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Wave-speed management of dipole, bright and W-shaped solitons in optical metamaterials

Houria Triki Radiation Physics Laboratory, Department of Physics, Faculty of Sciences, Badji Mokhtar University, P. O. Box 12, 23000 Annaba, Algeria    Vladimir I. Kruglov Centre for Engineering Quantum Systems, School of Mathematics and Physics, The University of Queensland, Brisbane, Queensland 4072, Australia
Abstract

Wave-speed management of soliton pulses in a nonlinear metamaterial exhibiting a rich variety of physical effects that are important in a wide range of practical applications, is studied both theoretically and numerically. Ultrashort electromagnetic pulse transmission in such inhomogeneous system is described by a generalized nonlinear Schrödinger equation with space-modulated higher-order dispersive and nonlinear effects of different nature. We present the discovery of three types of periodic wave solutions that are composed by the product of Jacobi elliptic functions in the presence of all physical processes. Envelope solitons of the dipole, bright and W-shaped types are also identified, thus illustrating the potentially rich set of localized pulses in the system. We develop an effective similarity transformation method to investigate the soliton dynamics in the presence of the inhomogeneities of media. The application of developed method to control the wave speed of the presented solitons is discussed. The results show that the wave speed of dipole, bright and W-shaped solitons can be effectively controlled through spatial modulation of the metamaterial parameters. In particular, the soliton pulses can be decelerated and accelerated by suitable variations of the distributed dispersion parameters.

pacs:
05.45.Yv, 42.65.Tg

I Introduction

Soliton formation in nonlinear metamaterials is presently a very active area of research PLi ; Pendry ; Reed ; Zharov ; Parazzoli ; Shen . Such new materials are known as negative-index materials and more commonly referred to as left-handed metamaterials Kozyrev1 . To demonstrate solitons experimentally, left-handed nonlinear transmission lines, employed as nonlinear metamaterials, have been recently used to study the generation of envelope solitons Kozyrev1 ; Kozyrev2 ; Kozyrev3 ; Kozyrev4 . In addition, the stable generation of soliton pulses has been also demonstrated experimentally in an active nonlinear metamaterial formed by a left-handed transmission line inserted into a ring resonator Kozyrev3 . Moreover, dark envelope solitons in a practical left-handed nonlinear transmission line with series nonlinear capacitance are demonstrated by circuit analysis, which showed that the left-handed nonlinear transmission lines could support dark solitons by tailoring the circuit parameters Kozyrev4 . Furthermore, a left-handed nonlinear electrical lattice has been shown to support the formation of discrete envelope solitons of the bright and dark type English . These significant results indicate that the soliton propagation is one of the physically relevant phenomena associated with practical nonlinear metamaterials.

To describe the transmission of an ultrashort optical pulse through an homogeneous nonlinear metamaterial, a generalized nonlinear Schrödinger equation (NLSE) for a dispersive dielectric susceptibility and permeability has been introduced by Scalora et al. Scalora . One should note here that the utilization of the NLSE to describe the nonlinear wave dynamics is not only restricted to nonlinear metamaterials, but also to other important physical media like optical fibers Agra , Bose-Einstein condensates Beitia , plasma physics Dodd , biomolecular dynamics Davydov , etc. Regarding realistic optical waveguiding media, they are actually inhomogeneous because of the existence of some nonuniformities which arise due to various factors such as the variation of lattice parameters in the optical medium, the imperfection of manufacture and fluctuation of the system diameters Abdullaev ; Lei . With consideration of the inhomogeneities in an optical material, the theoretical description of the light pulse dynamics is mainly based on the generalized NLSE equation with varying group velocity dispersion, nonlinearity, and gain (absorption) coefficients Serkin ; Kruglov3 ; Kruglov4 . Especially in optics, the application of such generalized NLSE has stimulated further studies of the integrable inhomogeneous equations giving rise to the concepts of nonautonomous and self-similar solitons Serkin ; Kruglov3 ; Kruglov4 ; Chen ; Ponomarenko ; Serkin2 . For the soliton transmission in an optical medium within the femtosecond duration range, however, the higher-order effects influenced by the variations of material parameters should be also taken into account Abdullaev1 .

From a physical viewpoint, a soliton structure can be described by four parameters which are the frequency (or velocity), amplitude (or width), time position and phase Has5 . An appropriate modulation of these parameters allows efficient control of the soliton dynamics. Recently, the problem of optimal control the parameters of optical solitons which is also called the problem of soliton management becomes a subject of significant interest Belya ; R1 ; R2 . This because concepts of soliton dispersion management and soliton control in optical fiber systems constitute a physically relevant developments in the practical application of envelope solitons for optical transmissions Hasegawa1 ; Hasegawa2 ; Hasegawa3 ; Hasegawa4 . Interestingly, studies of dispersion management have demonstrated that several effects can be reduced by utilizing this technique such as the modulational instability Doran1 , Gordon-Haus effect resulting from the interaction with noise Doran2 , radiation due to lumped amplifiers compensating the fiber loss Doran3 , and time jitters caused by the collisions between signals Doran4 .

While the control of solitons shape or amplitude under dispersion and nonlinearity managements have been demonstrated in physical systems within the framework of both cubic and higher-order NLSE models, the control of soliton wave speed in nonlinear media has been studied thus far only for the cubic NLSE case in Luke . With use of this envelope equation which includes only two physical effects, it is shown that one can control the wave speed of bright and dark NLS solitons by appropriate modification of the dispersion and nonlinearity coefficients Luke . A challenging problem is the study of wave-speed management of solitons in the presence of higher-order effects, which come into play as pulse durations get shorter and peak powers increase. Also, a more significant issue is to examine the wave-speed management of various types of solitons under the contributions of these higher-order processes. As is known, in addition to the bright and dark soliton types, solitons could also display other complex shapes such as dipole and W-shaped structures. It is worth noting that dipole-mode solitons which are consisting of two peaks Susanto , have been recently observed in a three-level cascade atomic system where it has been experimentally demonstrated that the key to observe them is to create via Kerr nonlinearity, a high enough index contrast in the atomic medium by laser-induced index gratings Yanpeng . As concerns solitons that take the shape of W, these have been firstly presented in optical fibers described by the higher-order NLSE with third-order dispersion, self-steepening, and self-frequency shift effects in Zhoou . Up to the present time, the control of soliton wave speed in optical metamaterials supporting higher-order effects has not been reported to our knowledge. In this paper, we present the analysis of wave-speed management of dipole, bright and W-shaped solitons in an inhomogeneous optical metamaterial exhibiting not only the group velocity dispersion and self-phase-modulation, but also a rich variety higher-order effects. One should note that studying on the control of soliton wave speed is not only of scientific relevance but also of practical significance.

This paper is organized as follows. In Sec. II, we present the generalized higher-order NLSE that governs the few-cycle pulse propagation through a nonlinear metamaterial with higher-order nonlinear dispersion effects and derive its general traveling wave solution. New types of exact analytical periodic wave solutions that are composed of the product of pairs of Jacobi elliptic functions are derived in Sec III. Results for dipole soliton solutions is also presented here in the long-wave limit of periodic wave solutions. We also present the exact bright and W-shaped soliton solutions of the model equation. In Sec IV, we introduce the similarity transformation method for solving the generalized NLSE with varying coefficients. The application of developed method for the wave-speed management of dipole solitons is presented in Sec V. We also apply the developed technique to the management of bright and W-shaped solitons in Sec VI. Finally, in Sec. VII, we give some concluding remarks.

