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arXiv:2610.15530

Breakdown of thermalization in quantum spin systems with long-range interactions

Filippo Caleca, Fabio Mezzacapo, Tommaso Roscilde

quant-phcond-mat.stat-mechSubmitted Oct 11, 2026• Announced Oct 13, 2026• 0 citations• Revised Oct 26, 2026 (v2)
v1 · Oct 11, 2026v2 · Oct 26, 2026
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Abstract

Quantum thermalization of closed systems -- i.e. the relaxation of local properties to their thermodynamic value along the Hamiltonian evolution -- is generically expected in non-integrable systems at finite energy density. In this work we show that quantum spin systems with at least one spin component coupled through long-range ferromagnetic interactions, and a second spin component coupled to a field, cannot in general thermalize to a paramagnetic state whenever they have a finite, negative energy per spin. The long-range interactions we consider decay as a power law of the distance, $\sim r^{-α}$ with $α< d$, where $d$ is the number of spatial dimensions of the system. The lack of thermalization is generic to an infinite family of Hamiltonians, and it is not associated to any form of integrability. It can instead be understood by the anomalous features of the thermodynamics of the system in the paramagnetic phase, which cannot be reflected in the properties of the eigenstates. This leads to a breakdown of eigenstate typicality and of the eigenstate thermalization hypothesis. Interestingly, the non-thermal states emerging at long times in the dynamics display long-range multipartite entanglement, elevating the breakdown of thermalization to a resource.

AI Summary

The paper asks whether nonintegrable quantum spin systems with nonadditive, Kac-normalized ferromagnetic interactions $r^{-\alpha}$, $\alpha<d$, can thermalize to a paramagnetic Gibbs state at finite negative energy density. It proposes a mechanism for ETH violation: transverse interaction energy is subextensive in thermal paramagnetic states, while atypical eigenstates retain extensive transverse interaction energy and long-range correlations. The numerical study concentrates on a one-dimensional spin-$1/2$ XX model with $\alpha=0.5$ and a field along $x$. Quantum Monte Carlo finds thermal transverse correlations approximately scaling as $C_y(r)=N^{-1}g(r/N)$. Exact diagonalization up to $N=22$, within a resolved symmetry sector, finds broadly distributed eigenstate expectation values despite level repulsion compatible with Wigner–Dyson statistics. Eigenstate fluctuations show little size dependence at negative energies, unlike the short-range comparison at $\alpha=3$. Threshold-based counts suggest exponentially many atypical eigenstates, although their fraction tends to zero. Quenches from a coherent spin state opposite to the field are studied using matrix-product states up to $N=48$, time-dependent variational Monte Carlo up to $N=100$, and rotor-plus-spin-wave theory. At $\Omega/\mathcal J=0.3$, the simulated magnetization remains opposite to the field and transverse fluctuations reach $\langle(J^y)^2\rangle=O(N^2)$, implying extensive quantum Fisher information density for these pure states. The general argument is supported numerically primarily for this model. Canonical–microcanonical equivalence is inferred rather than proved. The dynamical interpretation assumes dilute, stable spin waves; the supplemental analysis finds decreasing excitation density with increasing size.

No sign of AI-generated textOverclaimsPossible error

Central claim may not hold: The claimed extension to a broad family of long-range ferromagnetic Hamiltonians is not established by the model-specific numerical evidence and the invalid general argument. The estimated vanishing fraction of exceptional eigenstates can violate strong ETH without establishing that most eigenstates fail thermal typicality. The finite-time dynamics and approximate rotor–spin-wave treatment do not exclude eventual thermalization at finite size or establish nonthermalization independently of the order of limits. The central argument incorrectly infers that eigenstates of H must approach eigenstates of H_parallel from the vanishing expectation value of H_perp per spin, so its claimed contradiction with ETH does not follow. The displayed folded GOE spacing-ratio density has an incorrect normalization prefactor: it should be 27/4 rather than 8/27.

Written by gpt-6.1-sol from the paper's full text. Automated: it can be wrong.

