
This article studied the new traveling wave solutions of the cascaded model with higher-order dispersion effects combined with the effects of spatiotemporal dispersion and multiplicative white noise. In the process of exploring traveling wave solutions, a clever combination of the polynomial complete discriminant system was used to discover more forms of traveling wave solutions for this equation. In order to better observe and analyze the propagation characteristics of traveling wave solutions, we used Maple and Matlab software to provide two-dimensional and three-dimensional visualization displays of the equation solutions. Meanwhile, we also analyzed the internal mechanism of nonlinear partial differential equations using planar dynamical systems. The research results indicated that there are differences in the results of different forms of soliton solutions affected by external random factors, which provided more beneficial references for people to better understand the cascaded model with higher-order dispersion effects combined with the effects of spatiotemporal dispersion and multiplicative white noise, and helped people to more comprehensively understand the propagation characteristics of optical solitons. The solution method in this article was also applicable to the study of other nonlinear partial differential equations.
Citation: Da Shi, Zhao Li, Dan Chen. New traveling wave solutions, phase portrait and chaotic patterns for the dispersive concatenation model with spatio-temporal dispersion having multiplicative white noise[J]. AIMS Mathematics, 2024, 9(9): 25732-25751. doi: 10.3934/math.20241257
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This article studied the new traveling wave solutions of the cascaded model with higher-order dispersion effects combined with the effects of spatiotemporal dispersion and multiplicative white noise. In the process of exploring traveling wave solutions, a clever combination of the polynomial complete discriminant system was used to discover more forms of traveling wave solutions for this equation. In order to better observe and analyze the propagation characteristics of traveling wave solutions, we used Maple and Matlab software to provide two-dimensional and three-dimensional visualization displays of the equation solutions. Meanwhile, we also analyzed the internal mechanism of nonlinear partial differential equations using planar dynamical systems. The research results indicated that there are differences in the results of different forms of soliton solutions affected by external random factors, which provided more beneficial references for people to better understand the cascaded model with higher-order dispersion effects combined with the effects of spatiotemporal dispersion and multiplicative white noise, and helped people to more comprehensively understand the propagation characteristics of optical solitons. The solution method in this article was also applicable to the study of other nonlinear partial differential equations.
The term soliton is an important concept in modern mathematics and physics. From fluid mechanics, plasma, condensed matter physics, elementary particle theory to astrophysics, solitons have been found everywhere. In 1973, Akira and Frederick [1,2] first proposed the concept of optical soliton and theoretically proved that optical pulses in any lossless fiber can deform into solitons during transmission and then stably transmit. Subsequently, people successively discovered bright solitons, dark solitons, black solitons, and gray solitons [3,4]. Due to the fact that optical soliton transmission does not change its waveform and speed, optical soliton communication quickly developed. With the urgent demand for long-distance and high-capacity optical communication, the transmission evolution of soliton pulses in optical fibers is also receiving increasing attention. With the continuous deepening of research on solitons, people have gradually established relatively complete mathematical and physical soliton theories, especially using nonlinear partial differential equations to establish some typical solitary wave equations: the Korteweg-de Vries (KdV) equation, Sine Gordon (SG) equation, and nonlinear Schrödinger (NLS) equation. For the solutions of these equations, researchers applied the modified extended tanh function method [5,6], traveling wave transformation method [7], Jacobi elliptic function expansion method [8], the improved direct algebraic scheme [9], the sub-equation method [10], Lie symmetry analysis [11,12], Painlevé analysis [13,14], Bäcklund transformation method [15], the Darboux transformation method [16], and other methods to actively explore the numerical and exact solutions of solitary wave equations, where they have achieved many results. However, most studies are mainly limited to ideal conditions that ignore the influence of external factors on transmission models. In fact, in actual communication systems, various types of noise cannot be avoided. When studying the transmission law of optical solitons in noisy environments, it is necessary to establish a random optical soliton transmission model. That is to say, when considering the influence of various external disturbances on the transmission model of optical solitons, it is necessary to use a random Schrödinger square to describe its transmission law. In references [17,18], the author used white noise functional analysis to study multiple Wick type stochastic models and achieved a number of results. However, more research is needed on the exact solution methods for solitary wave equations with random perturbations.