II Generalized NLSE for nonlinear metamaterials

The generalized NLSE describing the propagation of a few-cycle pulse in nonlinear metamaterials has the following form for the optical pulse envelope U(z,t)U(z,t) M1 ; M2 ; M3 ; M4 ; M5 ; M6 ; M7 ; M8 ; M9 ,

iUz+iα1Utα2Utt+γ|U|2U=iλ(|U|2U)t+iϵ(|U|2)tU+σ1(|U|2U)tt+σ2|U|2Utt+σ3U2Utt,iU_{z}+i\alpha_{1}U_{t}-\alpha_{2}U_{tt}+\gamma\left|U\right|^{2}U=i\lambda(\left|U\right|^{2}U)_{t}+i\epsilon(\left|U\right|^{2})_{t}U+\sigma_{1}(\left|U\right|^{2}U)_{tt}+\sigma_{2}\left|U\right|^{2}U_{tt}+\sigma_{3}U^{2}U_{tt}^{\ast}, (1)

where U(z,t)U(z,t) represents the complex envelope of the electrical field, zz and tt are the propagation distance and time, respectively, while the parameters α2,\alpha_{2}, γ,\gamma, α1,\alpha_{1}, λ,\lambda, and ϵ\epsilon represent the group velocity dispersion, cubic nonlinearity, intermodal dispersion, self-steepening, and nonlinear dispersion coefficients, respectively. Also, σi\sigma_{i} (with i=1,2,3i=1,2,3) are higher-order terms that appear in the context of metamaterials.

This equation has gathered significant attention recently for its importance from various physical view points M3 ; M4 ; M5 ; M6 ; M7 ; M8 . In particular, the existence of bright and dark soliton solutions of Eq. (1) have been recently investigated using different methods M1 ; M9 . Super-Gaussian envelope solitons M3 as well as singular solitons M4 have been also presented for this model. Here, we present the important results showing the wave-speed management of different types of solitons obtained within the generalized NLSE (1) framework. It will be demonstrated that these soliton modes can be deceleraed and accelerated through appropriate modification of the distributed parameters.

To start with, we consider the solution of generalized NLSE (1) in the form Kruglov1 ; Kruglov2 ,

U(z,t)=u(x)exp[i(κzδt+θ)],U(z,t)=u(x)\exp[i(\kappa z-\delta t+\theta)], (2)

where u(x)u(x) is a real amplitude function depending on the traveling coordinate x=tqzx=t-qz, and q=v1q=v^{-1} is the inverse velocity. Also, κ\kappa and δ\delta are the respective real parameters describing the wave number and frequency shift, while θ\theta represents the phase of pulse at z=0z=0.

On substitution of the waveform solution (2) into the model (1), one obtains the system of ordinary differential equations:

(q2α2δα1)dudx+[3λ+2ϵ2δ(3σ1+σ2σ3)]u2dudx=0,(q-2\alpha_{2}\delta-\alpha_{1})\frac{du}{dx}+\left[3\lambda+2\epsilon-2\delta\left(3\sigma_{1}+\sigma_{2}-\sigma_{3}\right)\right]u^{2}\frac{du}{dx}=0, (3)
α2d2udx2+(3σ1+σ2+σ3)u2d2udx2+6σ1u(dudx)2[γλδ+δ2(σ1+σ2+σ3)]u3+(κα1δα2δ2)u=0.\alpha_{2}\frac{d^{2}u}{dx^{2}}+(3\sigma_{1}+\sigma_{2}+\sigma_{3})u^{2}\frac{d^{2}u}{dx^{2}}+6\sigma_{1}u\left(\frac{du}{dx}\right)^{2}-\left[\gamma-\lambda\delta+\delta^{2}\left(\sigma_{1}+\sigma_{2}+\sigma_{3}\right)\right]u^{3}+(\kappa-\alpha_{1}\delta-\alpha_{2}\delta^{2})u=0. (4)

In the general case the system of Eqs. (3) and (4) is overdetermined because we have two differential equations for the function U(z,t)U(z,t). However, if some constraints for the parameters in Eq. (3) are fulfilled the system of Eqs. (3) and (4) has non-trivial solutions. From Eq. (3), one finds the relations:

q=α1+2α2δ,δ=3λ+2ϵ2(3σ1+σ2σ3).q=\alpha_{1}+2\alpha_{2}\delta,~{}~{}~{}~{}\delta=\frac{3\lambda+2\epsilon}{2\left(3\sigma_{1}+\sigma_{2}-\sigma_{3}\right)}. (5)

The latter relations lead to the following expression for the wave velocity v=1/qv=1/q,

v=3σ1+σ2σ3α1(3σ1+σ2σ3)+α2(3λ+2ϵ).v=\frac{3\sigma_{1}+\sigma_{2}-\sigma_{3}}{\alpha_{1}(3\sigma_{1}+\sigma_{2}-\sigma_{3})+\alpha_{2}(3\lambda+2\epsilon)}. (6)

Moreover, the relations in Eq. (5) reduce the system of Eqs. (3) and (4) to the ordinary nonlinear differential equation,

(α2+bu2)d2udx2+cu(dudx)2du3+Γu=0,(\alpha_{2}+bu^{2})\frac{d^{2}u}{dx^{2}}+cu\left(\frac{du}{dx}\right)^{2}-du^{3}+\Gamma u=0,~{}~{}~{}~{}~{}~{}~{} (7)

where the parameters a,a, b,b, cc and dd are given by

b\displaystyle b =\displaystyle= 3σ1+σ2+σ3,c=6σ1,\displaystyle 3\sigma_{1}+\sigma_{2}+\sigma_{3},~{}~{}~{}~{}~{}~{}~{}~{}c=6\sigma_{1}, (8a)
d\displaystyle d =\displaystyle= γ+(3λ+2ϵ)[2ϵ(σ1+σ2+σ3)+λ(5σ3+σ23σ1)]4(3σ1+σ2σ3)2,\displaystyle\gamma+\frac{(3\lambda+2\epsilon)\left[2\epsilon\left(\sigma_{1}+\sigma_{2}+\sigma_{3}\right)+\lambda(5\sigma_{3}+\sigma_{2}-3\sigma_{1})\right]}{4(3\sigma_{1}+\sigma_{2}-\sigma_{3})^{2}}, (8b)
Γ\displaystyle\Gamma =\displaystyle= κ(3λ+2ϵ)[2α1(3σ1+σ2σ3)+α2(3λ+2ϵ)]4(3σ1+σ2σ3)2.\displaystyle\kappa-\frac{(3\lambda+2\epsilon)\left[2\alpha_{1}\left(3\sigma_{1}+\sigma_{2}-\sigma_{3}\right)+\alpha_{2}(3\lambda+2\epsilon)\right]}{4(3\sigma_{1}+\sigma_{2}-\sigma_{3})^{2}}. (8c)
By analytically solving the amplitude equation (7), we can identify the various nonlinear waves that can propagate in the optical metamaterial described by the generalized NLSE (1). Noting that Eq. (7) can be written as
d2udx2+f(u)(dudx)2+g(u)=0,\frac{d^{2}u}{dx^{2}}+f(u)\left(\frac{du}{dx}\right)^{2}+g(u)=0, (9)

where the functions f(u)f(u) and g(u)g(u) are given by

f(u)=cubu2+α2,g(u)=u(Γdu2)bu2+α2.f(u)=\frac{cu}{bu^{2}+\alpha_{2}},~{}~{}~{}~{}g(u)=\frac{u(\Gamma-du^{2})}{bu^{2}+\alpha_{2}}. (10)