Comments
4.5+2+2.5 pages, 3+4+3 figures

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Quantum thermalization of closed systems -- i.e. the relaxation of local properties to their thermodynamic value along the Hamiltonian evolution -- is generically expected in non-integrable systems at finite energy density. In this work we show that quantum spin systems with at least one spin component coupled through long-range ferromagnetic interactions, and a second spin component coupled to a field, cannot in general thermalize to a paramagnetic state whenever they have a finite, negative energy per spin. The long-range interactions we consider decay as a power law of the distance, ∼r−α\sim r^{-α}∼r−α with α<dα< dα<d, where ddd is the number of spatial dimensions of the system. The lack of thermalization is generic to an infinite family of Hamiltonians, and it is not associated to any form of integrability. It can instead be understood by the anomalous features of the thermodynamics of the system in the paramagnetic phase, which cannot be reflected in the properties of the eigenstates. This leads to a breakdown of eigenstate typicality and of the eigenstate thermalization hypothesis. Interestingly, the non-thermal states emerging at long times in the dynamics display long-range multipartite entanglement, elevating the breakdown of thermalization to a resource.
The paper asks whether nonintegrable quantum spin systems with nonadditive, Kac-normalized ferromagnetic interactions r−αr^{-\alpha}r−α, α<d\alpha<dα<d, can thermalize to a paramagnetic Gibbs state at finite negative energy density. It proposes a mechanism for ETH violation: transverse interaction energy is subextensive in thermal paramagnetic states, while atypical eigenstates retain extensive transverse interaction energy and long-range correlations.
The numerical study concentrates on a one-dimensional spin-1/21/21/2 XX model with α=0.5\alpha=0.5α=0.5 and a field along xxx. Quantum Monte Carlo finds thermal transverse correlations approximately scaling as Cy(r)=N−1g(r/N)C_y(r)=N^{-1}g(r/N)Cy​(r)=N−1g(r/N). Exact diagonalization up to N=22N=22N=22, within a resolved symmetry sector, finds broadly distributed eigenstate expectation values despite level repulsion compatible with Wigner–Dyson statistics. Eigenstate fluctuations show little size dependence at negative energies, unlike the short-range comparison at α=3\alpha=3α=3. Threshold-based counts suggest exponentially many atypical eigenstates, although their fraction tends to zero.
Quenches from a coherent spin state opposite to the field are studied using matrix-product states up to N=48N=48N=48, time-dependent variational Monte Carlo up to N=100N=100N=100, and rotor-plus-spin-wave theory. At Ω/J=0.3\Omega/\mathcal J=0.3Ω/J=0.3, the simulated magnetization remains opposite to the field and transverse fluctuations reach ⟨(Jy)2⟩=O(N2)\langle(J^y)^2\rangle=O(N^2)⟨(Jy)2⟩=O(N2), implying extensive quantum Fisher information density for these pure states.
The general argument is supported numerically primarily for this model. Canonical–microcanonical equivalence is inferred rather than proved. The dynamical interpretation assumes dilute, stable spin waves; the supplemental analysis finds decreasing excitation density with increasing size.
Understanding how closed quantum systems dynamically approach thermal equilibrium presents a major unresolved problem in statistical physics. Generically, non-integrable quantum systems are expected to thermalize as they comply with the Eigenstate Thermalization Hypothesis. However, in the presence of strong disorder, the dynamics can possibly slow down to a degree that systems fail to thermalize on experimentally accessible timescales, as in spin glasses or many-body localized systems. In general, particularly in long-range interacting quantum systems, the specific nature of the disorder necessary for the emergence of a prethermal, metastable state--distinctly separating the timescales of initial relaxation and subsequent slow thermalization--remains an open question. We study an ensemble of Heisenberg spins with a tunable distribution of random coupling strengths realized by a Rydberg quantum simulator. We observe a drastic change in the late-time magnetization when increasing disorder strength. The data is well described by models based on pairs of strongly interacting spins, which are treated as thermal for weak disorder and isolated for strong disorder. Our results indicate a crossover into a pair-localized prethermal regime in a closed quantum system of thousands of spins in the critical case where the exponent of the power law interaction matches the spatial dimension.
By developing a semiclassical analysis based on the eigenstate thermalization hypothesis, we determine the long time behavior of a large spin evolving with a nonlinear Hamiltonian. Despite integrable classical dynamics, we find the eigenstate thermalization hypothesis for the diagonal matrix elements of observables is satisfied in the majority of eigenstates, and thermalization of long time averaged observables is generic. The exception is an unusual mechanism for the breakdown of thermalization based on an unstable fixed point in the classical dynamics. Using the semiclassical analysis, we derive how the equilibrium values of observables encode properties of the initial state. This analysis shows an unusual memory effect in which the remembered initial state property is not conserved in the integrable classical dynamics. We conclude with a discussion of relevant experiments and the potential generality of this mechanism for long time memory and the breakdown of thermalization.
