soliton solution, backlund transformation, and conservation … · 2016-06-28 · soliton solution,...

10
Soliton Solution, B¨ acklund Transformation, and Conservation Laws for the Sasa-Satsuma Equation in the Optical Fiber Communications Ying Liu a , Yi-Tian Gao a,b , Tao Xu c , Xing L ¨ u c , Zhi-Yuan Sun a , Xiang-Hua Meng c , Xin Yu a , and Xiao-Ling Gai a a Ministry-of-Education Key Laboratory of Fluid Mechanics and National Laboratory for Computational Fluid Dynamics, Beijing University of Aeronautics and Astronautics, Beijing 100191, China b State Key Laboratory of Software Development Environment, Beijing University of Aeronautics and Astronautics, Beijing 100191, China c School of Science, P. O. Box 122, Beijing University of Posts and Telecommunications, Beijing 100876, China Reprint requests to Y.-T. G.; E-mail: [email protected] Z. Naturforsch. 65a, 291 – 300 (2010); received April 27, 2009 / revised August 11, 2009 Under investigation in this paper, with symbolic computation, is the Sasa-Satsuma (SS) equation which can describe the propagation of ultra short pulses in optical fiber communications. By virtue of the Ablowitz-Kaup-Newell-Segur procedure, the Lax pair for the SS equation is directly established. Based on such a Lax pair, a B¨ acklund transformation is constructed, through which the explicit one- soliton solution is derived. Meanwhile, an infinite number of conservation laws is provided to indicate the integrability of the SS equation in the Liouville sense. To further understand the stability of the one-soliton solution, we employ the split-step Fourier method to simulate the propagation of the soliton pulses under the finite initial perturbations. In addition, the interaction of two adjacent pulses with different separation distances is investigated through numerical simulation. Analytic and numerical results discussed in this paper are expected to be applied to the description of the optical pulse propagation. Key words: Sasa-Satsuma Equation; Lax Pair; B¨ acklund Transformation; One-Soliton Solution; Infinite Number of Conservation Laws; Soliton Interaction. PACS numbers: 42.65.Tg, 42.81.Dp, 05.45.Yv 1. Introduction In recent years, attention has been paid to the studies on the nonlinear evolution equations (NLEEs) [1 – 3] and the relevant soliton problems in the fluid dynamics [1], plasma physics [2 – 5], and optical fiber communications [6 – 10]. One of the prototype NLEEs is the nonlinear Schr¨ odinger (NLS) equation [11 – 15], iq t + 1 2 q x x + |q| 2 q = 0, (1) where q represents the complex amplitude of the pulse envelope, t and x are the normalized tem- poral and spatial variables [14]. The NLS equation usually governs the propagation of optical pulses in a monomode fiber based on the exact balance be- tween the group velocity dispersion and self-phase 0932–0784 / 10 / 0400–0291 $ 06.00 c 2010 Verlag der Zeitschrift f¨ ur Naturforschung, T ¨ ubingen · http://znaturforsch.com modulation [11], and the two effects lead to sym- metric broadening in the time and frequency do- mains, respectively [16]. However, in the real fiber communications, the NLS equation becomes inade- quate to describe the propagation of optical pulses in the subpicosecond or femtosecond region [13, 14]. In order to overcome the above limitations, the higher-order effects such as the third-order dispersion (TOD), self-steepening, and stimulated Raman scatter- ing (SRS) should be considered in the NLS models [11, 12, 14, 16]. Generally speaking, those effects can produce the asymmetrical temporal broadening, asym- metrical spectral broadening, and redshift increasing in the pulse spectrum for the ultrashort pulses, re- spectively [16]. With that consideration, the follow- ing modified higher-order NLS (HNLS) equation has been proposed for describing the propagation of the femtosecond optical pulses in the monomode optical

Upload: others

Post on 12-Feb-2020

9 views

Category:

Documents


0 download

TRANSCRIPT

Page 1: Soliton Solution, Backlund Transformation, and Conservation … · 2016-06-28 · Soliton Solution, Backlund Transformation, and Conservation Laws¨ for the Sasa-Satsuma Equation

Soliton Solution, Backlund Transformation, and Conservation Lawsfor the Sasa-Satsuma Equation in the Optical Fiber Communications