We introduce new function Y(u)Y(u) by equation,

dudx=Y(u).\frac{du}{dx}=Y(u). (11)

Thus, Eq. (9) for new function Y(u)Y(u) has the following form,

dYdu+f(u)Y+g(u)Y1=0.\frac{dY}{du}+f(u)Y+g(u)Y^{-1}=0. (12)

Now let us define the function F(u)F(u) by relation,

F(u)=Y2(u),F(u)=Y^{2}(u), (13)

then the equation for new function FF is

dFdu+2f(u)F+2g(u)=0.\frac{dF}{du}+2f(u)F+2g(u)=0. (14)

The general solution of this equation has the form,

F(u)=F0eG(u)2eG(u)u0ug(u)eG(u)𝑑u,F(u)=F_{0}e^{-G(u)}-2e^{-G(u)}\int_{u_{0}}^{u}g(u^{\prime})e^{G(u^{\prime})}du^{\prime}, (15)

where the function G(u)G(u) is defined as

G(u)=2u0uf(u)𝑑u.G(u)=2\int_{u_{0}}^{u}f(u^{\prime})du^{\prime}. (16)

We note the solution in Eq. (15) satisfies to the boundary condition as F(u0)=F0F(u_{0})=F_{0}. In addition, the function G(u)G(u) has the following explicit form,

G(u)=2cu0uudubu2+α2=cbln|bu2+α2||bu02+α2|.G(u)=2c\int_{u_{0}}^{u}\frac{u^{\prime}du^{\prime}}{bu^{\prime 2}+\alpha_{2}}=\frac{c}{b}\ln\frac{|bu^{2}+\alpha_{2}|}{|bu_{0}^{2}+\alpha_{2}|}. (17)

Also, Eqs. (11) and (13) yield the differential equation: dx=±du/F(u)dx=\pm du/\sqrt{F(u)}. Thus, we find that the general solution of Eq. (7) takes the form,

xx0=±u0uduF(u),x-x_{0}=\pm\int_{u_{0}}^{u}\frac{du^{\prime}}{\sqrt{F(u^{\prime})}}, (18)

where the function F(u)F(u) is defined by Eq. (15).

The general solution of Eq. (7) can also be written in the form: x=x0±[R(u)R(u0)]x=x_{0}\pm[R(u)-R(u_{0})] with R(u)=F1/2(u)𝑑uR(u)=\int F^{-1/2}(u)du. This solution defines the variable xx as a function of the amplitude uu. Hence, we have the boundary condition: x=x0x=x_{0} at u=u0u=u_{0} or u(x0)=u0u(x_{0})=u_{0}. This general solution leads to many different particular solutions when we define some constrains to the coefficients of NLSE given in Eq. (1). In what follows, the different classes of periodic (elliptic) waves are shown to exist in the presence of all physical processes. Such kind of waves serves as a model of pulse train propagation in optical systems CDai . Moreover, results for dipole, bright and W-shaped soliton solutions are also obtained for the governing envelope equation.

III Periodic and soliton solutions

III.1 Periodic waves

We have found that Eq. (7) possesses an exact solution that is composed of the product of periodic elliptic functions,

u(x)=±Rdn(w(xη),k)sn(w(xη),k),u(x)=\pm R\,\mathit{\mathrm{dn}}(w(x-\eta),k)\,\mathit{\mathrm{s}}\mathrm{n}(w(x-\eta),k), (19)

where η\eta is an arbitrary constant while dn(ζ,k)\mathrm{dn}(\zeta,k) and sn(ζ,k)\mathit{\mathrm{sn}}(\zeta,k) are Jacobi elliptic functions of modulus kk with 0<k<1.0<k<1\mathrm{.} The real parameters RR and ww in this solution are defined by the expressions:

R=4α2k2b,w=db(2k21).R=\sqrt{-\frac{4\alpha_{2}k^{2}}{b}},\quad w=\sqrt{\frac{d}{b(2k^{2}-1)}}. (20)

We assume here the constraint as σ1=(σ2+σ3)/7\sigma_{1}=-(\sigma_{2}+\sigma_{3})/7. Further, we obtain the parameter κ\kappa:

κ=α2db+(3λ+2ϵ)[2α1(3σ1+σ2σ3)+α2(3λ+2ϵ)]4(3σ1+σ2σ3)2.\kappa=-\frac{\alpha_{2}d}{b}+\frac{(3\lambda+2\epsilon)\left[2\alpha_{1}\left(3\sigma_{1}+\sigma_{2}-\sigma_{3}\right)+\alpha_{2}(3\lambda+2\epsilon)\right]}{4(3\sigma_{1}+\sigma_{2}-\sigma_{3})^{2}}. (21)

Relations (20) indicate that the necessary conditions for this solution to exist are bd>0bd>0 for 1/2<k<11/\sqrt{2}<k<1; and bd<0bd<0 for 0<k<1/20<k<1/\sqrt{2} and α2b<0\alpha_{2}b<0.

If we insert the solution (19) into Eq. (2), we obtain a class of periodic wave solutions for the NLSE model (1) of the form,

U(z,t)=±Rdn(wξ,k)sn(wξ,k)exp[i(κzδt+θ)],U(z,t)=\pm R\,\mathit{\mathrm{dn}}(w\xi,k)\,\mathit{\mathrm{s}}\mathrm{n}(w\xi,k)\exp[i(\kappa z-\delta t+\theta)], (22)

where ξ=tqzη\xi=t-qz-\eta with η\eta is the position of wave at z=0z=0.

We obtained another periodic solution for Eq. (7) that is expressed by the product of periodic elliptic functions,

u(x)=±Scn(p(xη),k)sn(p(xη),k),u(x)=\pm S\,\mathit{\mathrm{cn}}(p(x-\eta),k)\,\mathit{\mathrm{s}}\mathrm{n}(p(x-\eta),k), (23)

where cn(ζ,k)\mathit{\mathrm{cn}}(\zeta,k) is Jacobi elliptic function of modulus kk with 0<k<10<k<1. The real parameters SS and pp in this solution are given by

S=4α2b,p=db(2k2).S=\sqrt{-\frac{4\alpha_{2}}{b}},\quad p=\sqrt{\frac{d}{b(2-k^{2})}}. (24)

We also assume here the constraint as σ1=(σ2+σ3)/7\sigma_{1}=-(\sigma_{2}+\sigma_{3})/7. Moreover, we obtain the parameter κ\kappa:

κ=α2db+(3λ+2ϵ)[2α1(3σ1+σ2σ3)+α2(3λ+2ϵ)]4(3σ1+σ2σ3)2.\kappa=-\frac{\alpha_{2}d}{b}+\frac{(3\lambda+2\epsilon)\left[2\alpha_{1}\left(3\sigma_{1}+\sigma_{2}-\sigma_{3}\right)+\alpha_{2}(3\lambda+2\epsilon)\right]}{4(3\sigma_{1}+\sigma_{2}-\sigma_{3})^{2}}. (25)

Substitution of (23) into (2) yields to the following exact periodic wave solution of Eq. (1),

U(z,t)=±Scn(pξ,k)sn(pξ,k)exp[i(κzδt+θ)],U(z,t)=\pm S\,\mathit{\mathrm{cn}}(p\xi,k)\,\mathit{\mathrm{s}}\mathrm{n}(p\xi,k)\exp[i(\kappa z-\delta t+\theta)], (26)

where ξ\xi is the same as above. From Eq. (24), we see that this periodic solution exists when the following inequalities are satisfied: α2b<0\alpha_{2}b<0 and bd>0bd>0.