In our study, we contemplated the dimensionless expression of the cascaded model with higher-order dispersion effects, combined with the effects of spatiotemporal dispersion and multiplicative white noise in the Itô sense, which can be described as follows [19]:
ipt+apxx+bpxt+c|p|2p−iτ1(β1pxxx+β2|p|2px)+σ(p−ibpx)Wt(t)+τ2(β3pxxxx+β4|p|2pxx+β5|p|4p+β6|px|2p+β7p2xp∗+β8p∗xxp2)−iτ3(β9pxxxxx+β10|p|2pxxx+β11|p|4px+β12ppxp∗xx+β13p∗pxpxx+β14pp∗xpxx+β15p2xp∗x)=0. | (1.1) |
Here, the complex valued function p=p(x,t) stands for the wave profile. Parameter σ is used to reflect the intensity of white noise and is a positive constant, and i is the imaginary unit that satisfies i2=−1. W(t) is a standard Wiener process which is defined as W(t)=∫t0f(T)dW(T), where T<t, T stands for a stochastic variable and Wt(t)=dWdt [20] represents multiplicative white noise. This noise is used to identify the process where the excitation phase is interrupted.
Equation (1.1) investigates the effects of spatiotemporal dispersion and multiplicative white noise on the propagation of optical solitons. Regarding the influence of spatiotemporal dispersion on the propagation of optical solitons, Arnous et al. [19] used an improved Kudryashov method to study the effects of spatiotemporal dispersion and multiplicative white noise on soliton propagation in a cascaded model, and Liu et al. [21] selected an appropriate coefficient function to study the dynamic behavior of single solitons. The authors of Ref. [22] used the improved Kudryashov method to study the effect of spatio-temporal dispersion and multiplicative white noise on the propagation of optical solitons. The authors of Ref. [23] conducted in-depth research on the chaos phenomenon in the cascaded model and obtained accurate solutions for the cascaded model. Compared with these existing studies, our study provides more forms of accurate solutions and uses planar dynamical systems to perform chaotic analysis on nonlinear systems, enabling people to have a more comprehensive and in-depth understanding of the impact of spatiotemporal dispersion and multiplicative noise on optical soliton propagation in cascaded models, which is conducive to the wider application of optical solitons.
This article includes the following main parts: Section 2 introduces the wave transformation of the solution of Eq (1.1) and proves that the equation has an exact solution with polynomial function modules. Section 3 conducted a planar dynamic system analysis on Eq (1.1). Section 4 provides a detailed derivation process for the exact solution of optical solitons based on the polynomial complete discriminant system classification, obtaining more forms of traveling wave solutions. Section 5 provides visualization analysis of the solutions. Finally, we provide our research conclusion.
This article considered the traveling wave solution of Eq (1.1) in the following form:
p(x,t)=Q(ζ)eiϕ(x,t). | (2.1) |
The wave variable ζ is defined as
ζ=h(x−vt), | (2.2) |
where h and v are nonzero constants. Q(ζ) is a real-valued function which stands for the amplitude components of the solutions, v represents the speed of the soliton, and the phase component
ϕ(x,t)=−κx+ωt+σW(t)−32σ2t+θ0. | (2.3) |
Here, κ stands for the frequency of the solitons, ω denotes to the wave number, and θ0 represents the phase constant.