Ying Liua, Yi-Tian Gaoa,b, Tao Xuc, Xing Luc, Zhi-Yuan Suna, Xiang-Hua Mengc,Xin Yua, and Xiao-Ling Gaia

a Ministry-of-Education Key Laboratory of Fluid Mechanics and National Laboratory forComputational Fluid Dynamics, Beijing University of Aeronautics and Astronautics,Beijing 100191, China

b State Key Laboratory of Software Development Environment, Beijing University of Aeronauticsand Astronautics, Beijing 100191, China

c School of Science, P. O. Box 122, Beijing University of Posts and Telecommunications,Beijing 100876, China

Reprint requests to Y.-T. G.; E-mail: [email protected]

Z. Naturforsch. 65a, 291 – 300 (2010); received April 27, 2009 / revised August 11, 2009

Under investigation in this paper, with symbolic computation, is the Sasa-Satsuma (SS) equationwhich can describe the propagation of ultra short pulses in optical fiber communications. By virtue ofthe Ablowitz-Kaup-Newell-Segur procedure, the Lax pair for the SS equation is directly established.Based on such a Lax pair, a Backlund transformation is constructed, through which the explicit one-soliton solution is derived. Meanwhile, an infinite number of conservation laws is provided to indicatethe integrability of the SS equation in the Liouville sense. To further understand the stability ofthe one-soliton solution, we employ the split-step Fourier method to simulate the propagation ofthe soliton pulses under the finite initial perturbations. In addition, the interaction of two adjacentpulses with different separation distances is investigated through numerical simulation. Analytic andnumerical results discussed in this paper are expected to be applied to the description of the opticalpulse propagation.

Key words: Sasa-Satsuma Equation; Lax Pair; Backlund Transformation; One-Soliton Solution;Infinite Number of Conservation Laws; Soliton Interaction.

PACS numbers: 42.65.Tg, 42.81.Dp, 05.45.Yv

1. Introduction

In recent years, attention has been paid to thestudies on the nonlinear evolution equations (NLEEs)[1 – 3] and the relevant soliton problems in the fluiddynamics [1], plasma physics [2 – 5], and opticalfiber communications [6 – 10]. One of the prototypeNLEEs is the nonlinear Schrodinger (NLS) equation[11 – 15],

iqt′ +12

qx′x′ + |q|2q = 0, (1)

where q represents the complex amplitude of thepulse envelope, t ′ and x′ are the normalized tem-poral and spatial variables [14]. The NLS equationusually governs the propagation of optical pulses ina monomode fiber based on the exact balance be-tween the group velocity dispersion and self-phase

0932–0784 / 10 / 0400–0291 $ 06.00 c© 2010 Verlag der Zeitschrift fur Naturforschung, Tubingen · http://znaturforsch.com

modulation [11], and the two effects lead to sym-metric broadening in the time and frequency do-mains, respectively [16]. However, in the real fibercommunications, the NLS equation becomes inade-quate to describe the propagation of optical pulsesin the subpicosecond or femtosecond region [13, 14].In order to overcome the above limitations, thehigher-order effects such as the third-order dispersion(TOD), self-steepening, and stimulated Raman scatter-ing (SRS) should be considered in the NLS models[11, 12, 14, 16]. Generally speaking, those effects canproduce the asymmetrical temporal broadening, asym-metrical spectral broadening, and redshift increasingin the pulse spectrum for the ultrashort pulses, re-spectively [16]. With that consideration, the follow-ing modified higher-order NLS (HNLS) equation hasbeen proposed for describing the propagation of thefemtosecond optical pulses in the monomode optical

Page 2: Soliton Solution, Backlund Transformation, and Conservation … · 2016-06-28 · Soliton Solution, Backlund Transformation, and Conservation Laws¨ for the Sasa-Satsuma Equation

292 Y. Liu et al. · Soliton Solution, Backlund Transformation, and Conservation Laws for the Sasa-Satsuma Equation

fibers [11, 17],

iQZ +12

QT T + |Q|2Q

+ i[β1QT T T + β2|Q|2QT + β3Q(|Q|2)T

]= χ

[− iΓ Q+ σQ(|Q|2)T],

(2)

where Q(T,Z) is the normalized complex amplitudeof the pulse envelope, Z and T represent the nor-malized distance along the fiber and the retardedtime, respectively [17]. β1, β2, and β3 account forthe TOD, Kerr coefficient, and self-frequency shiftarising from the SRS, respectively [16, 18]. The twoterms on the right hand side of (2) give the fiber lossand self-induced Raman scattering effect. Moreover,Γ and σ are the real normalized parameters dependingon the fiber characteristics, and χ is a small parame-ter [17].

