Published June 2011 | Version v1
Journal article

Quantum quench dynamics of the Bose-Hubbard model at finite temperatures

  • 1. FOCUS Center and MCTP, Department of Physics, University of Michigan, Ann Arbor, Michigan 48109 (United States)
  • 2. Beijing National Laboratory for Condensed Matter Physics, Institute of Physics, Chinese Academy of Sciences, Beijing 100080 (China)

Description

We study quench dynamics of the Bose-Hubbard model by exact diagonalization. Initially, the system is at thermal equilibrium and of a finite temperature. The system is then quenched by changing the on-site interaction strength U suddenly. Both the single-quench and double-quench scenarios are considered. In the former case, the time-averaged density matrix and the real-time evolution are investigated. It is found that though the system thermalizes only in a very narrow range of the quenched value of U, it does equilibrate or relax well into a much larger range. Most importantly, it is proven that this is guaranteed for some typical observables in the thermodynamic limit. In order to test whether it is possible to distinguish the unitarily evolving density matrix from the time-averaged (thus time-independent), fully decohered density matrix, a second quench is considered. It turns out that the answer is affirmative or negative depending on whether the intermediate value of U is zero or not.

Additional details

Publishing Information

Journal Title
Physical Review. A
Journal Volume
83
Journal Issue
6
Journal Page Range
p. 063622-063622.10
ISSN
1050-2947
CODEN
PLRAAN

INIS

Country of Publication
United States
Country of Input or Organization
International Atomic Energy Agency (IAEA)
INIS RN
43028274
Subject category
S71: CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS;
Descriptors DEI
DENSITY MATRIX; DYNAMICS; HUBBARD MODEL; INTERACTIONS; QUANTUM MECHANICS; TEMPERATURE DEPENDENCE; THERMAL EQUILIBRIUM; THERMALIZATION; TIME DEPENDENCE
Descriptors DEC
CRYSTAL MODELS; EQUILIBRIUM; MATHEMATICAL MODELS; MATRICES; MECHANICS; SLOWING-DOWN

Optional Information

Notes
(c) 2011 American Institute of Physics