We also obtained the periodic solution for Eq. (7) that is expressed by the product of periodic functions as

u(x)=±Dcn(h(xη),k)dn(h(xη),k),u(x)=\pm D\,\mathit{\mathrm{cn}}(h(x-\eta),k)\,\mathit{\mathrm{d}}\mathrm{n}(h(x-\eta),k), (27)

The real parameters DD and hh in this solution are given by

D=4α2k2b(1k2)2,h=db(1+k2).D=\sqrt{\frac{4\alpha_{2}k^{2}}{b(1-k^{2})^{2}}},\quad h=\sqrt{-\frac{d}{b(1+k^{2})}}. (28)

We also assume here the constraint as σ1=(σ2+σ3)/7\sigma_{1}=-(\sigma_{2}+\sigma_{3})/7. Moreover, we obtain the parameter κ\kappa:

κ=α2db+(3λ+2ϵ)[2α1(3σ1+σ2σ3)+α2(3λ+2ϵ)]4(3σ1+σ2σ3)2.\kappa=-\frac{\alpha_{2}d}{b}+\frac{(3\lambda+2\epsilon)\left[2\alpha_{1}\left(3\sigma_{1}+\sigma_{2}-\sigma_{3}\right)+\alpha_{2}(3\lambda+2\epsilon)\right]}{4(3\sigma_{1}+\sigma_{2}-\sigma_{3})^{2}}. (29)

Substitution of (27) into (2) yields to the following exact periodic wave solution of Eq. (1),

U(z,t)=±Dcn(hξ,k)dn(hξ,k)exp[i(κzδt+θ)],U(z,t)=\pm D\,\mathit{\mathrm{cn}}(h\xi,k)\,\mathit{\mathrm{d}}\mathrm{n}(h\xi,k)\exp[i(\kappa z-\delta t+\theta)], (30)

where ξ\xi is the same as above. From Eq. (28), we see that this periodic solution exists when the following inequalities are satisfied: α2b>0\alpha_{2}b>0 and bd<0bd<0.

III.2 Dipole solitons

Considering the long-wave limit k1k\rightarrow 1, the periodic solutions (22) degenerates to a dipole-type soliton solution of the form,

U(z,t)=±R0sech(w0ξ)th(w0ξ)exp[i(κzδt+θ)],U(z,t)=\pm R_{0}~{}\mathrm{sech}(w_{0}\xi)~{}\mathrm{th}(w_{0}\xi)\exp[i(\kappa z-\delta t+\theta)], (31)

under the parametric condition as σ1=(σ2+σ3)/7.\sigma_{1}=-(\sigma_{2}+\sigma_{3})/7. The soliton amplitude R0R_{0} and the inverse width w0w_{0} are given by

R0=4α2b,w0=db,R_{0}=\sqrt{-\frac{4\alpha_{2}}{b}},\quad w_{0}=\sqrt{\frac{d}{b}}, (32)

while the wave number κ\kappa takes the same relation (21). Notice that when k1,k\rightarrow 1, the periodic wave solution (26) also degenerates to the same soliton-type solution (31). It follows from Eq. (32) that this dipole soliton exists when the next two conditions are satisfied: bα2<0b\alpha_{2}<0 and bd>0bd>0.

For this class of dipole solitons, the energy EE is given by

E=+|U(z,t)|2𝑑t=8|α2|3|b|w0.E=\int_{-\infty}^{+\infty}|U(z,t)|^{2}dt=\frac{8|\alpha_{2}|}{3|b|w_{0}}. (33)

Notice that the pulse energy EE is the integral of motion [dE/dz=0dE/dz=0] of the generalized NLSE (1) for any optical pulses satisfying the boundary condition: U(z,t)0U(z,t)\rightarrow 0 for t±t\rightarrow\pm\infty. An important observation here is that the energy of dipole solitons depends on all system parameters which are included in the coefficients bb and dd. This enable us to change the soliton energy by appropriate manipulation of the metamaterial parameters.

III.3 Bright solitons

We also find that Eq. (1) yields a bright soliton solution of the form,

U(z,t)=Λ0sech2(w0ξ)exp[i(κzδt+θ)],U(z,t)=\Lambda_{0}~{}\mathrm{sech}^{2}(w_{0}\xi)\exp[i(\kappa z-\delta t+\theta)], (34)

under the parametric conditions as α2=0\alpha_{2}=0 and σ1=(σ2+σ3)/7.\sigma_{1}=-(\sigma_{2}+\sigma_{3})/7. The amplitude Λ0\Lambda_{0} of this soliton solution is a free real parameter while its inverse width and wave number parameters w0w_{0} and κ\kappa are given as

w0=d2b,κ=α1(3λ+2ϵ)2(3σ1+σ2σ3),w_{0}=\sqrt{-\frac{d}{2b}},\quad\kappa=\frac{\alpha_{1}(3\lambda+2\epsilon)}{2(3\sigma_{1}+\sigma_{2}-\sigma_{3})}, (35)

with the condition db<0db<0. Moreover, the corresponding energy EE of this bright soliton reads

E=+|U(z,t)|2𝑑t=4Λ023w0.E=\int_{-\infty}^{+\infty}|U(z,t)|^{2}dt=\frac{4\Lambda_{0}^{2}}{3w_{0}}. (36)

III.4 W-shaped solitons

In addition, we obtained a W-shaped soliton solution of Eq. (1) as follows:

U(z,t)=B0(132sech2(w0ξ))exp[i(κzδt+θ)],U(z,t)=B_{0}\left(1-\frac{3}{2}\mathrm{sech}^{2}(w_{0}\xi)\right)\exp[i(\kappa z-\delta t+\theta)], (37)

which takes place for the conditions: α2=0\alpha_{2}=0 and σ1=(σ2+σ3)/7\sigma_{1}=-(\sigma_{2}+\sigma_{3})/7. The amplitude B0B_{0} of this waveform is a free real parameter while the inverse width parameter w0w_{0} reads

w0=d2b,w_{0}=\sqrt{\frac{d}{2b}}, (38)

with the condition db>0db>0. The parameter κ\kappa for this W-shaped soliton solution is

κ=dB02+α1(3λ+2ϵ)2(3σ1+σ2σ3).\kappa=dB_{0}^{2}+\frac{\alpha_{1}(3\lambda+2\epsilon)}{2(3\sigma_{1}+\sigma_{2}-\sigma_{3})}. (39)
Refer to caption
Figure 1: Evolution of the soliton solutions with parameters σ1=0.08,\sigma_{1}=-0.08, σ2=0.5,\sigma_{2}=0.5, and σ3=0.06\sigma_{3}=0.06 (a) dipole soliton (31) when α1=1.35,\alpha_{1}=1.35, α2=0.25,\alpha_{2}=-0.25, γ=2,\gamma=-2, λ=0.25,\lambda=0.25, ϵ=0.125,\epsilon=0.125, η=0\eta=0 (b) bright soliton (34) γ=1.4075,\gamma=-1.4075, α1=0.1,\alpha_{1}=0.1, λ=0.125,\lambda=0.125, ϵ=0.25,\epsilon=-0.25, η=0,\eta=0, Λ0=1\Lambda_{0}=1 (b) W-shaped soliton (37) when γ=2,\gamma=-2, α1=0.1,\alpha_{1}=0.1, λ=0.25,\lambda=0.25, ϵ=0.125,\epsilon=0.125, η=0,\eta=0, B0=1B_{0}=1.

