2003
DOI: 10.1103/physreve.68.016610
|View full text |Cite
|
Sign up to set email alerts
|

Stability of screening solitons in photorefractive media

Abstract: Normal mode stability of both rectilinear and self-bending photorefractive screening solitons is considered. In each case, the Evans function procedure is used to investigate stability and to search for internal modes. For the rectilinear case, a standard Evans function procedure is applied. However, in the self-bending case the asymptotic form of the eigenvalue problem is a system of Airy equations, instead of the usual system of constant coefficient differential equations. To overcome this difference, a modi… Show more

Help me understand this report

Search citation statements

Order By: Relevance

Paper Sections

Select...
1
1
1
1

Citation Types

0
22
0
1

Year Published

2008
2008
2016
2016

Publication Types

Select...
7

Relationship

1
6

Authors

Journals

citations
Cited by 28 publications
(23 citation statements)
references
References 17 publications
0
22
0
1
Order By: Relevance
“…However, other physical parameters, such as the gas pressure or the fiber geometry, may change the accelerating pulse profile characteristics imposing or not pulse decay during propagation. The amplitude oscillations, observed in both cases, do not have a constant period but their average period does increase with β 8/3 /η 2 as may be obtained by a simple analysis of the spectral stability problem [8], namely, the oscillation period should be close to the value of the edge of the continuous spectrum and that edge is, in this problem, varying with β 8/3 /η 2 . Returning to the dynamics of the decaying pulses, let us note that since the peak amplitude decreases, the corresponding stationary profile is also varying.…”
Section: Pulse Profilesmentioning
confidence: 96%
“…However, other physical parameters, such as the gas pressure or the fiber geometry, may change the accelerating pulse profile characteristics imposing or not pulse decay during propagation. The amplitude oscillations, observed in both cases, do not have a constant period but their average period does increase with β 8/3 /η 2 as may be obtained by a simple analysis of the spectral stability problem [8], namely, the oscillation period should be close to the value of the edge of the continuous spectrum and that edge is, in this problem, varying with β 8/3 /η 2 . Returning to the dynamics of the decaying pulses, let us note that since the peak amplitude decreases, the corresponding stationary profile is also varying.…”
Section: Pulse Profilesmentioning
confidence: 96%
“…The profile of dark soliton is described by an odd (antisymmetric) function which is easy to show by analysis of the structure of Eq. (27). For a coordinate ξ in the vicinity of ξ = 0, where y(0) = 0, for black solitons, the inequality y ∞ 2 ≫ y 2 holds, so Eq.…”
Section: Solution For the Dark Solitonmentioning
confidence: 98%
“…(7) is not used. Commonly, the assumption is made [1][2][3][4][5][6][18][19][20][21][22][23][24][25][26][27][28][29][30][31][32][33] that similar to diffusion terms, the second term in (6) can be also omitted. Thus, Eq.…”
Section: The Kukhtarev-vinetskii Model and Light-induced Space-chargementioning
confidence: 99%
“…We will solve (1.4.7) in order to investigate the stability of travelling wave solutions. The Evans function has been computed analytically (see for example [FaP03,PW92,SE90,Ter90,HZ06]) and for complicated problems it has been computed numerically (see [MN08,AB01,BDG02,Bri01,HZ06]). …”
Section: Stability Of Travelling Wavesmentioning
confidence: 99%