Research
Gravitation, Mathematical Physics and Field Theory
Modulation analysis and optical solitons of perturbed nonlinear
Schrödinger equation
A. Houwea
J. Sabi’ub
G. Betchewea
M. Incc
d
S. Y. Dokae
a Department of Physics, Faculty of Science, the
University of Maroua, P.O Box 814, Maroua, Cameroon.
bDepartment of Mathematics, Faculty of sciences,
Northwest University Kano, P.O.Box 3220, Kano, Nigeria.
c Firat University, Science Faculty, Department
of Mathematics, 23119 Elazig/Turkey. e-mail: minc@firat.edu.tr
d Department of Medical Research, China Medical
University Hospital, China Medical University, Taichung, Taiwan.
e Department of Physics, Faculty of Science, the
University of Ngaoundere, P.O Box 454, Cameroon.
Abstract
We investigate modulation analysis and optical solitons of perturbed nonlinear
Schrödinger equation (PNLSE). The PNLSE has terms of cubic nonlinearity and
self-steepening and spatio-temporal dispersion (STD). Proposed model has been
studied by [14, 15] without selfsteepening term. The presence of the STD can
help to compensate the low GVD to the model. Bright and dark solitary waves,
trigonometric, periodic and singular optical solitons are obtained by some
expansion methods including exponential and sinh-Gordon. Obtained results will
hold a significant place in the field of nonlinear optical fibers, where
solitons are used to codify data.
Keywords: Optical soliton; perturbed nonlinear Schrödinger equation; instability modulation
PACS: 04.20.Jb; 05.45.Yv; 94.05.Fg
1. Introduction
Research on exact solutions of nonlinear systems has reached cruising speed these
days. The best known solitons solutions have found their applications in several
research areas including optical fibers, plasm, biology, and quantum physics, just
to name a few. Thus, optical solitons did not remain anonymous for a long time
because of their direct implications in trans-continental and trans-oceanic data
transport [1-10]. It is important to remember that thanks to the advent of optical
solitons, the field of communication has experienced an expansion through high speed
data transfer, and guaranteed protection. Thereafter, many theoretical and
experimental results have been followed with the mathematical tools to handle them.
In this way, exact optical solitons resulting from the nonlinear Schrodinger
equations with different¨ nonlinearities have been reported [10-13]. Some of the
analytical methods that facilitated the success of these results are expansion
methods including modified exp(−ψ(ξ)) function,
(G’/G), trial-error, auxiliary equation,
rational function, Riccati-Bernoulli sub-ODE , the sine-Gordon expansion,
exp(−(((ξ))-expansion, see [2-23].
The present work, aims to unearth exact optical solitons to PNLSE [14,15]:
iψt+a1ψxt+a2ψxx+a3|ψ|2ψ-iβ(|ψ|2ψ)x=0,
(1)
ψ(x,t) is complex wave profile, t
represents temporal variable and x is spatial variable. α
1 is the STD, α2 the coefficient of group velocity
dispersion (GVD), while α 3 is the cubic nonlinearity which will be
combined with the dispersion terms in order to build optical solitons. However,
β is the self-steepening coefficient.
Section 2 concern the traveling-wave solution to transform the PNLSE into to
integrable form of nonlinear ordinary differential equation. In Secs. 3 and 4, we
apply two integration schemes to look optical solitons and we establish also the
existence criteria of the obtained results. In Sec. 5 we discussed the modulation
instability of of the obtained results. The last part of the paper is devoted to
conclusion. To determine optical solitons to Eq. (1), we will use sinh-Gordon and
exp(−Φ(ξ))-expansion techniques with the traveling-wave
hypothesis.
1.1. Traveling waves solution
It is used the following transformation to (1) to build soliton solution
ψ(x,t)=ϕ(ξ)exp[iθx,t],ξ=x-vt,
(2)
where ϕ represents the shape of the soliton and depends on the Kerr
non-linearity. However the phase θ(x,t) is
given by
θ(x,t)=-κx+ωt+θ0,
(3)
Inserting (2) and used (3) into (1) it is obtained the speed of the soliton from
the imaginary part
v=a1(2κ-ω)1-a1κ,1≠a1κ.
(4)
with the constrains relation on the self-steepening parameters.
β=0.