By inserting Eqs (2.1)–(2.3) into Eq (1.1) [24] and decomposing the real and imaginary parts of the solution, we can obtain the following expressions:
h2(10β9κ3τ3−6β3κ2τ2−3β1κτ1+a−bv)Q″+h4(β3τ2−5β9κτ3)Q(4)+(κ4(β3τ2−β9κτ3)+β1κ3τ1−aκ2−(bκ−1)(σ2−ω))Q+(β5τ2−β11κτ3)Q5+(κ2((β10+β12+β13−β14−β15)κτ3−(β4−β6+β7+β8)τ2)−β2κτ1+c)Q3+h2((β4+β8)τ2−(3β10+β12+β13−β14)κτ3)Q2Q″+h2((2β12−2(β13+β14)−β15)κτ3+(β6+β7)τ2)QQ′2=0. | (2.4) |
h(−5β9κ4τ3+4β3κ3τ2+3β1κ2τ1−2aκ−bσ2+bω+(bκ−1)v)Q′−β9τ3h5Q(5)−h3(2κ(2β3τ2−5β9κτ3)+β1τ1)Q(3)−β11hτ3Q4Q′−β10h3τ3Q2Q(3)−β15h3τ3Q′3−(β12+β13+β14)τ3h3QQ′Q″+h(κ((−3β10+β12−3β13+β14+β15)κτ3+2(β4+β7−β8)τ2)+β2τ1)Q2Q′=0, | (2.5) |
with the following parametric restrictions:
β9=β10=β11=β15=0, | (2.6) |
and
β12+β13+β14=0. | (2.7) |
Equation (2.5) can be simplified to
h(4β3κ3τ2+3β1κ2τ1−2aκ−bσ2+bω+(bκ−1)v)Q′−h3(4κβ3τ2+β1τ1)Q(3)+h(κ(−4β13κτ3+2(β4+β7−β8)τ2)+β2τ1)Q2Q′=0. | (2.8) |
Let the coefficients of the variable in the imaginary part of Eq (2.8) be zero. We can obtain the following parameter values:
v=−4β3κ3τ2+3β1κ2τ1−2aκ−bσ2+bωbκ−1, | (2.9) |
κ=(−2β2β3+β1β4+β1β7−β1β8)τ22β1β13τ3, | (2.10) |
and Eq (1.1) can be reduced to
ipt+apxx+bpxt+c|p|2p−iτ1(β1pxxx+β2|p|2px)+σ(p−ibpx)Wt(t)+τ2(β3pxxxx+β4|p|2pxx+β5|p|4p+β6|px|2p+β7p2xp∗+β8p∗xxp2)−iτ3(β12ppxp∗xx+β13p∗pxpxx+β14pp∗xpxx)=0, | (2.11) |
and Eq (2.4) can be reduced to
h4β3τ2Q(4)+h2(β4τ2+β8τ2+2β14κτ3)Q2Q″+h2(−6β3κ2τ2−3β1κτ1+a−bv)Q″+h2(−4(β13+β14)κτ3+β6τ2+β7τ2)QQ′2+β5τ2Q5+(−2κ3β14τ3−κ2β4τ2+κ2β6τ2−κ2β7τ2−κ2β8τ2−β2κτ1+c)Q3+(β3κ4τ2+β1κ3τ1−aκ2−bκσ2+bκω+σ2−ω)Q=0. | (2.12) |
Equation (2.12) can be further reduced to
h2Q(4)(ζ)+η6Q(ζ)2Q″(ζ)+η5Q″(ζ)+η4Q(ζ)Q′2(ζ)+η3Q(ζ)5+η2Q(ζ)3+η1Q(ζ)=0, | (2.13) |
with η1=(β3κ4τ2+β1κ3τ1−aκ2−bκσ2+bκω+σ2−ω)/(h2β3τ2), η2=(−2κ3β14τ3−κ2β4τ2+κ2β6τ2−κ2β7τ2−κ2β8τ2−β2κτ1+c)/(h2β3τ2), η3=(β5)/(h2β3), η4=(−4(β13+β14)κτ3+β6τ2+β7τ2)/(β3τ2), η5=(−6β3κ2τ2−3β1κτ1+a−bv)/(β3τ2), η6=(β4τ2+β8τ2+2β14κτ3)/(β3τ2), where h2β3τ2≠0.
