Search arXiv⌕ Search

arXiv · 2611.00598

Quantum Diffusion and the Block-Size Crossover in the Block Anderson Model

Abstract

We study the block Anderson Hamiltonian \(H_L=λΨ_L+\mathcal V\) on the discrete torus \((\mathbb Z/L\mathbb Z)^d\), \(d\geq2\), where \(Ψ_L\) is the nearest-neighbor Laplacian and \(\mathcal V\) consists of independent \(W^d\times W^d\) GOE blocks. In the weak-disorder limit \(λ\to\infty\), we establish an entrywise local law, a spatial scaling limit for the squared resolvent entries, time-averaged dynamical delocalization, and lower bounds on the localization length of most bulk eigenfunctions. Particularly, we allow the block size to be fixed or grow above a polylogarithmic threshold. In sufficiently large polynomial volumes, the dynamical estimates hold for \(C_δ(λ+W/λ)\leq T\leq λ^{1+κ_d^{\rm BA}-δ}\), with a dimension-dependent exponent \(κ_d^{\rm BA}>0\), and the spreading scale is \(\sqrt{(λ^3+λW)T}\). This identifies a transition at \(W\asympλ^2\) between \(λ^{3/2}\sqrt T\) and \(\sqrt{λWT}\). The proof combines Gaussian moment estimates with deterministic stability of a matrix Dyson equation. A partial Bloch transform handles fixed blocks, while scalar reduction controls growing blocks. A Feshbach--Schur reduction of the block \(T\)-equation separates a single scalar diffusion mode from the stable internal cell modes. A renewal expansion and exact cell counting give a positive representation of the diffusion coefficient and control the fourth moment uniformly across the block-size transition. Notably, our argument does not require an enumeration of Feynman diagrams.

Explore related subjects

Keep this discovery

Explore connections, maps & timelines

BibTeXRIS

Haoxuan Fu. 2026-10-31. Quantum Diffusion and the Block-Size Crossover in the Block Anderson Model. https://arxiv.org/abs/2611.00598

Cite the original work for its findings. Save a collection to share your selection of sources.

KEEP EXPLORING

Related papers

Quantitative Propagation of Chaos for Singular Interacting Particle Systems Driven by Fractional Brownian Motion

We consider interacting systems particle driven by i.i.d. fractional Brownian motions, subject to irregular, possibly distributional, pairwise interactions. We show propagation of chaos and mean field convergence to the law of the associated McKean--Vlasov equation, as the number of particles $N\to\infty$, with quantitative sharp rates of order $N^{-1/2}$. Our results hold for a wide class of possibly time-dependent interactions, which are only assumed to satisfy a Besov-type regularity, related to the Hurst parameter $H\in (0,+\infty)\setminus \mathbb{N}$ of the driving noises. In particular, as $H$ decreases to $0$, interaction kernels of arbitrary singularity can be considered, a phenomenon frequently observed in regularization by noise results. Our proofs rely on a combinations of Sznitman's direct comparison argument with stochastic sewing techniques.

math.PR↗

Power rate of convergence of discrete curves: framework and applications

We develop a framework for power-law rates of convergence of random discrete curves to Schramm Loewner Evolution (SLE). We show that a power-law rate of convergence of a suitable martingale observable gives a power-law rate of convergence of the interface to SLE, provided the discrete curves satisfy the Kemppainen-Smirnov crossing condition; the proof uses known estimates on the derivative of the SLE map. We apply the framework to the exploration process of critical site percolation on the triangular lattice, obtaining a power-law rate of convergence to SLE$_6$.

math.PR↗

Refining Concentration Bounds for Gaussian Quadratic Chaos with Applications

This paper studies concentration of measure for Gaussian quadratic chaos in the non-asymptotic regime. We begin by tightening the classic Hanson-Wright inequality, where we increase its absolute constant $κ$ from 0.125 to at least 0.1457 in the symmetric case. We present a sharper version of Laurent-Massart inequality (LMI), which increases $κ$ from the largest available value of $1-\frac{\sqrt{3}}{2}\approx 0.134$ to $\frac{9-\sqrt{17}}{32}\approx 0.152$ in the positive-semidefinite case. We develop a sequence of inequalities indexed by $m\ge1$ that involve Schatten norms of the underlying matrix. The case $m=1$ recovers HWI. The bounds undergo a phase transition in the sense that if the tail parameter is smaller than a critical threshold $τ_c$, then $m=1$ is the tightest, whereas if it is larger than $τ_c$, then $m=\infty$ is the tightest. This leads to a novel bound called the $m_\infty$ bound. All HWI, LMI and the $m_\infty$ inequality rely on Markov's inequality. By avoiding Markov's inequality, we introduce the strong and weak $χ^2$ inequalities. We provide a list of concentration bounds that depend only on the operator norm in the positive-definite case, namely, the $m_\infty$ bound, the weak $χ^2$ bound, relaxed versions of HWI and LMI, and the so-called large-deviations bound. The sharpest among these is shown to be always either the $m_\infty$ bound or the weak $χ^2$ bound. By utilizing conditioning, modified versions of $m_\infty$, $χ^2$, and HW inequalities of various orders are proposed, all of which can be significantly tighter than the original inequalities. By leveraging the Ruben-Kotz expansion for the distribution of a positive-definite quadratic form, we introduce the Ruben-Kotz inequalities (RKIs) for general symmetric quadratic forms. A key advantage of RKIs is that they provide an explicit upper bound on the approximation gap.

math.PR↗