(5)
Here, we omit the SPM term to preserve the obtained bright and dark optical
solitons against deformation of the waveform, sensitivity deterioration of the
receiver and the transmission limits distance cause by the latter in dispersion
optic fibers. Recently, it has been demonstrated numerically that a waveform
distortion is caused by the SPM in nonlinear Schrödinger equation in the
transmission fiber [15,18].
(-ω+a1κω+a2κ2)ϕ+(a12(2κ-ω)1-a1κ+a2)ϕξξ+a3ϕ3=0,
(6)
where ϕξξ =
∂2ϕ/∂ξ2.
Now, multiplying Eq. (6) by ϕξ and integrating once
gives
(a12(2κ-ω)1-a1κ+a2)ϕξ2-(ω-a1κω-a2κ2)ϕ2+a32ϕ4=0,
(7)
Then, after separating variables and integrating with zero constant it is
obtained
x-vt=∫dϕϕω-a1κω-a2κ2-a32ϕ2,
(8)
Consequently,
ϕ(x,t)=Acosh[Bx-vt],
(9)
in which
A=±a32,
(10)
B=±a12κ-ω1-a1κ,
(11)
and the corresponding chirp-free bright soliton
ψ1(x,t)=AcoshBx-vt×exp[i-κx+ωt+θ0],
(12)
Then, the constraint relation from the obtained Eq. (10) and Eq. (11) implies
(1-a1κ)(2κ-ω)>0,
(13)
and
a3>0,
(14)
We note that, in the absence of self-pentification (β = 0), the
asymmetry in the form of a pulse is also absent, which implicitly recognizes the
formation of shock waves. Here this absence could also affect the pulse width of
the solitons obtained. However, the presence of GVD and cubic nonlinearity
reinforces the search for optical solitons which will be at least robust against
the formation of shocks. In addition, we also point out that the ODE (7) can be
directly integrated, but to obtain specific optical solutions, we choose to do
so through two integration techniques.
2. Sinh-Gordon expansion method
Following expression is adopted as in [19-21], the detail of the method
can be obtained in [19]. By principle of
balance from (6) between ϕ
ξξ
and ϕ 3, N = 1.
ϕ(ξ)=ϕ(w(ξ))=A0+A1sinhw(ξ)+B1coshw(ξ),
(15)
and α0, α1 and B1 are parameters to
be determined.
To build some special Jacobian elliptic function solution, we used the following
expression
sinhwξ=csξ;m,
(16)
cosh[wξ]=ns(ξ;m),
(17)
m represents modulus of Jacobian functions [19-21]. Now,
substituting Eq. (15) along with others derivatives into Eq. (6) and taking into
consideration (16a-16b), it is recovered after some computations:
• cosh3(w(ξ)):
3a3A12B1+a3B13-2a12ωB11-a1κ+2a2B1+4a12κB11-a1κ=0,
(18)
• cosh2(w(ξ)):
3a3A0B12+3a3A0A12=0,
(19)
•
sinh(w(ξ))cosh2(w(ξ)):
a3A13-2a12ωA11-a1κ+2a2A1+3a3A1B12+4a12κA11-a1κ=0,
(20)
• cosh(w(ξ)):
a1κωB1+a2B1c-4a12κB11-a1κ-3a3A12B1-a12ωB1c1-a1κ-ωB1-2a2B1+2a12ωB11-a1κ+3a3A02B1+2a12κB1c1-a1κ+a2κ2B1=0,
(21)
•
sinh(w(ξ))cosh(w(ξ)):
6a3A0A1B1=0,
(22)
• Constant:
a2κ2A0-3a3A0A12+a1κωA0+a3A03-ωA0=0,
(23)
• sinh(w(ξ)):
-ωA1-a3A13+a1κωA1+2a12κA1c1-a1κ+a12ωA11-a1κ-a12ωA1c1-a1κ-2a12κA11-a1κ+3a3A02A1-a2A1+a2A1c+a2κ2A1=0,
(24)
With help of Maple 14, we solve Eqs. (17-23), and it is recovered the following
solution families
• Family 1:
A0=0,A1=0,B1=B1,
ω=--κ2a3B12+2a3B12-ca3B12-4a12κ3+a1κ3a3B12-2a3B12a1κ+a1ca3B12κ2(2a1κ-1).
