Journal Pre-proof A (3 + 1)-dimensional resonant nonlinear Schr¨odinger equation and its Jacobi elliptic and exponential function solutions K. Hosseini, M. Matinfar, M. Mirzazadeh
PII:
S0030-4026(20)30292-8
DOI:
https://doi.org/10.1016/j.ijleo.2020.164458
Reference:
IJLEO 164458
To appear in:
Optik
Received Date:
13 February 2020
Accepted Date:
21 February 2020
Please cite this article as: Hosseini K, Matinfar M, Mirzazadeh M, A (3 + 1)-dimensional resonant nonlinear Schr¨odinger equation and its Jacobi elliptic and exponential function solutions, Optik (2020), doi: https://doi.org/10.1016/j.ijleo.2020.164458
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A (3+1)-dimensional resonant nonlinear Schrödinger equation and its Jacobi elliptic and exponential function solutions
K. Hosseini1*, M. Matinfar1, M. Mirzazadeh2*
Department of Mathematics, Faculty of Mathematical Sciences, University of Mazandaran, Babolsar, Iran 2 Department of Engineering Sciences, Faculty of Technology and Engineering, East of Guilan, University of Guilan, P.C. 44891-63157 Rudsar-Vajargah, Iran
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*Corresponding Authors:
[email protected],
[email protected]
Abstract
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The current study is concerned with a (3+1)-dimensional resonant nonlinear Schrödinger (3D-RNLS) equation with diverse applications in nonlinear optics and its exact solutions. In this regard, by
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adopting the new expansion methods based on the Jacobi elliptic equation, a number of exact solutions in terms of Jacobi elliptic and exponential functions to the 3D-RNLS equation with Kerr law nonlinearity are formally constructed. The outcomes of this paper undoubtedly demonstrate the
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impressive capability of the new expansion methods to deal with nonlinear Schrödinger equations. Keywords: (3+1)-dimensional resonant nonlinear Schrödinger equation; Kerr law nonlinearity; New
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expansion methods; Jacobi elliptic and exponential function solutions
1. Introduction
It is known that nonlinear Schrödinger equations are of a key role in the vast areas of scientific
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disciplines, particularly nonlinear optics. Although, the physical features of this class of nonlinear PDEs can be investigated by extracting and studying its exact solutions, searching such solutions is not easy. Today with the availability of symbolic computation packages, many effective methods [138] have been applied to overcome the difficulties in looking for exact solutions of nonlinear PDEs. In this article, we mainly focus on a (3+1)-dimensional resonant nonlinear Schrödinger equation with Kerr law nonlinearity as [1, 2] 𝑖𝑢𝑡 + 𝜂𝛻 2 𝑢 + 𝜎|𝑢|2 𝑢 + 𝛿 {
𝛻2 |𝑢| } |𝑢|
𝑢 = 0,
𝑢 = 𝑢(𝑥, 𝑦, 𝑧, 𝑡),
1
𝛻2 =
𝜕2 𝜕𝑥 2
+
𝜕2 𝜕𝑦 2
+
𝜕2 𝜕𝑧 2
,
(1)
and extract its exact solutions by adopting the new expansion methods based on the Jacobi elliptic equation [33-38]. In the above equation, the non-zero constants 𝜂, 𝜎, and 𝛿 are the coefficients of the group velocity, cubic nonlinearity, and resonant nonlinearity. Several scholars have dedicated their investigations for seeking exact solutions of the (3+1)-dimensional resonant nonlinear Schrödinger equation. For example, Sedeeg et al. [1] exerted the tanh method to retrieve generalized optical solitons of the 3D-RNLS equation and Ferdous et al. [2] obtained oblique resonant optical solitons of the 3D-RNLS equation by employing the generalized exp(−𝛷(𝜉))-expansion method. It is worth noting that the resonant nonlinear Schrödinger equations at lower dimensions have been investigated by a series of systematic methods; the interested reader is referred to see [3-15]. The organization of this paper is as follows: In Section 2, the reduced form of the 3D-RNLS equation with Kerr law
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nonlinearity is derived. In Section 3, the exact solutions of the 3D-RNLS equation are constructed by considering the new expansion methods based upon the Jacobi elliptic equation. The concluding remarks are presented in the last section.
