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Approach to thermal equilibrium of macroscopic quantum systems

2009/11/09 by Sheldon Goldstein, Joel L. Lebowitz, Christian Mastrodonato +3 · 10 citations
Physics and Astronomy · #Advanced Thermodynamics and Statistical Mechanics #Quantum and electron transport phenomena #Quantum many-body systems #cond-mat.stat-mech #quant-ph

paper · pdf · doi:10.1103/physreve.81.011109

published as Phys. Rev. E 81: 011109 (2010) · 19 pages LaTeX, no figures

arxiv created 2009/11/09 · openalex publication_date 2010/01/07 · arxiv updated 2010/04/07 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28

Abstract

We consider an isolated macroscopic quantum system. Let H be a microcanonical ``energy shell,'' i.e., a subspace of the system's Hilbert space spanned by the (finitely) many energy eigenstates with energies between E and E+\ensuremathδE. The thermal equilibrium macrostate at energy E corresponds to a subspace Heq of H such that dim Heq/dim H is close to 1. We say that a system with state vector \ensuremathψ∊H is in thermal equilibrium if \ensuremathψ is ``close'' to Heq. We show that for ``typical'' Hamiltonians with given eigenvalues, all initial state vectors \ensuremathψ0 evolve in such a way that \ensuremathψt is in thermal equilibrium for most times t. This result is closely related to von Neumann's quantum ergodic theorem of 1929.

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