1993
DOI: 10.1016/0167-2789(93)90184-3
|View full text |Cite
|
Sign up to set email alerts
|

Stability and evolution of the quiescent and travelling solitonic bubbles

Help me understand this report

Search citation statements

Order By: Relevance

Paper Sections

Select...
3
1
1

Citation Types

0
84
0

Year Published

2007
2007
2021
2021

Publication Types

Select...
5
3

Relationship

0
8

Authors

Journals

citations
Cited by 103 publications
(84 citation statements)
references
References 14 publications
0
84
0
Order By: Relevance
“…Also, it should be noted that as in this case the dispersion relation implies that ω > k 2 , the allowable region in the (k, ω) plane for dark solitons is located above the parabola ω = 1 2 k 2 . As the integrals of motion of the NLS equation refer to both the background and the dark soliton, the integrals of motion for the dark soliton are renormalized so as to extract the contribution of the background [112][113][114]. In particular, the renormalized momentum and energy of the dark soliton (27) read (for k = 0):…”
Section: Bright and Dark Matter-wave Solitonsmentioning
confidence: 99%
“…Also, it should be noted that as in this case the dispersion relation implies that ω > k 2 , the allowable region in the (k, ω) plane for dark solitons is located above the parabola ω = 1 2 k 2 . As the integrals of motion of the NLS equation refer to both the background and the dark soliton, the integrals of motion for the dark soliton are renormalized so as to extract the contribution of the background [112][113][114]. In particular, the renormalized momentum and energy of the dark soliton (27) read (for k = 0):…”
Section: Bright and Dark Matter-wave Solitonsmentioning
confidence: 99%
“…In the case of dark solitons of the form u(x,t) = u(x − V t), with |u| 2 → ρ 0 as |x| → ∞, a similar criterion [25][26][27][28] involves the (renormalized) field momentum…”
Section: U + δU = R[u(xt); Xt]mentioning
confidence: 99%
“…In the latter setting, dark solitons typically move along the localized ground state trapped by the external potentials [42]. The main model for BECs is a modification of the NLS equation (1.1) with an external potential, which is called the Gross-Pitaevskii (GP) equation, 2) where ǫ ∈ R is the strength of the potential V (x) and V (x) : R → R is assumed to be a smooth function satisfying one of the three properties:…”
Section: Introductionmentioning
confidence: 99%
“…Among others, several analytical results were important in the development of dark solitons in recent years: perturbation theory based on renormalized power [24] and momentum [23], orbital stability of dark solitons [1,2], completeness of eigenfunctions in the cubic NLS [8,15], inverse scattering for the vector cubic NLS equation [41], construction of the Evans function for dark solitons in the perturbed cubic NLS [19], asymptotic analysis of the radiation and dynamics of dark solitons [26,27,35], and spectral analysis of transverse instabilities of one-dimensional dark solitons [25,36].…”
Section: Introductionmentioning
confidence: 99%