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Quantum many-body dynamics of dark solitons in optical lattices

Source: Phys. Rev. A 80, 053612 (2009); doi:10.1103/PhysRevA.80.053612

Published 13 November 2009

KEYWORDS and PACS
Keywords
PACS
  • 03.75.Gg
    Entanglement and decoherence in Bose-Einstein condensates
  • 03.75.Lm
    Tunneling, Josephson effect, Bose-Einstein condensates in periodic potentials, solitons, vortices and topological excitations
  • 05.45.Yv
    Solitons
  • YEAR: 2009
PUBLICATION DATA
Publisher:
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R. V. Mishmash,1,2,3 I. Danshita,3,4,5 Charles W. Clark,3 and L. D. Carr2,3
1Department of Physics, University of California, Santa Barbara, California 93106, USA
2Department of Physics, Colorado School of Mines, Golden, Colorado 80401, USA
3Joint Quantum Institute, National Institute of Standards and Technology, Gaithersburg, Maryland 20899, USA
4Department of Physics, Boston University, Boston, Massachusetts 02215, USA
5Department of Physics, Faculty of Science, Tokyo University of Science, Shinjuku-ku, Tokyo 162-8601, Japan

We present a fully quantum many-body treatment of dark solitons formed by ultracold bosonic atoms in one-dimensional optical lattices. Using time-evolving block decimation to simulate the single-band Bose-Hubbard Hamiltonian, we consider the quantum dynamics of density and phase engineered dark solitons as well as the quantum evolution of mean-field dark solitons injected into the quantum model. The former approach directly models how one may create quantum entangled dark solitons in experiment. While we have already presented results regarding the latter approach elsewhere [R. V. Mishmash and L. D. Carr, Phys. Rev. Lett. 103, 140403 (2009)], we expand upon those results in this work. In both cases, quantum fluctuations cause the dark soliton to fill in and may induce an inelasticity in soliton-soliton collisions. Comparisons are made to the Bogoliubov theory which predicts depletion into an anomalous mode that fills in the soliton. Our many-body treatment allows us to go beyond the Bogoliubov approximation and calculate explicitly the dynamics of the system's natural orbitals. ©2009 The American Physical Society
History: Received 26 June 2009; published 13 November 2009
Permalink: http://link.aps.org/abstract/PRA/v80/e053612
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