(25)
• Family 2:
A0=0,A1=A1,B1=0,
ω=--κ2a3A12-a3A12-ca3A12-4a12κ3+a1κ3a3A12+a3A12a1κ+a1ca3A12κ2(2a1κ-1).
(26)
• Family 3:
A0=0,A1=B1,B1=B1,
ω=--2κ2a3B12+a3B12-2ca3B12-2a12κ3-a3B12a1κ+2a1κ3a3B12+2a1ca3B12κ2a1κ-1.
(27)
• Family 4:
A0=0,A1=-B1,B1=B1,
ω=--2κ2a3B12+a3B12-2ca3B12-2a12κ3-a3B12a1κ+2a1κ3a3B12+2a1ca3B12κ2a1κ-1.
(28)
2.1. Jacobian elliptic function solutions
From family 1, it is obtained the following Jacobian elliptic function
solutions
ψ11(x,t)=B1ns(ξ,m)×expi[-κx+ωt+θ0].
(29)
From family 2, we recovered
ψ12(x,t)=A1cs(ξ,m)×exp(i[-κx+ωt+θ0]).
(30)
From family 3, it is gained the combined Jacobian elliptic function solutions
ψ13(x,t)=B1{cs(ξ,m)+ns(ξ,m)}exp(i[-κx+ωt+θ0]).
(31)
Then, from family 4 it is acquired the combined Jacobian elliptic function
solutions
ψ14(x,t)=B1{-cs(ξ,m)+ns(ξ,m)}exp(i[-κx+ωt+θ0]).
(32)
2.2. Trigonometric and singular solutions
From family 1, when m → 1,it is obtained
ψ15(x,t)=B1coth(x-a12κ-ω1-a1κt)exp(i[-κx+ωt+θ0]).
(33)
Then from family 2, when m → 1, it is recovered singular optical
solutions
ψ16(x,t)=A1cschx-a12κ-ω1-a1κtexp(i[-κx+ωt+θ0]).
(34)
To family 3 and 4, the combined optical solutions is obtained, when
m → 1.
ψ17(x,t)=B1cschx-a12κ-ω1-a1κt+cothx-a12κ-ω1-a1κtexp(i[-κx+ωt+θ0]).
(35)
and
ψ18(x,t)=B1-cschx-a12κ-ω1-a1κt+cothx-a12κ-ω1-a1κtexp(i[-κx+ωt+θ0]).
(36)
2.3. Periodic and singular solutions
When m → 0, it is recovered periodic and singular solutions to
(1) From family 1, it is obtained
ψ19(x,t)=B1cscx-a1[2κ-ω]1-a1κtexpi[-κx+ωt+θ0].
(37)
From family 2, we recovered
ψ20(x,t)=A1cotx-a12κ-ω1-a1κtexp(i[-κx+ωt+θ0]).
(38)
From family 3, it is gained the combined solutions
ψ21(x,t)=B1cotx-a12κ-ω1-a1κt+cscx-a12κ-ω1-a1κtexp(i[-κx+ωt+θ0]).
(39)
Then, from family 4 it is acquired the combined optical solutions
ψ22(x,t)=B1-cotx-a12κ-ω1-a1κt+cscx-a1[2κ-ω]1-a1κtexp(i[-κx+ωt+θ0]).
(40)
3. exp(−Φ(ξ))-expansion method
Let
ϕ(x,t)=∑i=0NAi(exp(-Φ(ξ)))i,
(41)
in which αi are unknown parameters, while
Φ(ξ) satisfies [22,23] the ODE:
Φ'(ξ)=exp(-Φ(ξ))+μexp(Φ(ξ))+λ,
(42)
Using homogeneous principle of balance between ϕξξ and
ϕ3 in (6), it is obtained N = 1. Hence,
ϕ(x,t)=A0+A1(exp(-Φ(ξ))),
(43)
Substituting Eqs. (41) and (42) into (6) leads to a polynomial in
(exp(−Φ(ξ))). By MAPLE software and letting coefficients of
(exp(−Φ(ξ))) to 0:
• Set 1: A0=A0,A1=A1,κ=1a1,ω=2a1
• Set 2:
A0=λ2a13κ2-2a12κ+2a2a1κ-a2a3(2a12κ2-a12λ2+4a12μ-4a1κ+2),A1=2(2a13κ2-2a12κ+2a2a1κ-a2a3(2a12κ2-a12λ2+4a12μ-4a1κ+2)),
ω=2a2κ2-a2λ2+4a2μ-2a2κ3a1+a2λ2a1κ-4a2μa1κ-2a12κλ2+8a12κμ2a12κ2-a12λ2+4a12μ-4a1κ+2,κ=κ.
