NTH

When quantum thermal states look classical

AuthorsHarald Putterman, Alexander Zlokapa, Jordan Cotler

August 5, 2026 2 min read
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The one-line take

The paper shows that surprisingly hot quantum systems can remain classically tractable long after entanglement and other quantum features begin to appear.

Key results

72
Separability guarantee constant

The Gibbs state is separable for β ≤ 1/(72sk).

4096
Classical preparation constant

Polynomial-time preparation works for β ≤ 1/(4096e sk).

What the paper found

Harald Putterman, Alexander Zlokapa of MIT, and Jordan Cotler of Harvard University show that quantum Gibbs states can remain classically tractable across several distinct finite-temperature regimes, even for long-range Pauli Hamiltonians whose terms act on at most k qubits and have total incident strength at most s. Their hierarchy begins with separability: the Gibbs state is guaranteed unentangled for inverse temperature β ≤ 1/(72sk), and this Θ(1/(sk)) threshold is tight, including for commuting Hamiltonians. A randomized polynomial-time algorithm prepares the state as a mixture of pure product stabilizer states up to β ≤ 1/(4096e sk), ruling out the proposed superpolynomial quantum advantage in this regime. For Hamiltonians ε-close to commuting, stabilizerness persists to the parametrically colder scale Θ(log(1/ε)/(sk)), separating the disappearance of entanglement from the disappearance of magic. Independently, a cluster expansion based on Pauli-specific polymer counting establishes a zero-free partition-function disk of radius Θ(1/(s√k)); within it, local thermal expectations and log Z are estimable in randomized polynomial time, and geometrically local systems exhibit exponential correlation decay. The proofs combine Kotecký–Preiss cluster expansions, interaction-picture Dyson expansions, adaptive pinning, and importance sampling of polymers. The paper also acknowledges that ChatGPT Pro contributed to technical appendices and proof development, while the authors retained responsibility for correctness.

Original abstract

At high temperature, quantum Gibbs states retain several classical features of the maximally mixed state: the absence of entanglement, the absence of magic, analyticity of the partition function, correlation decay, and algorithmic tractability. We prove new and sharp bounds showing that these features persist down to finite temperatures independent of system size, but fail at distinct inverse-temperature scales, forming a hierarchy of classical-to-quantum transitions. Our results hold for long-range Pauli interactions with bounded strength at every site. Despite such all-to-all interactions, we show that the death of entanglement occurs at constant temperature, resolving an open question of Rouze, Franca and Alhambra (STOC'25). We give a polynomial-time classical algorithm that prepares Gibbs states up to the death of entanglement transition. Notably, this is asymptotically colder than temperatures at which quantum Gibbs samplers are known to mix quickly, as well as the original separability temperature of Bakshi et al. (FOCS'24), which we improve to be tight up to constants. At asymptotically even colder temperatures, we show that the Gibbs state remains in the thermodynamic infinite-temperature phase. This leads to polynomial-time classical algorithms for estimating thermal expectations despite both entanglement and magic, and the resolution of a correlation decay conjecture of Harrow, Mehraban and Soleimanifar (STOC'20).

Read the original paper

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