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2. The reduced form of the 3D-RNLS equation
In order to arrive at the reduced form of the 3D-RNLS equation with Kerr law nonlinearity, we apply
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a complex transformation as follows
𝜖 = cos(𝛼)𝑥 + cos(𝛽)𝑦 + cos(𝛾)𝑧 + 𝑐𝑡.
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𝑢(𝑥, 𝑦, 𝑧, 𝑡) = 𝑈(𝜖)𝑒 𝑖(𝑘(cos(𝛼)𝑥+cos(𝛽)𝑦+cos(𝛾)𝑧)+𝜔𝑡) ,
(2)
By considering the above complex transformation (2) and Eq. (1), the reduced form of the 3D-RNLS equation with Kerr law nonlinearity can be written as
which
𝜗 = cos(𝛼)2 + cos(𝛽)2 + cos(𝛾)2 .
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𝑐 = −2𝜗𝜂𝑘,
(3)
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𝜗(𝛿 + 𝜂)𝑈 ′′ (𝜖) − (𝜗𝜂𝑘 2 + 𝜔)𝑈(𝜖) + 𝜎𝑈 3 (𝜖) = 0,
3. Exact solutions of the 3D-RNLS equation with Kerr law nonlinearity
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Exact solutions of the 3D-RNLS equation with Kerr law nonlinearity are established in this section by utilizing the new expansion methods based on the Jacobi elliptic equation. 3.1. Jacobi method
According to the new expansion method based upon the Jacobi elliptic equation and the terms 𝑈 ′′ (𝜖) and 𝑈(𝜖)3 , the solution of the 3D-RNLS equation with Kerr law nonlinearity can be written as 𝑈(𝜖) = 𝑎0 + 𝑎1
𝑓(𝜖) 1+𝑓(𝜖)2
+ 𝑎2
1−𝑓(𝜖)2 1+𝑓(𝜖)2
,
(4)
2
