Dark solitons interaction for a (2+1)-dimensional nonlinear Schrodinger equation in the Heisenberg ferromagnetic spin chain

被引:52
作者
Zhao, Xue-Hui [1 ]
Tian, Bo [1 ]
Liu, De-Yin [1 ]
Wu, Xiao-Yu [1 ]
Chai, Jun [1 ]
Guo, Yong-Jiang [1 ]
机构
[1] Beijing Univ Posts & Telecommun, Sch Sci, State Key Lab Informat Photon & Opt Commun, Beijing 100876, Peoples R China
基金
中国国家自然科学基金;
关键词
Heisenberg ferromagnetic spin chain; (2+1)-dimensional nonlinear Schrodinger equation; Hirota method; Dark solitons interaction; Linear stability analysis; MAGNETIC COMPOSITE-MATERIAL; BACKLUND TRANSFORMATION; CONSERVATION-LAWS; ROGUE WAVES; LAX PAIR; SYSTEM;
D O I
10.1016/j.spmi.2016.10.014
中图分类号
O469 [凝聚态物理学];
学科分类号
070205 ;
摘要
Under investigation in this paper is a (2 + 1)-dimensional nonlinear Schrodinger equation in the Heisenberg ferromagnetic spin chain. Via the symbolic computation and Hirota method, the bilinear forms, dark one-, two- and three-soliton solutions are derived. Propagation and interaction for the dark solitons are illustrated graphically: Amplitude and shape of the dark one soliton keep invariant during the propagation, which imply the transport of the energy is stable in the (2 + 1)-dimensional Heisenberg ferromagnetic spin chain. Through the asymptotic analysis, elastic and inelastic interactions between the dark two solitons are discussed. For the elastic interaction, oblique, head-on and overtaking interactions between the dark two solitons are displayed, where the amplitudes and shapes remain unchanged after interaction except for certain phase shifts. However, in the area of the inelastic interaction, amplitudes of the dark two solitons vanish after interaction. For the elastic interaction among the dark three solitons, oblique, overtaking and interaction among the dark two parallel solitons and a single one are presented, whose characteristics are similar to those of the dark two solitons. Inelastic-elastic interaction is investigated as well. Linear stability analysis is used to analyze modulation instability and prove the dark solitons are stable. (C) 2016 Elsevier Ltd. All rights reserved.
引用
收藏
页码:587 / 595
页数:9
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