Without the fiber loss and Raman scattering, i. e.,when χ = 0, (2) reduces to the following HNLS equa-tion [18 – 20]:

iQZ +12

QT T + |Q|2Q

+ i[β1QT T T + β2|Q|2QT + β3Q(|Q|2)T

]= 0.

(3)

In general, (3) is not completely integrable unless thereal parameters β1, β2, and β3 satisfy the followingconstraints: β1 : β2 : β3 = 0 : 1 : 1, β1 : β2 : β3 =0 : 1 : 0, β1 : β2 : β3 = 1 : 6 : 0, and β1 : β2 : β3 =1 : 6 : 3, which correspond to the completely inte-grable derivative NLS equation-type I, derivative NLSequation-type II, Hirota equation, and Sasa-Satsuma(SS) equation, respectively [13, 21 – 23]. In this paper,we will focus our interest on the SS equation, a gener-alized version of the case mentioned above [13, 20],

iQt +12

Qxx + |Q|2Q

+i

6ε[Qxxx + 6|Q|2Qx + 3Q(|Q|2)x

]= 0,

(4)

where Q represents a complex field, the subscripts xand t are the spatial and temporal partial derivatives,and ε is a small parameter [13, 20]. (4) can describethe development of the complex scalar field and theevolution of the short optical pulses [13, 20]. Authorsof [11, 24] mention that (4) is necessary for correctlymodelling the ultra-fast optical pulses in which the pe-riod of the envelope is comparable to that of the car-rier, i. e., on the scale of femtoseconds. In such a situ-ation, the pulse width can be decreased to a low level

(less than 1 ps) by the compression techniques [11],resulting in the increase of the bit rate in the opticalfiber communication systems for a single carrier fre-quency [8].

Integrable properties of (4) have been investigatedfrom different points of view [7, 13, 17, 20, 25, 26]. In-tegrability of (4) has been proved based on the inversescattering transform (IST) method [13]. It is knownthat a completely integrable NLEE often admits theBacklund transformation (BT), Lax pair representa-tion, Darboux transformation (DT), soliton solutions,and infinite number of conservation laws [15, 27, 28].In addition, compared with the generalized Hirotaequation [23, 29], (4) has some properties due to thedifferent higher-order terms, which can be concludedas:

• The Lax pair is a 3 × 3 matrix formalizationgeneralized from the Ablowitz-Kaup-Newell-Segur(AKNS) system [13, 30].

• The bilinearization of (4) is a reduction ofthe three-component Kadomtsev-Petviashvili hierar-chy [31].

• The one-soliton solution derived from the ISTmethod can exhibit the stable shape of two peaks withthe same height when the specific parameters satisfycertain conditions [13].

• The types of the infinite conserved quantitiesfor (4) are different from the ones for the Hirota equa-tion [32].

However, we notice that most of those studies havetreated the SS equation by reducing it to a com-plex modified Korteweg-de Vries (cmKdV) equationthrough the Galelian transformation, as seen in [13,17, 20, 26, 30]. Further, integrable properties and soli-ton solutions have been discussed based on such a re-duction [13, 17, 20, 26, 30], but the generality of theabove process for (4) is inadequate to some extent,i. e., some information might be neglected [13, 31]. Infact, authors of [31] have claimed that in many pre-vious attempts, the reduction from the SS equation tothe cmKdV equation produces only rather trivial solu-tions, in which the complex and multicomponent free-dom has been frozen due to the number of indepen-dent equations being more than the unknown variables.On the other hand, the two-soliton solutions have beenderived analytically by virtue of the cmKdV equa-tion [26], whereas the interaction patterns have beenlimited by the constraints of the real wavenumbers pre-sented in [26].