From set 1, it is obtained five families of solutions: (1.1) If
λ2 − 4µ > 0, and
µ 6= 0, it is acquired
ψ21,1(x,t)=A0+2A1μ--4μ+λ2tanh[12-8μ+2λ2x-a12κ-ω1-a1κt+ξ0]-λexpi-κx+2a1t+θ0,
(44)
(1.2) If λ2 − 4µ < 0, and
µ 6= 0, it is obtained
ψ21,2(x,t)=A0+2A1μ-4μ+λ2tanh[12-8μ+2λ2x-a12κ-ω1-a1κt+ξ0]-λexpi-κx+2a1t+θ0,
(45)
(1.3) If λ2 − 4µ < 0, and
µ0 and λ 6= 0, it is gained
ψ21,3(x,t)=(A0+2A1λcoshλx-a1(2κ-ω)1-a1κt+ξ0+sinhλx-a1(2κ-ω)1-a1κt+ξ0-1)×expi-κx+2a1t+θ0,
(46)
(1.4) If λ2 − 4µ = 0, and
µ 6= 0 and λ 6= 0, it is gained
ψ21,4(x,t)=(A0+2A1λ2x-a1(2κ-ω)1-a1κt+ξ0-2λx-a1(2κ-ω)1-a1κt+ξ0+2)expi-κx+2a1t+θ0,
(47)
(1.5) If λ2 − 4µ = 0, and
µ = 0 and λ = 0, we have
ψ21,5(x,t)=(A0+A1x-a1(2κ-ω)1-a1κt+ξ0)expi-κx+2a1t+θ0,
(48)
From set 2, it is obtained five general solutions as follows
(2.1) If λ2 − 4µ > 0, and
µ 6= 0, it is acquired
ψ21,6(x,t)=λ2a13κ2-2a12κ+2a2a1κ-a2a3(2a12κ2-a12λ2+4a12μ-4a1κ+2)+2A1μ--4μ+λ2tanh12-8μ+2λ2x-a1(2κ-ω)1-a1κt+ξ0-λexpi-κx+ωt+θ0,
(49)
(2.2) If λ2 − 4µ < 0, and
µ 6= 0, it is obtained
ψ21,7(x,t)=λ2a13κ2-2a12κ+2a2a1κ-a2a3(2a12κ2-a12λ2+4a12μ-4a1κ+2)+2A1μ4μ-λ2tan12-8μ+2λ2x-a1(2κ-ω)1-a1κt+ξ0-λexpi[-κx+ωt+θ0],
(50)
(2.3) If λ2 − 4µ < 0, and
µ0 and λ 6= 0, it is gained
ψ21,8(x,t)=λ2a13κ2-2a12κ+2a2a1κ-a2a3(2a12κ2-a12λ2+4a12μ-4a1κ+2)+2A1λcoshλx-a1(2κ-ω)1-a1κtξ0+sinhλx-a1(2κ-ω)1-a1κt+ξ0-1expi[-κx+ωt+θ0],
(51)
(2.4) If λ2 − 4µ = 0, and
µ 6= 0 and λ 6= 0, it is gained
ψ21,9(x,t)=(λ2a13κ2-2a12κ+2a2a1κ-a2a3[2a12κ2-a12λ2+4a12μ-4a1κ+2]+2A1λ2x-a1(2κ-ω)1-a1κt+ξ0-2λx-a1(2κ-ω)1-a1κt+ξ0+2)×expi[-κx+ωt+θ0],
(52)
(2.5) If λ2 − 4µ = 0, and
µ = 0 and λ = 0, we have
ψ21,10(x,t)=(λ2a13κ2-2a12κ+2a2a1κ-a2a3(2a12κ2-a12λ2+4a12μ-4a1κ+2)+A1x-a1(2κ-ω)1-a1κt+ξ0)×expi[-κx+ωt+θ0],
(53)
Where ξ0 is a constant of integration.