which 𝑎0 , 𝑎1 , and 𝑎2 are parameters to be determined and 𝑓(𝜖) is the Jacobi elliptic function satisfying the following ODE 𝑓 ′ (𝜖)2 = 𝐷 + 𝐸𝑓(𝜖)2 + 𝐹𝑓(𝜖)4 . By replacing the nontrivial solution (4) into Eq. (3) and exerting a series of calculations, we find −4𝜗𝐷𝛿𝑎2 − 4𝜗𝐷𝜂𝑎2 − 𝜗𝜂𝑘 2 𝑎0 − 𝜗𝜂𝑘 2 𝑎2 + 𝜎𝑎0 3 + 3𝜎𝑎0 2 𝑎2 + 3𝜎𝑎0 𝑎2 2 − 𝜔𝑎0 + 𝜎𝑎2 3 − 𝜔 𝑎2 = 0, −6𝜗𝐷𝛿𝑎1 − 6𝜗𝐷𝜂𝑎1 + 𝜗𝐸𝛿𝑎1 + 𝜗𝐸𝜂𝑎1 − 𝜗𝜂𝑘 2 𝑎1 + 3𝜎𝑎0 2 𝑎1 + 6𝜎𝑎0 𝑎1 𝑎2 + 3𝜎𝑎1 𝑎2 2 − 𝜔 𝑎1 = 0,
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12𝜗𝐷𝛿𝑎2 + 12𝜗𝐷𝜂𝑎2 − 8𝜗𝐸𝛿𝑎2 − 8𝜗𝐸𝜂𝑎2 − 3𝜗𝜂𝑘 2 𝑎0 − 𝜗𝜂𝑘 2 𝑎2 + 3𝜎𝑎0 3 + 3𝜎𝑎0 2 𝑎2 + 3𝜎 𝑎0 𝑎1 2 − 3𝜎𝑎0 𝑎2 2 − 3𝜔𝑎0 + 3𝜎𝑎1 2 𝑎2 − 3𝜎𝑎2 3 − 𝜔𝑎2 = 0, 2𝜗𝐷𝛿𝑎1 + 2𝜗𝐷𝜂𝑎1 − 6𝜗𝐸𝛿𝑎1 − 6𝜗𝐸𝜂𝑎1 + 2𝜗𝐹𝛿𝑎1 + 2𝜗𝐹𝜂𝑎1 − 2𝜗𝜂𝑘 2 𝑎1 + 6𝜎𝑎0 2 𝑎1 + 𝜎 𝑎1 3 − 6𝜎𝑎1 𝑎2 2 − 2𝜔𝑎1 = 0,
8𝜗𝐸𝛿𝑎2 + 8𝜗𝐸𝜂𝑎2 − 12𝜗𝐹𝛿𝑎2 − 12𝜗𝐹𝜂𝑎2 − 3𝜗𝜂𝑘 2 𝑎0 + 𝜗𝜂𝑘 2 𝑎2 + 3𝜎𝑎0 3 − 3𝜎𝑎0 2 𝑎2 + 3𝜎 𝑎0 𝑎1 2 − 3𝜎𝑎0 𝑎2 2 − 3𝜔𝑎0 − 3𝜎𝑎1 2 𝑎2 + 3𝜎𝑎2 3 + 𝜔𝑎2 = 0,
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𝜗𝐸𝛿𝑎1 + 𝜗𝐸𝜂𝑎1 − 6𝜗𝐹𝛿𝑎1 − 6𝜗𝐹𝜂𝑎1 − 𝜗𝜂𝑘 2 𝑎1 + 3𝜎𝑎0 2 𝑎1 − 6𝜎𝑎0 𝑎1 𝑎2 + 3𝜎𝑎1 𝑎2 2 − 𝜔𝑎1 = 0,
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4𝜗𝐹𝛿𝑎2 + 4𝜗𝐹𝜂𝑎2 − 𝜗𝜂𝑘 2 𝑎0 + 𝜗𝜂𝑘 2 𝑎2 + 𝜎𝑎0 3 − 3𝜎𝑎0 2 𝑎2 + 3𝜎𝑎0 𝑎2 2 − 𝜔𝑎0 − 𝜎𝑎2 3 + 𝜔 𝑎2 = 0.
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Now, the above nonlinear system is solved and the following results are obtained: Case 1. 𝑎0 = 0,
𝑎1 = ±4√−
𝑎0 = 0,
𝑎1 = 0,
𝑎0 = 0,
𝑎1 = 2√−
2𝜗(𝛿+𝜂) 𝜎
,
𝑎2 = 0,
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𝑎2 = ±2√ 2𝜗(𝛿+𝜂)
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𝜎
,
2𝜗(𝛿+𝜂) 𝜎
𝜔 = −(8𝜗𝛿 + (𝜗𝑘 2 + 8𝜗)𝜂),
𝜔 = 4𝜗𝛿 + (4𝜗 − 𝜗𝑘 2 )𝜂,
,
2𝜗(𝛿+𝜂)
𝑎2 = ± √
𝜎
,
𝑚 = 1,
𝑚 = 1,
𝜔 = −(2𝜗𝛿 + (𝜗𝑘 2 + 2𝜗)𝜂),
𝑚 = 1,
when 𝐷 = 1, 𝐸 = −(𝑚2 + 1), and 𝐹 = 𝑚2 . Now, due to 𝑓(𝜖) = 𝑠𝑛(𝜖) and 𝑠𝑛(𝜖, 1) → tanh(𝜖), the
