1\|G\|_2 = \|S\|_2 = 1), a robust linear relationship emerges: giSi.g_i \simeq -S_i. For finite NN, the Linear-2 ansatz introduces a one-parameter affine shift: vi(c)=Si+c,g(c)=v(c)v(c)2v_i(c) = S_i + c, \quad g(c) = \frac{v(c)}{\|v(c)\|_2} or equivalently,

gi=α+βSig_i = \alpha + \beta S_i

with β1\beta \approx 1 and α\alpha (related to cc) chosen via variational minimization with respect to the Rayleigh quotient. This ansatz maintains normalization and aligns with the optimal energy estimate (Pan et al., 2019).

3. Justification and Empirical Scaling

Justification for the scaling law arises from the Perron–Frobenius theorem, which ensures all ground-state components gi0g_i \geq 0 and guarantees uniqueness. A mean-field-type argument relates minimizing GHG\langle G|H|G\rangle with giSig_i \propto S_i under the described matrix conditions. Numerical tests on O(104)\mathcal{O}(10^4) random RRSMs with NN ranging from 10210^2 up to 10410^4—including dense and sparse scenarios with uniform or Gaussian entries—demonstrate that gig_i versus SiS_i shows an almost perfect linearity, slope 1-1, and zero intercept.

The root-mean-square (RMS) deviation

rms=1Ni(gi+Si)2\text{rms} = \sqrt{\frac{1}{N}\sum_i (g_i + S_i)^2}

drops below 10310^{-3} at N103N \approx 10^3 and decreases further for larger matrices. The linear correlation persists even with selective large-row rescalings. For diagonally-dominated or banded matrices, the strict giSig_i \propto -S_i law is dampened but a positive correlation is retained (Pan et al., 2019).

4. Variational Algorithm for Eigenvector Quantization

The Linear-2 method is operationalized via a one-parameter variational optimization, minimizing the Rayleigh quotient with respect to cc in the ansatz gi=Si+cg_i = S_i + c. The procedure is as follows:

  • Inputs: HH (N×NN \times N real symmetric, Hij0H_{ij} \leq 0 for iji \neq j).
  • Precomputation:
    • e(1,1,,1)TRNe \gets (1,1,\ldots,1)^T \in \mathbb{R}^N
    • SHeS \gets H e (row sums)
    • DSTSD \gets S^T S
    • E1STeE_1 \gets S^T e
    • FeTe=NF \gets e^T e = N
    • AST(HS)A \gets S^T(H S)
    • BST(He)B \gets S^T(H e)
    • CeT(He)C \gets e^T(H e)
  • Rayleigh quotient:
    • numerator(c)=A+2cB+c2C\text{numerator}(c) = A + 2cB + c^2C
    • denominator(c)=D+2cE1+c2F\text{denominator}(c) = D + 2cE_1 + c^2F
    • E(c)=numerator(c)denominator(c)E(c) = \frac{\text{numerator}(c)}{\text{denominator}(c)}
  • Minimization: Iteratively update cc (e.g., using Newton's method), stopping when Δc<108|\Delta c| < 10^{-8}, to minimize E(c)E(c).
  • Final eigenvector: viSi+c0v_i \gets S_i + c_0, g=v/v2g = v / \|v\|_2, and EmingTHgE_{\min} \approx g^T H g.

For typical RRSMs as N1N \gg 1, c00c_0 \to 0 and the relationship gS/Sg \approx -S / \|S\| holds. The dominant computational cost is forming S=HeS = H e, an O(N2)\mathcal{O}(N^2) operation for dense matrices, reducing to O(H0)\mathcal{O}(\|H\|_0) for sparse inputs. The single-parameter optimization adds negligible cost (Pan et al., 2019).

5. Computational Cost and Accuracy

The Linear-2 method requires:

  • O(N2)\mathcal{O}(N^2) operations for dense HH to compute SS and a few quadratic forms.
  • O(nnz)\mathcal{O}(\text{nnz}) operations for sparse HH with nnz nonzero entries.
  • Memory usage O(N2)\mathcal{O}(N^2) (dense) or O(nnz)\mathcal{O}(\text{nnz}) (sparse).
  • Empirical ground-state energy errors <103<10^{-3} for random N100N \geq 100, with errors diminishing as NN increases.

Compared to full diagonalization (O(N3)\mathcal{O}(N^3)), the Linear-2 method offers significant computational savings, especially for large NN (Pan et al., 2019).

6. Representative Applications and Performance

The efficacy and generality of the Linear-2 method are demonstrated on several classes of matrices:

Matrix Type N or Dimension Observations
Random RRSM (uniform/Gaussian) N=100N=1001000010\,000 gig_i vs SiS_i linear (slope 1-1, intercept 0\approx 0); RMS <103<10^{-3} for N103N\gtrsim 10^3
1D 4-site half-filled Hubbard model 36×3636 \times 36 U/t=0,1U/t = 0,1, all off-diagonal 0\leq 0; c00.00954c_0 \approx 0.00954 (U=0U=0), 0.0137-0.0137 (U=1U=1); ΔE0.002|\Delta E| \approx 0.002 (U=0U=0), $0.0077$ (U=1U=1)
1D transverse-field Ising chain L=4L=4 to $14$ (dim 2L2^L) gig_i vs SiS_i linear; EscalingEexact/Eexact<104|E_{\text{scaling}} - E_{\text{exact}}|/|E_{\text{exact}}| < 10^{-4} across all LL

Empirical performance indicates that accuracy improves further with increasing NN. The methodology also maintains a strong positive correlation for matrices outside the strict class if diagonal dominance or bandedness is present, with the linear law holding less precisely (Pan et al., 2019).

7. Summary and Scope

The Linear-2 eigenvector quantization method provides a scalable, accurate tool for approximating the ground-state eigenvector of real symmetric matrices with nonpositive off-diagonal entries, with immediate applications in quantum many-body physics and network theory. The technique leverages a universal linear scaling law, justifiable by mean-field reasoning and empirically validated across both random and model Hamiltonians. Its computational advantages are most pronounced in large-scale or high-dimensional settings where traditional diagonalization is infeasible (Pan et al., 2019).

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