Figures 1(a), 1(b) and 1(c) depict the the evolution of the intensity profiles of dipole, bright and W-shaped solitons (31), (34) and (37) for the parameter values σ1=0.08,\sigma_{1}=-0.08, σ2=0.5,\sigma_{2}=0.5, and σ3=0.06\sigma_{3}=0.06. The other parameters are taken as α1=1.35,\alpha_{1}=1.35, α2=0.25,\alpha_{2}=-0.25, γ=2,\gamma=-2, λ=0.25,\lambda=0.25, ϵ=0.125\epsilon=0.125 for solution (31), γ=1.4075,\gamma=-1.4075, α1=0.1,\alpha_{1}=0.1, λ=0.125,\lambda=0.125, ϵ=0.25,\epsilon=-0.25, Λ0=1\Lambda_{0}=1 for solution (34), and γ=2,\gamma=-2, α1=0.1,\alpha_{1}=0.1, λ=0.25,\lambda=0.25, ϵ=0.125,\epsilon=0.125, B0=1B_{0}=1 for solution (37). Also, we choose the position η\eta of pulses at z=0z=0 to be equal to 0.0.  From these figures, we observe that the soliton profiles remain unchanged during evolution.

IV Method of solving generalized NLSE with variable coefficients

A natural situation would be to consider the inhomogeneities of media in describing more realistic phenomena. The presence of such inhomogeneities modifies the propagation dynamics of nonlinear waves since in this case, the system parameters become functions of the propagation distance. Thus, the ultrashort light pulse transmission in a realistic nonlinear metamaterial can be described by the generalized NLSE with varied coefficients:

iψz+iD1(z)ψtD2(z)ψtt+R(z)|ψ|2ψ=iρ(z)(|ψ|2ψ)t+if(z)(|ψ|2)tψ+χ1(z)(|ψ|2ψ)tt+χ2(z)|ψ|2ψtt+χ3(z)ψ2ψtt.i\psi_{z}+iD_{1}(z)\psi_{t}-D_{2}(z)\psi_{tt}+R(z)\left|\psi\right|^{2}\psi=i\rho(z)(\left|\psi\right|^{2}\psi)_{t}+if(z)(\left|\psi\right|^{2})_{t}\psi+\chi_{1}(z)(\left|\psi\right|^{2}\psi)_{tt}+\chi_{2}(z)\left|\psi\right|^{2}\psi_{tt}+\chi_{3}(z)\psi^{2}\psi_{tt}^{\ast}. (40)

where D1(z),D_{1}(z), D2(z),D_{2}(z), R(z),R(z), ρ(z)\rho(z) and f(z)f(z) are the variable intermodal dispersion, group velocity dispersion, Kerr nonlinearity, self-steepening, and nonlinear dispersion coefficients, respectively. The functions χi(z)\chi_{i}(z) for i=1,2,3i=1,2,3 stand for the varying higher-order nonlinear dispersion coefficients.

Equation (1) is an important generalization of the model (1) which may be useful for further understanding of the general behavior of the realistic system. In what follows, we introduce a powerful similarity transformation method which enables us to study the soliton dynamics in a real optical metamaterial described by Eq. (40). One notes that studying the control and manipulation of the soliton pulses within the framework of variable-coefficient NLSE models may help to manage them experimentally not only in inhomogeneous nonlinear metamaterials but also in optical fibers and Bose-Einstein condensates where the NLS family of equations can be also applied to describe the field dynamics.

To obtain the exact analytical solutions for Eq. (40), we developed the method based on the following form of the wave function ψ(z,t)\psi(z,t):

ψ(z,t)=u(y)exp[i(κZ(z)δT(z,t)+θ)],\psi(z,t)=u(y)\exp[i(\kappa Z(z)-\delta T(z,t)+\theta)], (41)
y=T(z,t)qZ(z),q=α1+2α2δ,y=T(z,t)-qZ(z),~{}~{}~{}~{}q=\alpha_{1}+2\alpha_{2}\delta, (42)

where T(z,t)T\left(z,t\right) and Z(z)Z\left(z\right) are two functions to be determined and the frequency shift δ\delta is given in Eq. (5). It is important that we present here the function T(z,t)T\left(z,t\right) and variable yy in the special form as

T(z,t)=t+P(z),y=t[qZ(z)P(z)].T(z,t)=t+P(z),~{}~{}~{}~{}y=t-[qZ(z)-P(z)]. (43)

Moreover, we require that the wave function ψ(z,t)\psi(z,t) in (41) coincides with the wave function U(z,t)U(z,t) in (2) for z=0z=0. This initial condition for the wave functions ψ(z,t)\psi(z,t) and U(z,t)U(z,t) yields the following initial conditions for the functions Z(z)Z(z) and T(z,t)T(z,t): Z(0)=0Z(0)=0 and T(0,t)=tT(0,t)=t. Hence, using the expressions in Eq. (43) we have the initial conditions for the functions Z(z)Z(z) and P(z)P(z): Z(0)=0Z(0)=0 and P(0)=0P(0)=0.

Substitution of the expressions (41) and (43) into Eq. (40) leads to the following equations:

(PqZ+D1+2δD2)dudy=[3ρ+2f2δ(3χ1+χ2χ3)]u2dudy,(P^{\prime}-qZ^{\prime}+D_{1}+2\delta D_{2})\frac{du}{dy}=\left[3\rho+2f-2\delta\left(3\chi_{1}+\chi_{2}-\chi_{3}\right)\right]u^{2}\frac{du}{dy}, (44)
D2d2udy2+(3χ1+χ2+χ3)u2d2udy2+6χ1u(dudy)2[Rρδ+δ2(χ1+χ2+χ3)]u3+(κZδPδD1δ2D2)u=0,D_{2}\frac{d^{2}u}{dy^{2}}+(3\chi_{1}+\chi_{2}+\chi_{3})u^{2}\frac{d^{2}u}{dy^{2}}+6\chi_{1}u\left(\frac{du}{dy}\right)^{2}-\left[R-\rho\delta+\delta^{2}\left(\chi_{1}+\chi_{2}+\chi_{3}\right)\right]u^{3}+(\kappa Z^{\prime}-\delta P^{\prime}-\delta D_{1}-\delta^{2}D_{2})u=0, (45)

where P=dP/dzP^{\prime}=dP/dz and Z=dZ/dzZ^{\prime}=dZ/dz. Eq. (44) is satisfied when the following relations are accepted:

dPdzqdZdz+D1+2δD2=0,\frac{dP}{dz}-q\frac{dZ}{dz}+D_{1}+2\delta D_{2}=0, (46)
3ρ+2f2δ(3χ1+χ2χ3)=0.3\rho+2f-2\delta\left(3\chi_{1}+\chi_{2}-\chi_{3}\right)=0. (47)