Page 3: Soliton Solution, Backlund Transformation, and Conservation … · 2016-06-28 · Soliton Solution, Backlund Transformation, and Conservation Laws¨ for the Sasa-Satsuma Equation

Y. Liu et al. · Soliton Solution, Backlund Transformation, and Conservation Laws for the Sasa-Satsuma Equation 293

Therefore, to better understand the features of (4),we will organize this paper, with symbolic computa-tion [2, 3, 5, 9], as follows: In Section 2, a new Lax pairwill be constructed directly from (4) by virtue of theAKNS procedure [33], which appears to be differentfrom the one in [20]. Section 3 will present the BT bymeans of the Γ -Riccati form of the Lax pair. Mean-while, the one-soliton solution of (4) will be derivedvia the obtained BT. In Section 4, we will constructa set of the related symmetrical Γ -Riccati equationsand subsequently exhibit an infinite number of conser-vation laws, which are considered to be more generalthan the conserved quantities in [20] and [30]. In Sec-tion 5, numerical simulation for the propagation of thederived one-soliton solution under the finite initial per-turbation will be investigated to demonstrate its stabil-ity. In addition, the two adjacent pulses with differentseparation distances will be studied on their interac-tion process, and the results will provide more generalinteraction patterns for the initial pulses, such as fu-sion and repulsion. Finally, our conclusions will be ad-dressed in Section 6.

2. Lax Pair

In this section, we will employ the Painleve analy-sis similar to the procedure in [18] and [34] to validatethe integrability of (4) in the Painleve sense. In order toperform the Painleve analysis, we rewrite (4) in termsof two complex functions q(x,t) and p(x,t) by defin-ing q(x, t) = Q(x,t) and p(x,t) = Q∗(x,t), where ∗ de-notes the complex conjugate. In such case, (4) can beexpressed as the following equations:

iqt +12

qxx + q2p

+i

6ε[qxxx + 6pqqx + 3q(pq)x] = 0,

(5)

−ipt +12

pxx + p2q

− i6ε

[pxxx + 6qppx + 3p(qp)x] = 0.

(6)

The Weiss-Talor-Carnevale method [35] with the sim-plified Kruskal ansatz can be carried out to seek a so-lution of (5) and (6) in the form

q(x, t) = ϕ−α(x,t)∞

∑j=0

q j(x,t)ϕ j(x,t), (7)

p(x, t) = ϕ−β (x,t)∞

∑j=0

p j(x,t)ϕ j(x,t), (8)

where q j(x, t), p j(x, t), and ϕ(x, t) are the arbitrary an-alytic functions with variables x and t in the neighbour-hood of a noncharacteristic movable singularity mani-fold defined by ϕ(x, t) = 0, while α and β are two pos-itive integers to be determined. Via the leading orderanalysis, we can derive α = β = 1 and p0q0 = − 1

2 ϕ2x .

Then the resonance terms are found at j = −1, 0, 2,3, 4, in which j = −1 corresponds to the arbitrarinessof the singular manifold. Furthermore, (5) and (6) areproved to pass the Painleve test through verifying thecompatibility conditions for the remaining resonanceterm.

In the following content, by employing the AKNSprocedure, the Lax pair for (4) can be constructed.Consider the following two linear eigenvalue prob-lems [15]:

Φx = UΦ = (λU0 +U1)Φ, (9)

Φt = VΦ = (λ 3V0 + λ 2V1 + λV2 +V3)Φ, (10)

where λ is a spectral parameter, U and V are both 3×3 matrices, Φ = (φ1,φ2,φ3)T with T representing thetranspose of the vector. (9) and (10) are required to becompatible, so U and V should satisfy the zero curveequation,

Ut −Vx +[U,V ] = 0, (11)

by which the matrices U0, U1, V0, V1, V2, and V3 can bedetermined in the following forms:

U0 =

−i 0 0

0 i 00 0 i

,

U1 =

0 kq k∗p−k∗p 0 0−kq 0 0

,

(12)

V0 =2

3εU0, V1 =

23ε

U1, (13)

V2 =

A1 + i

3ε pq kA2 −k∗A∗2

−k∗A∗2 A∗

1 (−k∗)2A∗3

kA2 k2A3 A∗1

,

V3 =

0 kA4 k∗A∗

4−k∗A∗

4 A5 0kA4 0 A∗

5

,

(14)

Page 4: Soliton Solution, Backlund Transformation, and Conservation … · 2016-06-28 · Soliton Solution, Backlund Transformation, and Conservation Laws¨ for the Sasa-Satsuma Equation

294 Y. Liu et al. · Soliton Solution, Backlund Transformation, and Conservation Laws for the Sasa-Satsuma Equation

with

k = exp[

i(

tε2

3− xε

)], A1 =

ipq3ε

+iε2

,

A2 =qε + iqx

3ε, A3 = − iq2

3ε,

A4 = − 16ε

(2ε2q + 4pq2−2iεqx + qxx),

A5 =1

6ε(qpx − pqx−2iε pq).