By the trial equation method [25], Eq (2.13) has a polynomial solution Q(ζ), which satisfies the following equation:
Q″(ζ)=α0+α1Q+α3Q3. | (2.14) |
Suppose Eq (2.13) has the following polynomial solution Q(ζ):
Q″(ζ)=F(Q)=α0+α1Q+α2Q2+α3Q3. | (2.15) |
After integrating Eq (2.15), it can be concluded that:
(Q′)2=12α3Q4+23α2Q3+α1Q2+2α0Q+d. | (2.16) |
Taking the derivative of Eq (2.16) yields:
Q(3)=α1Q′+2α2QQ′+3α3Q2Q′, | (2.17) |
and from Eq (2.17), we can obtain
Q(4)= 6α23Q5+10α2α3Q4+(10α1α3+103α22)Q3 +(5α1α2+15α0α3)Q2+ (α21+6α0α2+6α3d)Q+α0α1+2α2d. | (2.18) |
Substituting Eqs (2.16)–(2.18) into Eq (2.13), it can be concluded that:
(6h2α23+α3η6+12α3η4+η3)Q5+(10h2α2α3+α2η6+23α2η4)Q4+(10h2α1α3+103h2α22+α1η6+α3η5+α1η4+η2)Q3+(5h2α1α2+152α0α3+α0η6+α2η5+2α0η4)Q2+(h2α21+6h2α0α2+6h2α3d+α1η5+dη4+η1)Q+h2α0α1+2h2α2d+α0η5=0. | (2.19) |
Equation (2.19) is a 5th degree equation about the function variable Q. To determine the coefficient αi,i=0,⋯,5, supposing all coefficients of the Eq (2.19) are 0,
{6h2α23+α3η6+12α3η4+η3=0,10h2α2α3+α2η6+23α2η4=0,10h2α1α3+103h2α22+α1η6+α3η5+α1η4+η2=0,5h2α1α2+15h2α0α3+α0η6+α2η5+2α0η4=0,h2α21+6h2α0α2+6h2α3d+α1η5+dη4+η1=0,h2α0α1+2h2α2d+α0η5=0. | (2.20) |
Based on Eq (2.20), we can obtain the following results:
{α3=−(2η6+η4)±√(2η6+η4)2−96h2η324h2, α2=0, α1=−α3η5+η210h2α3+η4+η6,α0=0, d=h2α21+α1η5+η16h2α3+η4, | (2.21) |
or
{α3=−(2η6+η4)±√(2η6+η4)2−96h2η324h2, α2=0, α1=−η5h2,α0=C, d=h2α21+α1η5+η16h2α3+η4, | (2.22) |
where C is an arbitrary nonzero constant.
In either Eq (2.21) or Eq (2.22), the coefficient α2 is zero, so Eq (2.13) has the solution in the form of Eq (2.14).
In order to observe the stability state of the Eq (1.1), as well as the condition of the system being affected by external random factors, we are going to discuss the dynamic behavior [26,27,28,29] characteristics of the Eq (1.1).
In the absence of precise expressions for solutions, phase diagram analysis is an effective method for analyzing the behavioral characteristics of solutions.
Equation (2.14) can be expressed as the two-dimensional system of equations in the following form:
{dQdζ=y,dydζ=α3Q3+α1Q. | (3.1) |
Then, the corresponding Hamilton system of Eq (3.1) is as follows
H(Q,y)=12y2−(α12Q2+α34Q4). | (3.2) |
While α1α3>0, there is an equilibrium point (0,0) for the system (see Figure 1a,d), and the point (0,0) is also the saddle point in Figure 1a. While α1α3<0, we can get three equilibrium points of the system: (0,0), (−√−α1α3,0), and (√−α1α3,0) (see Figure 1b,c). From Figure 1b,c,d, we can conclude that Eq (3.1) has periodic solutions because they all comprise closed orbits, while in the case of Figure 1a, Eq (3.1) may contain optical soliton solutions.
Next, we add a perturbation factor to Eq (3.1) to to analyze the sensitivity of this system,
{dQdζ=y,dydζ=α3Q3+α1Q+Acos(ϖζ), | (3.3) |
where ϖ represents frequency and A represents amplitude.
We fix parameters α1 and α3, and adjust the values of A and ϖ to compare the impact of external disturbances on the system. The phase portraits of Figure 2a,b,d,e and the sensitivity analysis of Figure 3 shows that the system is highly sensitive to the influence of frequency, therefore, in practical applications, we should explore appropriate frequencies to ensure stable operation of the system. The Poincaré sections (see Figure 2c,f) show the existence of chaotic states and quasiperiodic solutions in the system.
According to the derivation in Section 2, as long as the solution to Eq (2.16) under Eq (2.21) is obtained, the solution to Eq (2.13) can be obtained.
Assuming
λ=2α1α3, μ=4α0α3, τ=2dα3, | (4.1) |
then Eq (2.16) can be transformed to
±√α32(ζ−ζ0)=∫dQ√Q4+λQ2+μQ+τ=∫dQ√F(Q), | (4.2) |
where ζ0 is an integral constant and F(Q)=Q4+λQ2+μQ+τ.