Now we perform the important transformation in Eq. (45) using the following change of the variable: yxy\mapsto x. This mapping also yields the change of function in (45) as u(y)u(x)u(y)\mapsto u(x). One can see that above mapping does not change the form of function uu. Moreover, Eq. (45) is equivalent to Eq. (4) when the above mapping of variable is performed (yxy\mapsto x) and the following equations are satisfied:

3χ1+χ2+χ3D2=3σ1+σ2+σ3α2,χ1D2=σ1α2,\frac{3\chi_{1}+\chi_{2}+\chi_{3}}{D_{2}}=\frac{3\sigma_{1}+\sigma_{2}+\sigma_{3}}{\alpha_{2}},~{}~{}~{}~{}\frac{\chi_{1}}{D_{2}}=\frac{\sigma_{1}}{\alpha_{2}}, (48)
Rρδ+δ2(χ1+χ2+χ3)D2=γλδ+δ2(σ1+σ2+σ3)α2,\frac{R-\rho\delta+\delta^{2}\left(\chi_{1}+\chi_{2}+\chi_{3}\right)}{D_{2}}=\frac{\gamma-\lambda\delta+\delta^{2}\left(\sigma_{1}+\sigma_{2}+\sigma_{3}\right)}{\alpha_{2}}, (49)
1D2(κdZdzδdPdzδD1δ2D2)=κα1δα2δ2α2.\frac{1}{D_{2}}\left(\kappa\frac{dZ}{dz}-\delta\frac{dP}{dz}-\delta D_{1}-\delta^{2}D_{2}\right)=\frac{\kappa-\alpha_{1}\delta-\alpha_{2}\delta^{2}}{\alpha_{2}}. (50)

By solving Eqs. (46-50) with the initial conditions Z(0)=0Z(0)=0 and P(0)=0P(0)=0 self-consistently, we obtain the following results that define the mapping variables:

P(z)=α1α20zD2(s)𝑑s0zD1(s)𝑑s,Z(z)=1α20zD2(s)𝑑s,\displaystyle\left.P(z)=\frac{\alpha_{1}}{\alpha_{2}}\int_{0}^{z}D_{2}(s)ds-\int_{0}^{z}D_{1}(s)ds,\quad Z(z)=\frac{1}{\alpha_{2}}\int_{0}^{z}D_{2}(s)ds,\right. (51)
R(z)=γα2D2(z),ρ(z)=λα2D2(z),f(z)=ϵα2D2(z),\displaystyle\left.R(z)=\frac{\gamma}{\alpha_{2}}D_{2}(z),\quad\rho(z)=\frac{\lambda}{\alpha_{2}}D_{2}(z),\quad f(z)=\frac{\epsilon}{\alpha_{2}}D_{2}(z),\right. (52)
χ1(z)=σ1α2D2(z),χ2(z)=σ2α2D2(z),χ3(z)=σ3α2D2(z),\displaystyle\left.\chi_{1}(z)=\frac{\sigma_{1}}{\alpha_{2}}D_{2}(z),\quad\chi_{2}(z)=\frac{\sigma_{2}}{\alpha_{2}}D_{2}(z),\quad\chi_{3}(z)=\frac{\sigma_{3}}{\alpha_{2}}D_{2}(z),\right. (53)

Thus, all varying parameters in Eq. (40) completely defined by arbitrary function D2(z)D_{2}(z) via the constraints given in Eqs. (52) and (53). We also have found that the function T(z,t)T(z,t) and variable yy have the form,

T(z,t)=t+α1α20zD2(s)𝑑s0zD1(s)𝑑s,T(z,t)=t+\frac{\alpha_{1}}{\alpha_{2}}\int_{0}^{z}D_{2}(s)ds-\int_{0}^{z}D_{1}(s)ds, (54)
y=t0zD1(s)𝑑s2δ0zD2(s)𝑑s.y=t-\int_{0}^{z}D_{1}(s)ds-2\delta\int_{0}^{z}D_{2}(s)ds. (55)

Hence, the dynamics of solitons depends on two arbitrary functions as D1(z)D_{1}(z) and D2(z)D_{2}(z). Incorporating these results into Eq. (41), we obtain the general self-similar wave solutions to the generalized NLSE with distributed coefficients (40) as

ψ(z,t)=u(tζ(z))exp[i(κZ(z)δT(z,t)+θ)],\psi(z,t)=u(t-\zeta(z))\exp[i(\kappa Z(z)-\delta T(z,t)+\theta)], (56)

where

ζ(z)=0zD1(s)𝑑s+2δ0zD2(s)𝑑s,\zeta(z)=\int_{0}^{z}D_{1}(s)ds+2\delta\int_{0}^{z}D_{2}(s)ds, (57)

and parameter δ\delta is given here in Eq. (5). Thus, one can construct exact self-similar solutions to Eq. (40) by using the exact solutions of Eq. (1) via the transformation (56). It is worth noting that the existence of general self-similar solution (56) depends on the specific nonlinear and dispersive features of the medium, which have to satisfy the parametric conditions (52) and (53). These conditions present the exact balances among dispersive and nonlinear processes of different nature.

The equation for velocity of solitons follows from Eq. (56) which yields the relation dt=(dζ/dz)dzdt=(d\zeta/dz)dz. Thus, the velocity of solitons V(z)=dz/dtV(z)=dz/dt has the form,

V(z)=(dζ(z)dz)1=1D1(z)+2δD2(z).V(z)=\left(\frac{d\zeta(z)}{dz}\right)^{-1}=\frac{1}{D_{1}(z)+2\delta D_{2}(z)}. (58)

We emphasize that the solutions described by Eqs. (56), (57) and (51-(55) are satisfied to appropriate boundary conditions. The substitution into Eqs. (51-53) the limiting boundary conditions D1(z)=α1D_{1}(z)=\alpha_{1} and D2(z)=α2D_{2}(z)=\alpha_{2} yield the following relations: P(z)=0P(z)=0, Z(z)=zZ(z)=z, R(z)=γR(z)=\gamma, ρ(z)=λ\rho(z)=\lambda, f(z)=ϵf(z)=\epsilon, χ1(z)=σ1\chi_{1}(z)=\sigma_{1}, χ2(z)=σ2\chi_{2}(z)=\sigma_{2}, χ3(z)=σ3\chi_{3}(z)=\sigma_{3} which transform NLSE (40) into generalized NLSE (1). Moreover, in this case we have Z(z)=zZ(z)=z, T(z,t)=tT(z,t)=t and ζ(z)=(α1+2α2δ)z=qz\zeta(z)=(\alpha_{1}+2\alpha_{2}\delta)z=qz which leads the wave function in (56) to the form,

ψ(z,t)=u(tqz)exp[i(κzδt+θ)].\psi(z,t)=u(t-qz)\exp[i(\kappa z-\delta t+\theta)]. (59)

Hence, in this limiting case we have ψ(z,t)=U(z,t)\psi(z,t)=U(z,t) where the wave function U(z,t)U(z,t) is defined in (2), and the velocity in (58) is V(z)=1/q=vV(z)=1/q=v. Note that from this limiting case we have the relation ψ(0,t)=U(0,t)\psi(0,t)=U(0,t) which is connected with our initial conditions as Z(0)=0Z(0)=0 and P(0)=0P(0)=0.

We also note that the developed method of solving the generalized NLSE with variable coefficients is applied here to Eq. (40). However, this general method can be used for solving an arbitrary NLSE with variable coefficients. We emphasize that this method for solving the generalized NLSE with variable coefficients is significantly differ from the mapping given in the previous papers Kruglov3 ; Kruglov4 ; Dai2 ; Krug3 .

