Analytical and numerical aspects of certain nonlinear evolution equations. II. Numerical, nonlinear Schrödinger equation

1984 ◽  
Vol 55 (2) ◽  
pp. 203-230 ◽  
Author(s):  
Thiab R Taha ◽  
Mark I Ablowitz
2017 ◽  
Vol 5 (1) ◽  
pp. 17
Author(s):  
Salam Subhaschandra Singh

In this paper, using the methods of ansatz, sine-cosine and He’s semi-inverse variation, non-topological 1-soliton solution to Resonant Nonlinear Schrodinger Equation with Kerr law nonlinearity is obtained. The results show that these methods are very effective ones for finding exact solutions to various types of nonlinear evolution equations appearing in the studies of science and engineering.


2018 ◽  
Vol 32 (33) ◽  
pp. 1850407 ◽  
Author(s):  
E. Tala-Tebue ◽  
Aly R. Seadawy

The resonant nonlinear Schrödinger equation is studied in this work with the aid of two methods, namely the exponential rational function method and the modified exponential function method. This equation is used to describe the propagation of optical pulses in nonlinear optical fibers. Being concise and straightforward, these methods are used to build new exact analytical solutions of the model. The solutions obtained are not yet reported in the literature. The methods proposed can be extended to other types of nonlinear evolution equations in mathematical physics.


1985 ◽  
Vol 63 (5) ◽  
pp. 632-641 ◽  
Author(s):  
R. H. Enns ◽  
S. S. Rangnekar

The sine-Gordon, sinh-Gordon, modified Korteweg-deVries (KdV), and nonlinear (cubic) Schrödinger equations are four of the most important (from a physical point of view) nonlinear evolution equations that fit into the Ablowitz–Kaup–Newell–Segur (AKNS) inverse scattering framework. Historically, the soliton solutions of these equations have been exhaustively studied in the literature, the radiation solutions being almost entirely neglected. Using an expansion approach (expanding the reflection coefficient in powers of the area A of the input potential), we have previously studied the complete spatial and temporal evolution of the radiation solutions of the first three equations cited above. In this paper we demonstrate, using an illustrative example, that the expansion approach also works for the nonlinear Schrödinger equation. The qualitative features of the radiation solution thus obtained are easily understood in the physical context of the self-defocusing of an intense optical beam. Making use of numerical simulation, we show that the features persist as A is increased to very large values. The solution is also found to be analytically consistent with the asymptotic (t → ∞) form quoted in the literature for a general input profile.


2021 ◽  
pp. 2150470
Author(s):  
Md. Tarikul Islam ◽  
Md. Ali Akbar ◽  
Ozkan Guner ◽  
Ahmet Bekir

Nonlinear evolution equations of arbitrary order bearing a significantly broad range of capability to illustrate the underlying behavior of naturalistic structures relating to the real world, have become a major source of attraction of scientists and scholars. In quantum mechanics, the nonlinear dynamical system is most reasonably modeled through the Schrödinger-type partial differential equations. In this paper, we discuss the (2+1)-dimensional time-fractional nonlinear Schrödinger equation and the (1+1)-dimensional space–time fractional nonlinear Schrödinger equation for appropriate solutions by means of the recommended enhanced rational [Formula: see text]-expansion technique adopting Cole–Hopf transformation and Riccati equation. The considered equations are turned into ordinary differential equations by implementing a composite wave variable replacement alongside the conformable fractional derivative. Then a successful execution of the proposed method has been made, which brought out supplementary innovative outcomes of the considered equations compared with the existing results found so far. The well-generated solutions are presented graphically in 3D views for numerous wave structures. The high performance of the employed technique shows the acceptability which might provide a new guideline for research hereafter.


2021 ◽  
Vol 39 (2) ◽  
pp. 121-131
Author(s):  
Ahmad Neirameh ◽  
Mostafa Eslami ◽  
Mostafa Mehdipoor

New definitions for traveling wave transformation and using of new conformable fractional derivative for converting fractional nonlinear evolution equations into the ordinary differential equations are presented in this study. For this aim we consider the time and space fractional derivatives cubic nonlinear Schrodinger equation. Then by using of the efficient and powerful method the exact traveling wave solutions of this equation are obtained. The new definition introduces a promising tool for solving many space-time fractional partial differential equations.


2010 ◽  
Vol 07 (06) ◽  
pp. 1043-1049 ◽  
Author(s):  
GOPAL MUNIRAJA ◽  
M. LAKSHMANAN

We consider the dynamics of moving curves in three-dimensional Minkowski space [Formula: see text] and deduce the evolution equations for the curvature and torsion of the curve. Next by mapping a continuous SO(2,1) Heisenberg spin chain on the space curve in [Formula: see text], we show that the defocusing nonlinear Schrödinger equation(NLSE) can be identified with the spin chain, thereby giving a geometrical interpretation of it. The associated linear eigenvalue problem is also obtained in a geometrical way.


2009 ◽  
Vol 64 (11) ◽  
pp. 691-696 ◽  
Author(s):  
Sheng Zhang ◽  
Jin-Mei Ba ◽  
Ying-Na Sun ◽  
Ling Dong

In this paper, a generalized (G'/G)-expansion method, combined with suitable transformations, is used to construct exact solutions of the nonlinear Schrödinger equation with variable coefficients. As a result, hyperbolic function solutions, trigonometric function solutions, and rational solutions with parameters are obtained. When the parameters are taken as special values, some solutions including the known kink-type solitary wave solution and the singular travelling wave solution are derived from these obtained solutions. It is shown that the generalized (G'/G)-expansion method is direct, effective, and can be used for many other nonlinear evolution equations with variable coefficients in mathematical physics.


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