2015
DOI: 10.1088/1367-2630/17/4/045002
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Extremely quick thermalization in a macroscopic quantum system for a typical nonequilibrium subspace

Abstract: Extremely quick thermalization in a macroscopic quantum system for a typical nonequilibrium subspace AbstractThe fact that macroscopic systems approach thermal equilibrium may seem puzzling, for example, because it may seem to conflict with the time-reversibility of the microscopic dynamics. We here prove that in a macroscopic quantum system for a typical choice of 'nonequilibrium subspace', any initial state indeed thermalizes, and in fact does so very quickly, on the order of the Boltzmann time τ = h k T :.… Show more

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Cited by 89 publications
(126 citation statements)
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“…(1)] than the measure of all t ∈ ½0; T. Altogether, we thus can conclude that, for the overwhelming majority of U's, the difference hAi ρðtÞ − hAi¯ρ remains below the resolution limit δA for the vast majority of times t contained in any sufficiently large time interval ½0; T. The same conclusion carries over to our actual Hamiltonian H and observable A, given their eigenbases are related by a typical transformation U as discussed above. To establish quantitative bounds for T is a subject of considerable current interest [8,13,[29][30][31][32] but goes beyond our present scope. The salient point is that (5) holds independently of the initial condition ρð0Þ.…”
mentioning
confidence: 99%
“…(1)] than the measure of all t ∈ ½0; T. Altogether, we thus can conclude that, for the overwhelming majority of U's, the difference hAi ρðtÞ − hAi¯ρ remains below the resolution limit δA for the vast majority of times t contained in any sufficiently large time interval ½0; T. The same conclusion carries over to our actual Hamiltonian H and observable A, given their eigenbases are related by a typical transformation U as discussed above. To establish quantitative bounds for T is a subject of considerable current interest [8,13,[29][30][31][32] but goes beyond our present scope. The salient point is that (5) holds independently of the initial condition ρð0Þ.…”
mentioning
confidence: 99%
“…Finally, we noted that fast thermalization on timescales of order the inverse temperature seems to be generic for broad classes of quantum states and Hamiltonians [10,11]. If, as is sometimes conjectured, all QFTs have gravitational duals, this result might be understood in terms of horizon formation: the timescale for gravitational collapse is of order the light crossing time of the resulting black hole, which is roughly the inverse temperature.…”
Section: Resultsmentioning
confidence: 66%
“…Explicit demonstrations of fast quantum thermalization have been obtained for broad classes initial states, on timescales of order the inverse temperature (i.e., average energy per mode) [10,11]. Indeed the conceptual challenge is to understand the conditions which lead to the more familiar slow (semi-classical) thermalization.…”
Section: Quantum Thermalization and Properties Of Typical Pure Statesmentioning
confidence: 99%
“…The former is important since equilibration on very long time-scales would mean we can never actually observe it. General bounds on thermalization times, based on very few generic assumptions, are available [32][33][34][35][36][37], but they are far off from those observed in numerical calculations and actual experiments, see Ref. [28] and references therein.…”
Section: Quantum Thermalizationmentioning
confidence: 99%
“…The center-of-mass motion then decouples, and the z motion is free. The relative Hamiltonian then readŝ 37) where r = r 2 − r 1 is the relative coordinate between the two atoms and the transverse…”
Section: Interactions In Ultra-cold Gasesmentioning
confidence: 99%