V Wave-speed management of dipole solitons

Having obtained the general self-similar solution (56) of the physically relevant model (40), we now analyze the problem of wave-speed management of soliton pulses by considering important spatial modulation of metamaterial parameters. In particular, we will study the deceleration (i.e., the slowing) and acceleration motions of the dipole soliton pulse as it propagates through the optical metamaterial.

To start with, we first construct the exact self-similar soliton solutions of the generalized NLSE with distributed coefficients (40). Substitution of the solution (31) into Eq. (56) leads to a family of exact self-similar dipole soliton solution for Eq. (40) of the form,

ψ(z,t)=±R0sech(w0τ(z,t))th(w0τ(z,t))exp[i(κZ(z)δT(z,t)+θ)],\psi(z,t)=\pm R_{0}~{}\mathrm{sech}\left(w_{0}\tau(z,t)\right)\mathrm{th}\left(w_{0}\tau(z,t)\right)\exp[i(\kappa Z(z)-\delta T(z,t)+\theta)], (60)

where τ(z,t)=tζ(z)η\tau(z,t)=t-\zeta(z)-\eta. Here the amplitude R0R_{0} and inverse width w0w_{0} are given in (32) and the wave number κ\kappa in (22) with the parametric condition as σ1=(σ2+σ3)/7\sigma_{1}=-(\sigma_{2}+\sigma_{3})/7.

Expression (60) shows that the amplitude and inverse width of dipole solitons remain constants as they propagate through the metamaterial while their velocity V(z)V(z), given by Eq. (58), is affected by the varying dispersion coefficients D1(z)D_{1}(z) and D2(z).D_{2}(z). This may lead to the decelerating or accelerating soliton motions by suitable variations of these parameters. Below, we analyze the deceleration and acceleration processes of dipole solitons by managing the distributed parameters D1(z)D_{1}(z) and D2(z)D_{2}(z).

V.1 Deceleration of a dipole soliton

To illustrate the wave-speed management of the obtained self-similar dipole soliton solution (60), we consider as example an exponential distributed control system with a spatial modulation of D1(z)D_{1}(z) and D2(z)D_{2}(z) in the form,

D1(z)=g0+g1exp(mz),D_{1}(z)=g_{0}+g_{1}\exp(mz), (61)
D2(z)=d0+d1exp(nz),D_{2}(z)=d_{0}+d_{1}\exp(nz), (62)

where d0,d_{0}, d1,d_{1}, g0,g_{0}, g1g_{1} and mm, nn are real constants. Here, the parameters mm and nn can be utilized for adjusting the rate of slowing soliton. The other parameters of the metamaterial can be obtained exactly through Eqs. (51), (52) and (53). Consequently, the function ζ(z)\zeta(z) given in Eq. (57) can be derived as

ζ(z)=(g0+2δd0)z+g1m(emz1)+2δd1n(enz1)\zeta(z)=(g_{0}+2\delta d_{0})z+\frac{g_{1}}{m}\left(e^{mz}-1\right)+\frac{2\delta d_{1}}{n}\left(e^{nz}-1\right) (63)

It follows from Eq. (58) that slowing of dipole soliton can be achieved when V(z)1/qV(z)\ll 1/q or D1(z)+2δD2(z)qD_{1}(z)+2\delta D_{2}(z)\gg q.

Refer to caption
Figure 2: Intensity distribution of (a)-(b) the dipole soliton (60) for D1(z)D_{1}(z) and D2(z)D_{2}(z) given by Eqs. (61) and (62). The parameters are g0=0.5,g_{0}=0.5, g1=1.5,g_{1}=1.5, d0=0.1,d_{0}=0.1, d1=0.48,d_{1}=0.48, m=0.5,m=-0.5, n=0.48,n=-0.48, and η=0\eta=0. The other parameters are the same as in Fig. 1(a).

Figure 2 depicts the propagation dynamics of the dipole soliton (60) in the presence of spatial dependent dispersions D1(z)D_{1}(z) and D2(z)D_{2}(z) given by Eqs. (61) and (62) for the parameter values g0=0.5,g_{0}=0.5, g1=1.5,g_{1}=1.5, d0=0.1,d_{0}=0.1, d1=0.48,d_{1}=0.48, m=0.5,m=-0.5, n=0.48,n=-0.48, and η=0\eta=0. The other parameters are chosen as those in Fig. 1(a). One can clearly see that through this spatial variation of D1(z)D_{1}(z) and D2(z)D_{2}(z), the soliton structure can be slowed as it propagates in the optical metamaterial. It can be also observed that neither the soliton amplitude nor width change during the propagation.

V.2 Acceleration of a dipole soliton

To accelerate the motion of obtained dipole soliton, we select the parameters D1(z)D_{1}(z) and D2(z)D_{2}(z) to vary periodically along the propagation direction inside the system as,

D1(z)=gzacos(az2)gz3sin(az2),D_{1}(z)=\frac{gz}{a}\cos(az^{2})-gz^{3}\sin(az^{2}), (64)
D2(z)=d0+d1cos(bz),D_{2}(z)=d_{0}+d_{1}\cos(bz), (65)

where g,g, d0d_{0}, d1d_{1}, aa and bb are constants. The other metamaterial parameters can be calculated by using Eqs. (51), (52) and (53). In this case, the function ζ(z)\zeta(z) can be obtained using Eq. (57) as

ζ(z)=12agz2cos(az2)+2δ[d0z+d1bsin(bz)].\zeta(z)=\frac{1}{2a}gz^{2}\cos(az^{2})+2\delta\left[d_{0}z+\frac{d_{1}}{b}\sin(bz)\right]. (66)
Refer to caption
Figure 3: Intensity distribution of (a)-(b) the dipole soliton (60) for D1(z)D_{1}(z) and D2(z)D_{2}(z) given by Eqs. (64) and (65). The parameters are g=0.3,g=-0.3, d0=0.02,d_{0}\,=-0.02, d1=1,d_{1}=1, a=1a=1, b=1b=1 and η=0\eta=0. The other parameters are the same as in Fig. 1(a).

We present the propagation dynamics of the dipole soliton (60) with the distributed parameters D1(z)D_{1}(z) and D2(z)D_{2}(z) given by Eqs. (64) and (65) in Fig. 3 with g=0.3,g=-0.3, d0=0.02,d_{0}\,=-0.02, d1=1,d_{1}=1, a=1a=1, b=1b=1, and η=0\eta=0. The other parameters are chosen as in Fig. 1(a). We observe that the dipole soliton displays an accelerating behavior as it propagates through the optical metamaterial.