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following exact solutions to the 3D-RNLS equation are constructed 𝑢1,2 (𝑥, 𝑦, 𝑧, 𝑡) = ±4 √−
2𝜗(𝛿+𝜂)
tanh(cos(𝛼)𝑥+cos(𝛽)𝑦+cos(𝛾)𝑧−2𝜗𝜂𝑘𝑡)
𝜎
1+tanh2 (cos(𝛼)𝑥+cos(𝛽)𝑦+cos(𝛾)𝑧−2𝜗𝜂𝑘𝑡)
𝑒 𝑖(𝑘(cos(𝛼)𝑥+cos(𝛽)𝑦+cos(𝛾)𝑧)−(8𝜗𝛿+(𝜗𝑘
2 +8𝜗)𝜂)𝑡)
𝑢3,4 (𝑥, 𝑦, 𝑧, 𝑡) = ±2 √
2𝜗(𝛿+𝜂) 1−tanh2 (cos(𝛼)𝑥+cos(𝛽)𝑦+cos(𝛾)𝑧−2𝜗𝜂𝑘𝑡) 𝑖(𝑘(cos(𝛼)𝑥+cos(𝛽)𝑦+cos(𝛾)𝑧)+(4𝜗𝛿+(4𝜗−𝜗𝑘 2 )𝜂)𝑡) 𝑒 , 𝜎 1+tanh2 (cos(𝛼)𝑥+cos(𝛽)𝑦+cos(𝛾)𝑧−2𝜗𝜂𝑘𝑡)
3
,
𝑢5,6 (𝑥, 𝑦, 𝑧, 𝑡) = (2√− √
2𝜗(𝛿+𝜂)
tanh(cos(𝛼)𝑥+cos(𝛽)𝑦+cos(𝛾)𝑧−2𝜗𝜂𝑘𝑡)
𝜎
1+tanh2 (cos(𝛼)𝑥+cos(𝛽)𝑦+cos(𝛾)𝑧−2𝜗𝜂𝑘𝑡)
±
2 2𝜗(𝛿+𝜂) 1−tanh2 (cos(𝛼)𝑥+cos(𝛽)𝑦+cos(𝛾)𝑧−2𝜗𝜂𝑘𝑡) ) 𝑒 𝑖(𝑘(cos(𝛼)𝑥+cos(𝛽)𝑦+cos(𝛾)𝑧)−(2𝜗𝛿+(𝜗𝑘 +2𝜗)𝜂)𝑡) . 𝜎 1+tanh2 (cos(𝛼)𝑥+cos(𝛽)𝑦+cos(𝛾)𝑧−2𝜗𝜂𝑘𝑡)
Case 2. 𝜗(𝛿+𝜂)
𝑎0 = ± √
2𝜎
,
𝑎1 = 0,
𝑎2 = ±
𝜗(𝛿+𝜂) 𝜗(𝛿+𝜂) 𝜎√ 2𝜎
,
1
𝜔 = 𝜗(−2𝜂𝑘 2 + 5𝛿 + 5𝜂), 2
1
𝑚= , 2
when 𝐷 = 1 − 𝑚2 , 𝐸 = 2𝑚2 − 1, and 𝐹 = −𝑚2 . Now, owing to 𝑓(𝜖) = 𝑐𝑛(𝜖), the following exact
𝜗(𝛿+𝜂)
𝑢7,8 (𝑥, 𝑦, 𝑧, 𝑡) = ±√
2𝜎
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solutions to the 3D-RNLS equation are established ± 1
1 2 𝜗(𝛿+𝜂) 1−𝑐𝑛 (cos(𝛼)𝑥+cos(𝛽)𝑦+cos(𝛾)𝑧−2𝜗𝜂𝑘𝑡,2) 𝑖(𝑘(cos(𝛼)𝑥+cos(𝛽)𝑦+cos(𝛾)𝑧)+(2𝜗(−2𝜂𝑘 2 +5𝛿+5𝜂))𝑡) 𝑒 . 1 𝜗(𝛿+𝜂) 1+𝑐𝑛2 (cos(𝛼)𝑥+cos(𝛽)𝑦+cos(𝛾)𝑧−2𝜗𝜂𝑘𝑡, ) 𝜎√ 2
2𝜎
𝑎0 = 0,
𝑎1 = ±4√−
𝑎0 = 0,
𝑎1 = 0,
𝑎0 = 0,
𝑎1 = 2√−
2𝜗(𝛿+𝜂) 𝜎
,
𝑎2 = ±2√ 𝜎
,
2𝜗(𝛿+𝜂) 𝜎
𝜔 = −(8𝜗𝛿 + (𝜗𝑘 2 + 8𝜗)𝜂), 𝜔 = 4𝜗𝛿 + (4𝜗 − 𝜗𝑘 2 )𝜂,
,
2𝜗(𝛿+𝜂)
𝑎2 = ± √
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2𝜗(𝛿+𝜂)
𝑎2 = 0,
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Case 3.
