Linear growth of the entanglement entropy and the Kolmogorov-Sinai rate

dc.creatorEugenio Bianchi
dc.creatorLucas Fabian Hackl
dc.creatorNelson de Oliveira Yokomizo
dc.date.accessioned2025-08-29T17:53:19Z
dc.date.accessioned2025-09-09T01:07:27Z
dc.date.available2025-08-29T17:53:19Z
dc.date.issued2018
dc.description.sponsorshipCNPq - Conselho Nacional de Desenvolvimento Científico e Tecnológico
dc.format.mimetypepdf
dc.identifier.doihttps://doi.org/10.1007/JHEP03(2018)025
dc.identifier.issn1029-8479
dc.identifier.urihttps://hdl.handle.net/1843/84724
dc.languageeng
dc.publisherUniversidade Federal de Minas Gerais
dc.rightsAcesso Aberto
dc.subjectTeoria de campos
dc.subjectTeoria quântica de campos
dc.subjectSistemas quânticos
dc.subject.otherField theories in lower dimensions
dc.subject.otherLattice quantum field theory
dc.subject.otherQuantum dissipative systems
dc.titleLinear growth of the entanglement entropy and the Kolmogorov-Sinai rate
dc.typeArtigo de periódico
local.citation.epage68
local.citation.issue3
local.citation.spage1
local.citation.volume2018
local.description.resumoThe rate of entropy production in a classical dynamical system is characterized by the Kolmogorov-Sinai entropy rate hKS given by the sum of all positive Lyapunov exponents of the system. We prove a quantum version of this result valid for bosonic systems with unstable quadratic Hamiltonian. The derivation takes into account the case of time-dependent Hamiltonians with Floquet instabilities. We show that the entanglement entropy SA of a Gaussian state grows linearly for large times in unstable systems, with a rate ΛA ≤ hKS determined by the Lyapunov exponents and the choice of the subsystem A. We apply our results to the analysis of entanglement production in unstable quadratic potentials and due to periodic quantum quenches in many-body quantum systems. Our results are relevant for quantum field theory, for which we present three applications: a scalar field in a symmetry-breaking potential, parametric resonance during post-inflationary reheating and cosmological perturbations during inflation. Finally, we conjecture that the same rate ΛA appears in the entanglement growth of chaotic quantum systems prepared in a semiclassical state.
local.identifier.orcidhttps://orcid.org/0000-0001-7847-9929
local.identifier.orcidhttps://orcid.org/0000-0002-4172-0317
local.identifier.orcidhttps://orcid.org/0000-0002-0732-8733
local.publisher.countryBrasil
local.publisher.departmentICX - DEPARTAMENTO DE FÍSICA
local.publisher.initialsUFMG
local.url.externahttps://link.springer.com/article/10.1007/JHEP03(2018)025

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