4. Modulation analysis
This section of the paper will address the modulation analysis of the unstable
solutions. It is well established that bright and dark solitons are stable; thus, it
is necessary to verify the regime of the instability of the rest of solutions. On
this fact, it will be used the following solutions of Eq. (1).
ψx,t=[P0+Ax,t]eiϕNL,ϕNL=P0x,
(54)
while P0 is the incident power. To seek the perturbation,
we use Eq. (53) into Eq. (1)
iAt(x,t)+a1Axt(x,t)+a2Axx+a3P0A(x,t)+a3P0(A(x,t)+A*(x,t))-iβP0Ax(x,t)-iβP0(Ax(x,t)+Ax*(x,t))=0,
(55)
Hence, Eq. (54) maybe solved in the frequency domain. To do so, it will be considered
form of α(x,t) as:
A(x,t)=b1⋅ei(Kx-Ωt)+b2⋅e-i(Kx-Ωt).
(56)
Inserting Eq. (55) into Eq. (54) gives the coefficient matrix of
b1 and b2,
Ω+2a3P0+a1KΩ-a2K2+2βP0KβP0K+a3P0-βP0K+a3P0a1KΩ-Ω-2βP0K+2a3P0-a2K2b1b200.
(57)
The dispersion relation is obtained when a solution of Eq. (56) exists. Spreading out
determinant leads to
-4ΩβP0K-4a3P0a2K2-2a1K3Ωa2-3β2P02K2-Ω2+3a32P02+a22K4+4a3P0a1KΩ+a12K2Ω2=0.
(58)
For α21K2 6= 1, it
is appear the modulation instability (MI) ,
(-2a3P0a1K+2βP0K+a1K3a2+a32P02a12K2-8a3P02a1K2β+β2P02K2+4βP0K4a1a2+3a12K4β2P02+3a32P02+a22K4-4a3P0a2K2)<0,
(59)
and the gain spectrum G(K) =
2Im(Ω) and it is revealed
G(K)=2(1a12K2-1)(-2a3P0a1K+2βP0K+a1K3a2+a32P02a12K2-8a3P02a1K2β+β2P02K2+4βP0K4a1a2+3a12K4β2P02+3a32P02+a22K4-4a3P0a2K2).
(60)
Figures 1 and 2 plot the analytical 2D and 3D free-chirp bright solutions for
|ψ
1| at at α1 = 1, α3 =
1.14,ω = 0.324,
κ = 0.2,v = 0.25. We
note that when the self-steepening is absent (β = 0), it is
obtained bright and dark optical solitons with normal-GVD without any deformation of
waveform. However, Kerr nonlinearity, STD and low GVD lead to dark solitons to the
proposed model of NLSE. In addition, the obtained bright solitons depend on the GVD,
STD, and Kerr nonlinearity parameters. Also, it is observed that the (MI) gain
spectrum depends on the STD, Kerr nonlinearity and self-steepening parameters; Figures 3a) and 3b) stress the (MI) gain spectrum
with the effect of self-steepening. More and more the presence of SPM in the MI gain
instability will accentuate the instability zone and the MI gain will grow
exponentially. The formation of soliton due the fighting between nonlinear and
dispersion terms of the nonlinear Schrödinger equation will be impacted during the
propagation in long distance because of the act of SPM and the signal received will
be highly perturbed.
5. Conclusion
This work studies modulation analysis and optical solitons of PNLSE having STD,
perturbation and some nonlinearity terms. We employ the sinh-Gordon technique and
exp(−Φ(ξ))-technique to handle the obtained ordinary
differential equation (ODE). Obtained results are bright and dark optical solitons
and trigonometric functions. Compare our findings with some previous works [14,15],
some additional are obtained by adopting the famous
exp(−Φ(ξ))-expansion method. In addition, the STD and the cubic
nonlinearity terms have contributed to generation og bright and dark solitons. Thus,
in order to verify the instability regime, we used the modulation instability (MI),
to establish the gain spectrum. From there, two areas emerge, where one is stable
and the second unstable. The model will take into account modulations of self-phase
and cross-phase in a future work.
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