According the complete discriminant system for fourth order polynomials [30]
{D1=4,D2=−λ,D3=−2λ3+8λτ−9μ2,D4=−λ3μ2+4λ4τ+36λμ2τ−32λ2τ2−274μ4+64τ3,E2=9λ2−32λτ, | (4.3) |
the roots of quartic polynomials F(x)=x4+λx2+μx+τ can be classified into the following types:
(ⅰ) If D2<0, D3=0, D4=0, then F(x) has a pair of conjugate complex roots.
(ⅱ) If D2=0, D3=0, D4=0, then F(x) has one quadruple root.
(ⅲ) If D2>0, D3=0, D4=0, E2>0, then F(x) has two different double real roots.
(ⅳ) If D2>0, D3>0, D4=0, then F(x) has one double real root and two single real roots.
(ⅴ) If D2>0, D3=0, D4=0, E2=0, then F(x) has a triple real root and a single real root.
(ⅵ) If D2D3<0, D4=0, then F(x) has a double real root and a pair of conjugate complex roots.
(ⅶ) If D1>0, D3>0, D4>0, then F(x) has four real roots.
(ⅷ) If D2D3≥0, D4<0, then F(x) has two different real roots and a pair of conjugate complex roots.
(ⅸ) If D2D3≤0, D4>0, then F(x) has two pair of conjugate complex roots.
According to the Liu's classification for the roots of quartic polynomials (see [30]), we can derive the following solutions of Eq (1.1):
When D2<0, D3=0, D4=0, Eq (1.1) admits the following solution:
p1(x,t)=[stan[s√α32(h(x−vt)−ζ0)]+l]ei(−κx+ωt+σW(t)−32σ2t+θ0). | (4.4) |
When D2<0, D3=0, D4=0, F(Q) has a pair of conjugate complex roots, namely: F(Q)=[(Q−l)2+s2]2. Here, l and s are both real numbers, and s>0. So, Eq (4.2) can be transformed into
±√α32(ζ−ζ0)=∫dQ(Q−l)2+s2=1sarctanQ−ls. | (4.5) |
So, we can get the solution to Eq (2.16):
Q=stan[s√α32(ζ−ζ0)]+l. | (4.6) |
Inserting Eq (4.6) into Eq (2.1), the exact solution p1(x,t) of Eq (1.1) can be attained.
When D2=0, D3=0, D4=0, Eq (1.1) admits the following solution:
p2(x,t)=−√2√α3(h(x−vt)−ζ0)ei(−κx+ωt+σW(t)−32σ2t+θ0). | (4.7) |
If D2=0, D3=0, D4=0, F(Q) has one quadruple root, namely: F(Q)=Q4. Then, Eq (4.2) can be transformed into
±√α32(ζ−ζ0)=∫dQQ2=−Q−1. | (4.8) |
So, the solution to Eq (2.16) can be described as follows
Q=−√2√α3(ζ−ζ0). | (4.9) |
Substituting Eq (4.9) into Eq (2.1), the exact solution p2(x,t) of Eq (1.1) can be attained.
When D2>0, D3=0, D4=0, E2>0, the following solutions of Eq (1.1) can be derived:
p3(x,t)=[l−s2[coth[√α38(s−l)(h(x−vt)−ζ0)]−1]+l]ei(−κx+ωt+σW(t)−32σ2t+θ0), | (4.10) |
p4(x,t)=[l−s2[tanh[√α38(s−l)(h(x−vt)−ζ0)]−1]+l]ei(−κx+ωt+σW(t)−32σ2t+θ0). | (4.11) |
If D2>0, D3=0, D4=0, E2>0, F(Q) has two different double real roots, namely: F(Q)=(Q−s)2(Q−l)2. Here, l and s are both real numbers, and s>l. From Eq (4.2), we can obtain
±√α32(ζ−ζ0)=∫dQ(Q−s)(Q−l)=1s−lln|Q−sQ−l|. | (4.12) |
When Q>s or Q<l, the solution to Eq (2.16) can be derived:
Q=−l−se√α32(s−l)(ζ−ζ0)−1+l=l−s2[coth[√α38(s−l)(ζ−ζ0)]−1]+l. | (4.13) |
When l<Q<s, the solution to Eq (2.16) can be derived:
Q=−l−s−e√α32(s−l)(ζ−ζ0)−1+l=l−s2[tanh[√α38(s−l)(ζ−ζ0)]−1]+l. | (4.14) |
Uniting Eq (4.9) and Eq (2.1), we can get the exact solutions p3(x,t) and p4(x,t) of Eq (1.1).