A very fundamental problem in quantum statistical mechanics involves whether—and how—an isolated quantum system will reach thermal equilibrium after waiting a long time. In quantum systems that do thermalize, the long-time expectation value of any “reasonable” operator will match its predicted value in the canonical ensemble. The Eigenstate Thermalization Hypothesis (ETH) posits that this thermalization occurs at the level of each individual energy eigenstate; in fact, any single eigenstate in a microcanonical energy window will predict the expectation values of such operators exactly. In the first part of this dissertation, we identify, for a generic model system, precisely which operators satisfy ETH, as well as limits to the information contained in a single eigenstate. Remarkably, our results strongly suggest that a single eigenstate can contain information about energy densities—and therefore temperatures—far away from the energy density of the eigenstate.Additionally, we study the possible breakdown of quantum thermalization in a model of itinerant electrons on a one-dimensional chain, with both spin and charge degrees of freedom. This model exhibits peculiar properties in the entanglement entropy, the apparent scaling of which is modified from a “volume law” to an “area law” after performing a partial, site-wise measurement on the system. These properties and others suggest that this model realizes a new, non-thermal phase of matter, known as a Quantum Disentangled Liquid (QDL). The putative existence of this phase has striking implications for the foundations of quantum statistical mechanics.
We investigate the eigenstate thermalization hypothesis (ETH) in integrable models, focusing on the $\text{spin}\ensuremath{-}\frac{1}{2}$ isotropic Heisenberg (XXX)(XXX)(XXX) chain. We provide numerical evidence that the ETH holds for typical eigenstates (weak ETH scenario). Specifically, using a numerical implementation of state-of-the-art Bethe ansatz results, we study the finite-size scaling of the eigenstate-to-eigenstate fluctuations of the reduced density matrix. We find that fluctuations are normally distributed, and their standard deviation decays in the thermodynamic limit as ${L}^{\ensuremath{-}1/2}$, with LLL the size of the chain. This is in contrast with the exponential decay that is found in generic nonintegrable systems. Based on our results, it is natural to expect that this scenario holds in other integrable spin models and for typical local observables. Finally, we investigate the entanglement properties of the excited states of the XXXXXXXXX chain. We numerically verify that typical midspectrum eigenstates exhibit extensive entanglement entropy (i.e., volume-law scaling).
The eigenstate thermalization hypothesis (ETH) is a successful theory that establishes the criteria for ergodicity and thermalization in isolated quantum many-body systems. In this work, we investigate the thermalization properties of spin-$ 1/2 $ XXZ chain with linearly-inhomogeneous interactions. We demonstrate that introduction of the inhomogeneous interactions leads to an onset of quantum chaos and thermalization, which, however, becomes inhibited for sufficiently strong inhomogeneity. To exhibit ETH, and to display its breakdown upon varying the strength of interactions, we probe statistics of energy levels and properties of matrix elements of local observables in eigenstates of the inhomogeneous XXZ spin chain. Moreover, we investigate the dynamics of the entanglement entropy and the survival probability which further evidence the thermalization and its breakdown in the considered model. We outline a way to experimentally realize the XXZ chain with linearly-inhomogeneous interactions in systems of ultracold atoms. Our results highlight a mechanism of emergence of ETH due to insertion of inhomogeneities in an otherwise integrable system and illustrate the arrest of quantum dynamics in presence of strong interactions.
The eigenstate thermalization hypothesis (ETH) is a successful theory that establishes the criteria for ergodicity and thermalization in isolated quantum many-body systems. In this work, we investigate the thermalization properties of a spin-1/21/21/2 XXZ chain with linearly inhomogeneous interactions. We demonstrate that introduction of the inhomogeneous interactions leads to an onset of quantum chaos and thermalization, which, however, becomes inhibited for sufficiently strong inhomogeneity. To exhibit ETH, and to display its breakdown upon varying the strength of interactions, we probe statistics of energy levels and properties of matrix elements of local observables in eigenstates of the inhomogeneous XXZ spin chain. Moreover, we investigate the dynamics of the entanglement entropy and the survival probability which further evidence the thermalization and its breakdown in the considered model. We outline a way to experimentally realize the XXZ chain with linearly inhomogeneous interactions in systems of ultracold atoms. Our results highlight a mechanism of emergence of ETH due to insertion of inhomogeneities in an otherwise integrable system and illustrate the arrest of quantum dynamics in the presence of strong interactions.