VI Wave-speed management of bright and W-shaped solitons

Now we turn our attention to discuss the wave-speed management of bright and W-shaped soliton solutions of the variable-coefficient NLSE (40) by designing appropriate metamaterial parameters. On should note here that these self-similar wave solutions take place when the constant and variable parameters of group velocity dispersion vanish (namely, D2(z)=0D_{2}(z)=0 and α2=0)\alpha_{2}=0). We can find appropriate transformation given in Eqs. (41) and (43) using the found mapping relations in Eqs.(51-55). In this case we make in NLSE (40) and other equations the change D2(z)α2D_{2}(z)\mapsto\alpha_{2} and after the limit α20\alpha_{2}\rightarrow 0. Thus, we have the following mapping in (40): R(z)=γR(z)=\gamma, ρ(z)=λ\rho(z)=\lambda, f(z)=ϵf(z)=\epsilon, χ1(z)=σ1\chi_{1}(z)=\sigma_{1}, χ2(z)=σ2\chi_{2}(z)=\sigma_{2}, χ3(z)=σ3\chi_{3}(z)=\sigma_{3}, and Eqs. (51) and (54) yield

P(z)=α1z0zD1(s)𝑑s,P(z)=\alpha_{1}z-\int_{0}^{z}D_{1}(s)ds, (67)
Z(z)=z,T(z,t)=t+α1z0zD1(s)𝑑s.Z(z)=z,\quad T(z,t)=t+\alpha_{1}z-\int_{0}^{z}D_{1}(s)ds. (68)

We also have the relation ζ(z)=α1zP(z)\zeta(z)=\alpha_{1}z-P(z) which leads to equations,

ζ(z)=0zD1(s)𝑑s,V(z)=(dζ(z)dz)1=1D1(z).\zeta(z)=\int_{0}^{z}D_{1}(s)ds,\quad V(z)=\left(\frac{d\zeta(z)}{dz}\right)^{-1}=\frac{1}{D_{1}(z)}. (69)

Moreover, in this case we have the relation Z(z)=zZ(z)=z, which reduces Eq. (56) to the form,

ψ(z,t)=u(tζ(z))exp[i(κzδT(z,t)+θ)].\psi(z,t)=u(t-\zeta(z))\exp[i(\kappa z-\delta T(z,t)+\theta)]. (70)

Thus, using the solution (34) and the transformation (70) we can write the self-similar bright soliton solution of Eq. (40) as

ψ(z,t)=Λ0sech2(w0τ(z,t))exp[i(κzδT(z,t)+θ)].\psi(z,t)=\Lambda_{0}~{}\mathrm{sech}^{2}\left(w_{0}\tau(z,t)\right)\exp[i(\kappa z-\delta T(z,t)+\theta)]. (71)

where τ(z,t)=tζ(z)η\tau(z,t)=t-\zeta(z)-\eta. The amplitude Λ0\Lambda_{0} is a free real parameter, the inverse width w0w_{0} and the wave number κ\kappa are given in (35) with the parametric conditions as α2=0\alpha_{2}=0 and σ1=(σ2+σ3)/7\sigma_{1}=-(\sigma_{2}+\sigma_{3})/7.

The solution (37) and transformation (70) gives rise to a family of self-similar W-shaped soliton solution for Eq. (40) as

ψ(z,t)=B0(132sech2(w0τ(z,t)))exp[i(κzδT(z,t)+θ)],\psi(z,t)=B_{0}\left(1-\frac{3}{2}\mathrm{sech}^{2}\left(w_{0}\tau(z,t)\right)\right)\exp[i(\kappa z-\delta T(z,t)+\theta)], (72)

where τ(z,t)=tζ(z)η\tau(z,t)=t-\zeta(z)-\eta. The amplitude B0B_{0} is a free real parameter, the inverse width w0w_{0} and the wave number κ\kappa are given in (38) and (39) with the parametric conditions as α2=0\alpha_{2}=0 and σ1=(σ2+σ3)/7\sigma_{1}=-(\sigma_{2}+\sigma_{3})/7.

VI.1 Deceleration of bright and W-shaped solitons

Now consider an exponential distributed control system with a spatial modulation of D1(z)D_{1}(z) as given by Eq. (61). Consequently, the function ζ(z)\zeta(z) for the bright and W-shaped soliton pulses given in Eq. (69) is determined as

ζ(z)=g0z+g1m(emz1).\zeta(z)=g_{0}z+\frac{g_{1}}{m}\left(e^{mz}-1\right). (73)

This shows that the slowing soliton can be achieved for V(z)=1/D1(z)1/α1V(z)=1/D_{1}(z)\ll 1/\alpha_{1} or D1(z)α1.D_{1}(z)\gg\alpha_{1}.

Refer to caption
Figure 4: Intensity distribution of (a)-(b) the bright soliton (71) and (c)-(d) the W-shaped soliton (72) for D1(z)D_{1}(z) given by Eq. (61). The parameters are g0=1,g_{0}=1, g1=4,m=0.5g_{1}=4,m=-0.5 and η=0\eta=0. The other parameters are the same as those in Figs. 1(b) and 1(c) respectively.

In Figs. 4(a)-(b) and 4(c)-(d), we have depicted the propagation dynamics of the bright and W-shaped solitons (71) and (72) in the control system with D1(z)D_{1}(z) given by Eq. (61) for the parameter values g0=1,g_{0}=1, g1=4,m=0.5g_{1}=4,m=-0.5 and η=0\eta=0. The other parameters are chosen as those in Figs. 1(b) and 1(c) respectively. We clearly see that that through this spatial variation of D1(z)D_{1}(z), the soliton pulses can be slowed while evolving in distance. We also observe that the amplitude and the width of the solitons keep invariant as distance increases.

VI.2 Acceleration of bright and W-shaped solitons

We now consider a periodic variation of the intermodal dispersion coefficient D1(z)D_{1}(z) in the form (64). For this parametric choice, the function ζ(z)\zeta(z) for the bright and W-shaped solitons given in Eq. (69) takes the form,

ζ(z)=12agz2cos(az2).\zeta(z)=\frac{1}{2a}gz^{2}\cos(az^{2}). (74)
Refer to caption
Figure 5: Intensity distribution of (a)-(b) the bright soliton (71) and (c)-(d) the W-shaped soliton (72) for D1(z)D_{1}(z) given by Eq. (64). The parameters are g=0.3g=-0.3, a=1a=1 and η=0\eta=0. The other parameters are the same as those in Figs. 1(b) and 1(c) respectively.

We present the propagation dynamics of the bright and W-shaped solitons (71) and (72) in the control system with D1(z)D_{1}(z) given Eq. (64) in Figs. 5(a)-(b) and 5(c)-(d) with g=0.3g=-0.3, a=1a=1 and η=0\eta=0. The other parameters are chosen as those in Figs. 1(b) and 1(c) respectively. The changes of the soliton trajectories in these figures clearly indicate their accelerating motion.

VII Conclusion

In conclusion, we have studied the wave-speed management of dipole, bright and W-shaped solitons in an optical metamaterial exhibiting higher-order dispersive and nonlinear effects of different nature. The propagation of few-cycle pulse in such system is described by the generalized nonlinear Schrödinger equation incorporating distributed group velocity dispersion, cubic nonlinearity, intermodal dispersion, self-steepening, nonlinear dispersion, and higher-order nonlinear terms that appear in the setting of metamaterials. We have found that the medium supports the existence of three new types of periodic wave solutions that are composed of the product of pairs of Jacobi elliptic functions in the presence of all physical processes. We have also developed an effective similarity transformation method to study the soliton dynamics in the presence of the inhomogeneities of media and analyze the soliton wave-speed management. The results have showed that an effective control of the soliton wave speed can be achieved through an appropriate choice of the group velocity dispersion and intermodal dispersion parameters. In particular, we have demonstrated that the soliton pulses can be decelerated and accelerated by suitably choosing the spatial variation of the dispersion parameters. We anticipate that the obtained results will be important in the future investigations of ultrashort solitons in nonlinear metamaterials.

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