When D2>0, D3>0, D4=0, Eq (1.1) has implicit function solutions.
If D2>0, D3>0, D4=0, F(Q) has one double real root and two single real roots, namely: F(Q)=(Q−s)2(Q−l)(Q−m). Here, l, s, and m are real numbers, and l>m.
When s>l and Q>l, from Eq (4.2), we can obtain the implicit function solution of Eq (2.16):
±√α32(ζ−ζ0)=1(s−l)(s−m)ln[√(Q−l)(s−m)−√(s−l)(Q−m)]2|Q−s|. | (4.15) |
When s>l and Q<m, or s<m and Q<l, from Eq (4.2), we can obtain the implicit function solution of Eq (2.16):
±√α32(ζ−ζ0)=1(s−l)(m−s)ln[√(Q−l)(m−s)−√(l−s)(Q−m)]2|Q−s|. | (4.16) |
When l>s>m from Eq (4.2), we can obtain the implicit function solution of Eq (2.16):
±√α32(ζ−ζ0)=1(l−s)(s−m)arcsin(Q−l)(s−m)+(s−l)(Q−m)|(Q−s)(l−m)|. | (4.17) |
By combining Eqs (4.15)–(4.17) and Eq (2.1), the implicit function solution of Eq (1.1) can be acquired.
When D2>0, D3=0, D4=0, E2=0, we are able to derive the following solution for Eq (1.1):
p5(x,t)=[8(s−l)α3(l−s)2(h(x−vt)−ζ0)2−8+s]ei(−κx+ωt+σW(t)−32σ2t+θ0). | (4.18) |
When D2>0, D3=0, D4=0, E2=0, F(Q) has a triple real root and a single real root, namely: F(Q)=(Q−s)3(Q−l). Here, s and l are both real numbers.
When Q>s and Q>l, or Q<s and Q<l, from Eq (4.2), we can get the solution of Eq (2.16):
Q=8(s−l)α3(l−s)2(ζ−ζ0)2−8+s. | (4.19) |
Accordingly, by combining Eq (4.19) and Eq (2.1), we can derive the exact solution p5(x,t) of Eq (1.1).
When D2D3<0, D4=0, Eq (1.1) has the solution
p6(x,t)=e±√(s−l)2+m2√α32(h(x−vt)−ζ0)−γ+√(s−l)2+m2(2−γ)[e±√(s−l)2+m2√α32(h(x−vt)−ζ0)−γ]2−1ei(−κx+ωt+σW(t)−32σ2t+θ0). | (4.20) |
While D2D3<0, D4=0, F(Q) has a double real root and a pair of conjugate complex roots, namely: F(Q)=(Q−s)2[(Q−l)2+m2]. Here, s, l, and m are real numbers.
Thus, the equivalent form of Eq (4.2) is
±√α32(ζ−ζ0)=∫dQ(Q−s)√(Q−l)2+m2=1√(s−l)2+m2ln|γQ+δ−√(Q−l)2+m2Q−s|, | (4.21) |
where γ=s−2l√(s−l)2+m2, δ=√(s−l)2+m2−s(s−2l)√(s−l)2+m2.
With further derivation, the solution to Eq (2.16) can be described as
Q=e±√(s−l)2+m2√α32(ζ−ζ0)−γ+√(s−l)2+m2(2−γ)[e±√(s−l)2+m2√α32(ζ−ζ0)−γ]2−1. | (4.22) |
Putting Eq (4.22) into Eq (2.1), the exact solution p6(x,t) of Eq (1.1) can be derived.