𝜎
,
𝑚 = 1,
𝑚 = 1,
𝜔 = −(2𝜗𝛿 + (𝜗𝑘 2 + 2𝜗)𝜂),
𝑚 = 1,
when 𝐷 = 𝑚2 , 𝐸 = −(𝑚2 + 1), and 𝐹 = 1. Now, due to 𝑓(𝜖) = 𝑛𝑠(𝜖) and 𝑛𝑠(𝜖, 1) → coth(𝜖), the
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following exact solutions to the 3D-RNLS equation are constructed 𝑢9,10 (𝑥, 𝑦, 𝑧, 𝑡) = ±4 2𝜗(𝛿+𝜂)
coth(cos(𝛼)𝑥+cos(𝛽)𝑦+cos(𝛾)𝑧−2𝜗𝜂𝑘𝑡)
𝜎
1+coth2 (cos(𝛼)𝑥+cos(𝛽)𝑦+cos(𝛾)𝑧−2𝜗𝜂𝑘𝑡)
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√−
𝑒 𝑖(𝑘(cos(𝛼)𝑥+cos(𝛽)𝑦+cos(𝛾)𝑧)−(8𝜗𝛿+(𝜗𝑘
2 +8𝜗)𝜂)𝑡)
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𝑢11,12 (𝑥, 𝑦, 𝑧, 𝑡) = ±2 √
2𝜗(𝛿+𝜂) 1−coth2 (cos(𝛼)𝑥+cos(𝛽)𝑦+cos(𝛾)𝑧−2𝜗𝜂𝑘𝑡) 𝑖(𝑘(cos(𝛼)𝑥+cos(𝛽)𝑦+cos(𝛾)𝑧)+(4𝜗𝛿+(4𝜗−𝜗𝑘 2 )𝜂)𝑡) 𝑒 , 𝜎 1+coth2 (cos(𝛼)𝑥+cos(𝛽)𝑦+cos(𝛾)𝑧−2𝜗𝜂𝑘𝑡)
𝑢13,14 (𝑥, 𝑦, 𝑧, 𝑡) = (2√− √
2𝜗(𝛿+𝜂)
coth(cos(𝛼)𝑥+cos(𝛽)𝑦+cos(𝛾)𝑧−2𝜗𝜂𝑘𝑡)
𝜎
1+coth2 (cos(𝛼)𝑥+cos(𝛽)𝑦+cos(𝛾)𝑧−2𝜗𝜂𝑘𝑡)
±
2 2𝜗(𝛿+𝜂) 1−coth2 (cos(𝛼)𝑥+cos(𝛽)𝑦+cos(𝛾)𝑧−2𝜗𝜂𝑘𝑡) ) 𝑒 𝑖(𝑘(cos(𝛼)𝑥+cos(𝛽)𝑦+cos(𝛾)𝑧)−(2𝜗𝛿+(𝜗𝑘 +2𝜗)𝜂)𝑡) . 𝜎 1+coth2 (cos(𝛼)𝑥+cos(𝛽)𝑦+cos(𝛾)𝑧−2𝜗𝜂𝑘𝑡)
Case 4. 4
,
𝜗(𝛿+𝜂)
𝑎0 = ± √
2𝜎
,
𝑎1 = 0,
𝑎2 = ∓
𝜗(𝛿+𝜂) 𝜗(𝛿+𝜂) 𝜎√ 2𝜎
,
1
𝜔 = 𝜗(−2𝜂𝑘 2 + 5𝛿 + 5𝜂), 2
1
𝑚= , 2
when 𝐷 = −𝑚2 , 𝐸 = 2𝑚2 − 1, and 𝐹 = 1 − 𝑚2 . Now, due to 𝑓(𝜖) = 𝑛𝑐(𝜖), the following exact solutions to the 3D-RNLS equation are established 𝜗(𝛿+𝜂)
𝑢15,16 (𝑥, 𝑦, 𝑧, 𝑡) = ±√
∓
2𝜎
1
1 2 𝜗(𝛿+𝜂) 1−𝑛𝑐 (cos(𝛼)𝑥+cos(𝛽)𝑦+cos(𝛾)𝑧−2𝜗𝜂𝑘𝑡,2) 𝑖(𝑘(cos(𝛼)𝑥+cos(𝛽)𝑦+cos(𝛾)𝑧)+(2𝜗(−2𝜂𝑘 2 +5𝛿+5𝜂))𝑡) 𝑒 . 1 𝜗(𝛿+𝜂) 1+𝑛𝑐 2 (cos(𝛼)𝑥+cos(𝛽)𝑦+cos(𝛾)𝑧−2𝜗𝜂𝑘𝑡, ) 𝜎√ 2
2𝜎
The three- and two-dimensional profiles of |𝑢2 (𝑥, 𝑦, 𝑧, 𝑡)| are plotted in Figure 1 by taking the
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parameters 𝜎 = 𝛿 = 1, cos(𝛽) = cos(𝛾) = 0.6, 𝑘 = 0.5, 𝜂 = −0.1, and 𝑥 = 𝑦 = 𝑡 = 0.
