corner
corner

Phys. Rev. A 72, 033611 (2005) [11 pages]

Exact soliton solutions and nonlinear modulation instability in spinor Bose-Einstein condensates

Download: PDF (215 kB) Buy this article Export: BibTeX or EndNote (RIS)

Lu Li1,2, Zaidong Li1, Boris A. Malomed3, Dumitru Mihalache4, and W. M. Liu2
1College of Physics and Electronics Engineering, Shanxi University, Taiyuan, 030006, China
2Joint Laboratory of Advanced Technology in Measurements, Beijing National Laboratory for Condensed Matter Physics, Institute of Physics, Chinese Academy of Sciences, Beijing 100080, China
3Department of Interdisciplinary Studies, Faculty of Engineering, Tel Aviv University, Tel Aviv 69978, Israel
4National Institute of Physics and Nuclear Engineering, Institute of Atomic Physics, Department of Theoretical Physics, P.O. Box MG-6, Bucharest, Romania

Received 11 July 2005; published 14 September 2005

We find one-, two-, and three-component solitons of the polar and ferromagnetic (FM) types in the general (nonintegrable) model of a spinor (three-component) model of the Bose-Einstein condensate, based on a system of three nonlinearly coupled Gross-Pitaevskii equations. The stability of the solitons is studied by means of direct simulations and, in a part, analytically, using linearized equations for small perturbations. Global stability of the solitons is considered by means of an energy comparison. As a result, ground-state and metastable soliton states of the FM and polar types are identified. For the special integrable version of the model, we develop the Darboux transformation (DT). As an application of the DT, analytical solutions are obtained that display full nonlinear evolution of the modulational instability of a continuous-wave state seeded by a small spatially periodic perturbation. Additionally, by dint of direct simulations, we demonstrate that solitons of both the polar and FM types, found in the integrable system, are structurally stable; i.e., they are robust under random changes of the relevant nonlinear coefficient in time.

© 2005 The American Physical Society

URL:
http://link.aps.org/doi/10.1103/PhysRevA.72.033611
DOI:
10.1103/PhysRevA.72.033611
PACS:
03.75.Mn, 05.45.Yv, 04.20.Jb