When D1>0, D3>0, D4>0, Eq (1.1) has the solutions
p7(x,t)=l(s−n)sn2(√α3(s−m)(l−n)2√2(h(x−vt)−ζ0),r)−s(l−n)(s−n)sn2(√α3(s−m)(l−n)2√2(h(x−vt)−ζ0),r)−l+nei(−κx+ωt+σW(t)−32σ2t+θ0). | (4.23) |
p8(x,t)=n(l−m)sn2(√α3(s−m)(l−n)2√2(h(x−vt)−ζ0),r)−m(l−n)(l−m)sn2(√α3(s−m)(l−n)2√2(h(x−vt)−ζ0),r)−l+nei(−κx+ωt+σW(t)−32σ2t+θ0). | (4.24) |
While D1>0, D3>0, D4>0, F(Q) has four real roots, namely: F(Q)=(Q−s)(Q−l)(Q−m)(Q−n). Here, s, l, m, and n are real numbers, and s>l>m>n.
When Q>s or Q<n, the following changes:
Q=l(s−n)sin2φ−s(l−n)(s−n)sin2φ−(l−n). | (4.25) |
When m<Q<l, the following changes:
Q=n(l−m)sin2φ−m(l−n)(l−m)sin2φ−(l−n). | (4.26) |
Under the given conditions, Eq (4.2) can be transformed into
√α32(ζ−ζ0)=∫dQ√(Q−s)(Q−l)(Q−m)(Q−n)=2√(s−m)(l−n)∫dQ√1−r2sin2φ, | (4.27) |
where r2=(s−n)(l−m)(s−m)(l−n).
According to Eq (4.27) and the definition of the Jacobian elliptic sine function, the following conclusions can be obtained:
sn(√α3(s−m)(l−n)2√2(ζ−ζ0),r)=sinφ. | (4.28) |
So the corresponding solution of Eq (2.16) is
Q=l(s−n)sn2(√α3(s−m)(l−n)2√2(ζ−ζ0),r)−s(l−n)(s−n)sn2(√α3(s−m)(l−n)2√2(ζ−ζ0),r)−l+n, | (4.29) |
and
Q=n(l−m)sn2(√α3(s−m)(l−n)2√2(ζ−ζ0),r)−m(l−n)(l−m)sn2(√α3(s−m)(l−n)2√2(ζ−ζ0),r)−l+n, | (4.30) |
Substituting Eqs (4.29) and (4.30) into Eq (2.1), respectively, we can get the exact solutions p7(x,t) and p8(x,t) of Eq (1.1).
When D2D3≥0, D4<0, Eq (1.1) has the solution
p9(x,t)=c1cn(√∓α3ne(s−l)2re(h(x−vt)−ζ0),r)+c2c3cn(√∓α3ne(s−l)2re(h(x−vt)−ζ0),r)+c4ei(−κx+ωt+σW(t)−32σ2t+θ0). | (4.31) |
If D2D3≥0, D4<0, F(Q) has two different real roots and a pair of conjugate complex roots, namely: F(Q)=(Q−s)(Q−l)[(Q−m)2+n2]. Here, s, l, m, and n are both real numbers, s>l, and n>0.
Introducing the following transformation:
Q=c1cosφ+c2c3cosφ+c4, | (4.32) |
where c1=12(s+l)c3−12(s−l)c4, c2=12(s+l)c4−12(s−l)c3, c3=s−m−ne, c4=s−m−ne, E=n2+(s−m)(l−m)n(s−l), e=E−√E2+1.
Under the given conditions, Eq (4.2) can be transformed to
√α32(ζ−ζ0)=∫dQ√±(Q−s)(Q−l)[(Q−m)2+n2]=2re√∓2ne(s−l)∫dQ√1−r2sin2φ, | (4.33) |
where r2=11+e2.
According to Eq (4.33) and the definition of the Jacobian elliptic cosine function, we can get
cn(√∓α3ne(s−l)2re(ζ−ζ0),r)=cosφ. | (4.34) |
So the corresponding solution of Eq (2.16) can be depicted as
Q=c1cn(√∓α3ne(s−l)2re(ζ−ζ0),r)+c2c3cn(√∓α3ne(s−l)2re(ζ−ζ0),r)+c4, | (4.35) |
and then the exact solution p9(x,t) of Eq (1.1) can be derived.
