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Phys. Rev. A 81, 063604 (2010) [15 pages]

Multiple atomic dark solitons in cigar-shaped Bose-Einstein condensates

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G. Theocharis1, A. Weller2, J. P. Ronzheimer2, C. Gross2, M. K. Oberthaler2, P. G. Kevrekidis1, and D. J. Frantzeskakis3
1Department of Mathematics and Statistics, University of Massachusetts, Amherst, MA 01003-4515, USA
2Kirchhoff Institut für Physik, INF 227, Universität Heidelberg, D-69120 Heidelberg, Germany
3Department of Physics, University of Athens, Panepistimiopolis, Zografos, Athens GR-15784, Greece

Received 8 September 2009; revised 16 March 2010; published 3 June 2010

We consider the stability and dynamics of multiple dark solitons in cigar-shaped Bose-Einstein condensates. Our study is motivated by the fact that multiple matter-wave dark solitons may naturally form in such settings as per our recent work [ Phys. Rev. Lett. 101 130401 (2008)]. First, we study the dark soliton interactions and show that the dynamics of well-separated solitons (i.e., ones that undergo a collision with relatively low velocities) can be analyzed by means of particle-like equations of motion. The latter take into regard the repulsion between solitons (via an effective repulsive potential) and the confinement and dimensionality of the system (via an effective parabolic trap for each soliton). Next, based on the fact that stationary, well-separated dark multisoliton states emerge as a nonlinear continuation of the appropriate excited eigenstates of the quantum harmonic oscillator, we use a Bogoliubov-de Gennes analysis to systematically study the stability of such structures. We find that for a sufficiently large number of atoms, multiple soliton states are dynamically stable, while for a small number of atoms, we predict a dynamical instability emerging from resonance effects between the eigenfrequencies of the soliton modes and the intrinsic excitation frequencies of the condensate. Finally, we present experimental realizations of multisoliton states including a three-soliton state consisting of two solitons oscillating around a stationary one and compare the relevant results to the predictions of the theoretical mean-field model.

© 2010 The American Physical Society

URL:
http://link.aps.org/doi/10.1103/PhysRevA.81.063604
DOI:
10.1103/PhysRevA.81.063604
PACS:
03.75.Lm, 05.45.Yv