Another Return of 'Return to Equilibrium'
arXiv:math-ph/0410011 · doi:10.1007/s00220-004-1176-6
Abstract
The property of ``{\it return to equilibrium}'' is established for a class of quantum-mechanical models describing interactions of a (toy) atom with black-body radiation, or of a spin with a heat bath of scalar bosons, under the assumption that the interaction strength is {\it sufficiently weak}. For models describing the first class of systems, our upper bound on the interaction strength is {\it independent} of the temperature , (with ), while, for the spin-boson model, it tends to zero logarithmically, as . Our result holds for interaction form factors with physically realistic infrared behaviour. Three key ingredients of our analysis are: a suitable concrete form of the Araki-Woods representation of the radiation field, Mourre's positive commutator method combined with a recent virial theorem, and a norm bound on the difference between the equilibrium states of the interacting and the non-interacting system (which, for the system of an atom coupled to black-body radiation, is valid for {\it all} temperatures , assuming only that the interaction strength is sufficiently weak).
References in corpus (5)
Cited by in corpus (30)
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