When D2D3≤0, D4>0, Eq (1.1) has the solution
p10(x,t)=c1sn(ε(h(x−vt)−ζ0),r)+c2cn(ε(h(x−vt)−ζ0),r)c3sn(ε(h(x−vt)−ζ0),r)+c4cn(ε(h(x−vt)−ζ0),r)ei(−κx+ωt+σW(t)−32σ2t+θ0). | (4.36) |
While D2D3≤0, D4>0, F(Q) has two pairs of conjugate complex roots, namely: F(Q)=[(Q−s)2+l2][(Q−m)2+n2]. Here, s, l, m, and n are real numbers, and l≥n>0.
Making the following transformation:
Q=c1tanφ+c2c3tanφ+c4, | (4.37) |
where c1=sc3+lc4, c2=sc4−lc3, c3=−l−m−ne, c4=s−m, E=(s−m)2+l2+n22ln, e=E+√E2−1.
So, we can obtain the equivalent form of Eq (4.2)
√α32(ζ−ζ0)=∫dQ√[(Q−s)2+l2][(Q−m)2+n2]=c23+c24n√(c23+c24)(e2c23+c24)∫dQ√1−r2sin2φ, | (4.38) |
where r2=e2−1e2.
According to Eq (4.38) and the definition of the Jacobian elliptic cosine function and the Jacobian elliptic cosine function, we can derive the following results:
sn(n√α3(c23+c24)(e2c23+c24)√2(c23+c24)(ζ−ζ0),r)=sinφ. | (4.39) |
cn(n√α3(c23+c24)(e2c23+c24)√2(c23+c24)(ζ−ζ0),r)=cosφ. | (4.40) |
Then we can obtain the solution of Eq (2.16) as
Q=c1sn(ε(ζ−ζ0),r)+c2cn(ε(ζ−ζ0),r)c3sn(ε(ζ−ζ0),r)+c4cn(ε(ζ−ζ0),r), | (4.41) |
where ε=n√α3(c23+c24)(e2c23+c24)√2(c23+c24), and the exact solution p10(x,t) of Eq (1.1) can be derived.
In order to better observe the propagation characteristics of the traveling wave solution of Eq (1.1), we visualized the obtained traveling wave solutions p1,p5,p7,p9,p10 in 2D and 3D graphs with Maple and Matlab software. Figures 4–8 show that traveling wave solitons have distinct shapes and propagation characteristics, specifically, their modulus exhibit different periodic characteristics and prominent changes. The real and imaginary part images of these solutions help people understand the different phases or polarization states of waves, while the modulus images of the solutions can help people understand the amplitude distribution of waves, which plays an important role in understanding phenomena such as wave propagation, reflection, and interference. Figure 4 shows the morphological characteristics of traveling wave solution with tangent function modulus in 2D and 3D graphs. We compare the morphological characteristics of the real and imaginary parts of p5,p7,p9,p10 under different intensities of random interference in Figures 5–8. For the traveling wave solution with rational function modulus, its real and imaginary parts undergo significant irregular abrupt changes under low intensity random interference, and its modulus does not exhibit periodic morphological characteristics (Figure 5). However, Figures 6 and 7 show that the real and imaginary parts of the traveling wave solutions with Jacobian sine function modulus or Jacobian cosine function modulus undergo significant irregular sudden changes under high intensity random interference, and their modulus exhibit periodic morphological characteristics. From Figure 9, we can observe that the traveling wave maintains a certain periodic fluctuation during propagation, but with the enhancement of external random interference, the local mutation of the traveling wave becomes more pronounced.
This article enriches the research on the traveling wave solution of Eq (1.1), and combines visualization techniques to analyze the morphological changes and propagation characteristics of traveling wave solutions. Compared with other literature, this article provides more forms of exact solutions, such as the Jacobian elliptic functions, which is beneficial for people to have a more comprehensive understanding of the morphological changes of the exact solution of Eq (1.1). By applying random interference factors of different intensities, the influence of random factors on the solution of Eq (1.1) were explored, providing more references for further in-depth research on the internal mechanism of Eq (1.1) and its practical application. These research results are also beneficial for people to better understand the propagation characteristics of traveling waves and promote the wider application of the system Eq (1.1).
Da Shi: Writing-Review & Editing; Writing-Original Draft; Zhao Li: Software; Dan Chen: Formal Analysis. All authors have read and approved the final version of the manuscript for publication.
The authors declare they have not used Artificial Intelligence (AI) tools in the creation of this article.
The authors declare no conflicts of interest.
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