Closeness of the reduced density matrix of an interacting small system
to the Gibbs state
- URL: http://arxiv.org/abs/2003.09258v2
- Date: Thu, 6 Aug 2020 07:56:17 GMT
- Title: Closeness of the reduced density matrix of an interacting small system
to the Gibbs state
- Authors: Wen-ge Wang
- Abstract summary: I study the statistical description of a small quantum system, which is coupled to a large quantum environment in a generic form.
The focus is on the difference between the reduced density matrix (RDM) of the central system in this interacting case.
I also study the RDM which is computed from a typical state of the total system within an energy shell.
- Score: 0.0
- License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/
- Abstract: I study the statistical description of a small quantum system, which is
coupled to a large quantum environment in a generic form and with a generic
interaction strength, when the total system lies in an equilibrium state
described by a microcanonical ensemble. The focus is on the difference between
the reduced density matrix (RDM) of the central system in this interacting case
and the RDM obtained in the uncoupled case. In the eigenbasis of the central
system's Hamiltonian, it is shown that the difference between diagonal elements
is mainly confined by the ratio of the maximum width of the eigenfunctions of
the total system in the uncoupled basis to the width of the microcanonical
energy shell; meanwhile, the difference between off-diagonal elements is given
by the ratio of certain property of the interaction Hamiltonian to the related
level spacing of the central system. As an application, a sufficient condition
is given, under which the RDM may have a canonical Gibbs form under
system-environment interactions that are not necessarily weak; this Gibbs state
usually includes certain averaged effect of the interaction. For central
systems that interact locally with many-body quantum chaotic systems, it is
shown that the RDM usually has a Gibbs form. I also study the RDM which is
computed from a typical state of the total system within an energy shell.
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