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Figure 1: The profiles of |𝑢2 (𝑥, 𝑦, 𝑧, 𝑡)| for 𝜎 = 𝛿 = 1, cos(𝛽) = cos(𝛾) = 0.6, 𝑘 = 0.5, 𝜂 = −0.1, and 𝑥 = 𝑦 = 𝑡 = 0.
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3.2. Kudryashov method (New form)
Based upon the Kudryashov method and the balance number 𝑁 = 1, the solution of the 3D-RNLS equation with Kerr law nonlinearity can be written as 𝑎1 ≠ 0,
ur
𝑈(𝜖) = 𝑎0 + 𝑎1 𝐾(𝜖),
(5)
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which 𝑎0 and 𝑎1 are parameters to be computed and 𝐾(𝜖) ia the solution of the following ODE 𝐾 ′ (𝜖)2 = 𝐾(𝜖)2 (1 − 𝜏𝐾(𝜖)2 ),
𝐾(𝜖) =
4𝐴 4𝐴2 𝑒 𝜖 +𝜏𝑒 −𝜖
,
𝜏 = 4𝐴𝐵.
Replacing the nontrivial solution (5) into Eq. (3) and utilizing a number of calculations yields −𝜗𝜂𝑘 2 𝑎0 + 𝜎𝑎0 3 − 𝜔𝑎0 = 0, 𝜗𝛿𝑎1 − 𝜗𝜂𝑘 2 𝑎1 + 𝜗𝜂𝑎1 + (3𝜎𝑎0 2 − 𝜔)𝑎1 = 0, 3𝜎𝑎0 𝑎1 2 = 0, 5
−2𝜗𝛿𝜏𝑎1 − 2𝜗𝜂𝜏𝑎1 + 𝜎𝑎1 3 = 0. By solving the above nonlinear system, the following results are derived 𝑎0 = 0,
𝑎1 = ±√
2𝜗𝜏(𝛿+𝜂) 𝜎
,
𝜔 = 𝜗(𝛿 − 𝜂𝑘 2 + 𝜂).
Now, the following exact solutions to the 3D-RNLS equation are constructed 𝑢1,2 (𝑥, 𝑦, 𝑧, 𝑡) = ±√
2𝜗𝜏(𝛿+𝜂)
4𝐴
𝜎
4𝐴2 𝑒 cos(𝛼)𝑥+cos(𝛽)𝑦+cos(𝛾)𝑧−2𝜗𝜂𝑘𝑡 +4𝐴𝐵𝑒 −(cos(𝛼)𝑥+cos(𝛽)𝑦+cos(𝛾)𝑧−2𝜗𝜂𝑘𝑡)
× 𝑒 𝑖(𝑘(cos(𝛼)𝑥+cos(𝛽)𝑦+cos(𝛾)𝑧)+𝜗(𝛿−𝜂𝑘
2 +𝜂)𝑡)
.
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The three- and two-dimensional profiles of |𝑢1 (𝑥, 𝑦, 𝑧, 𝑡)| are depicted in Figure 2 by considering the
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parameters 𝐴 = 𝐵 = 𝜎 = 𝛿 = 1, cos(𝛽) = cos(𝛾) = 0.6, 𝑘 = 0.5, 𝜂 = −0.1, and 𝑥 = 𝑦 = 𝑡 = 0.
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Figure 2: The profiles of |𝑢1 (𝑥, 𝑦, 𝑧, 𝑡)| for 𝐴 = 𝐵 = 𝜎 = 𝛿 = 1, cos(𝛽) = cos(𝛾) = 0.6, 𝑘 = 0.5,
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𝜂 = −0.1, and 𝑥 = 𝑦 = 𝑡 = 0.
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4. Conclusion
Our concern in the present work was to retrieve exact solutions of a nonlinear model with diverse applications in nonlinear optics namely ‘’the (3+1)-dimensional resonant nonlinear Schrödinger equation’’. In this regard, a wide variety of exact solutions in terms of Jacobi elliptic and exponential functions to the 3D-RNLS equation with Kerr law nonlinearity were successfully extracted by exerting the new expansion techniques based upon the Jacobi elliptic equation. The findings presented herein undeniably reveal the impressive capability of the new expansion methods to handle nonlinear Schrödinger equations.
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No conflict of interest exits in the submission of this manuscript, and manuscript is approved by all authors for publication.
Acknowledgment The first author (K. Hosseini) would like to acknowledge the financial support of the University of Mazandaran for this research work. References
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