Substituting U and V into the compatibility condi-tion (11), it can be proved that (11) is equivalent to (5)and its conjugate form (6). The derived Lax pair, whichensures the complete integrability of (4), can be used toconstruct the BT and DT to obtain the N-soliton solu-tions. In the next section, the one-soliton solution willbe derived by employing the BT.

3. BT and One-Soliton Solution

The BT has been widely used to derive soliton so-lutions for the NLEEs [5, 7, 10, 35 – 38]. There existseveral methods to obtain the BT [36], such as trun-cating the Painleve expansion at the constant levelterm [5, 35], bilinearizing the NLEEs [37, 38], and us-ing the Γ -Riccati form of the Lax pair [7]. Here,through the obtained Lax pair in Section 2, we can con-struct the BT of (4), based on which the explicit one-soliton solution can be further given as an illustrativeexample.

By introducing

Γ1 =φ1

φ3, Γ2 =

φ2

φ3, (15)

the eigenvalue problems can be expressed in the Γ -Riccati form

Γ1x = k∗p−2iλΓ1 + kqΓ2 + kqΓ 21 , (16)

Γ2x = −k∗pΓ1 + kqΓ1Γ2. (17)

We can define a transformation from (Γ1, Γ2, λ , q, p)to (Γ ′

1 , Γ ′2 , λ ′

, q′, p

′), which keeps the forms of (16)

and (17) invariant. For simplicity, the transformationcan be tried by giving Γ ′

1 = Γ1, Γ ′2 = Γ2 together with

λ ′= λ ∗ [7], and then the following relationships are

obtained:

q′ −q =2iΓ1(λ ∗ −λ )2kΓ2 + kΓ 2

1, (18)

p′ − p =2iΓ1Γ2(λ ∗ −λ )2k∗Γ2 + k∗Γ 2

1. (19)

(18) and (19) are regarded as the BT for (4), throughwhich a series of explicit solutions can be obtained ina recursive manner from a given seed solution. For in-stance, by choosing q0 = 0, p0 = 0, and λ = iβ (β isa real constant), we obtain the following pseudopoten-tials via (16) and (17):

Γ1 = c1 exp[

2β x− t(

4β 3

3ε+ β ε

)], (20)

Γ2 = c2, (21)

where c1 and c2 are the arbitrary complex integral con-stants. Furthermore, c1 and c2 can be found to satisfythe relationship c2 = c1/c∗1, which implies the exis-tence of only two arbitrary constants c1 and β . Sub-stituting (20) and (21) into (18) and (19), we can de-rive the one-soliton solution for (4), which can be ex-pressed as

Q(x, t) = 4β c∗1 exp(

4tβ 3

3ε+ 2xβ + tεβ −1

3itε2 + ixε

)

·[

c1c∗1 exp(4xβ )+ 2exp(

8tβ 3

3ε+ 2tεβ

)]−1

, (22)

Q∗(x, t)=4β c1 exp(

4tβ 3

3ε+ 2xβ + tεβ +

13

itε2−ixε)

·[

c1c∗1 exp(4xβ )+ 2exp(

8tβ 3

3ε+ 2tεβ

)]−1

. (23)

Notice that Expression (22) can be simplified as

Q(x, t) = 2β c∗1 exp(

2β x + iεx− iε2

3t − 4β 3

3εt −β εt

)

·[

1 +|c1|2

2exp

(4β x− 8β 3

3εt −2β εt

)]−1

= β c∗1 exp(

ixε − itε2

3− δ

)

· sech(

2xβ − 4tβ 3

3ε− tεβ + δ

),

(24)

with δ = 12 ln |c1|2

2 . If β and c1 are chosen as

β =µ2

, c∗1 =Lµ

, (25)

Page 5: Soliton Solution, Backlund Transformation, and Conservation … · 2016-06-28 · Soliton Solution, Backlund Transformation, and Conservation Laws¨ for the Sasa-Satsuma Equation

Y. Liu et al. · Soliton Solution, Backlund Transformation, and Conservation Laws for the Sasa-Satsuma Equation 295

Expression (24) can be changed into the followingform:

Q(x, t) =Lexp

(µx + iεx− iε2

3 t − µ3

6ε t − εµ2 t

)

1 +|L|22µ2 exp

(2µx− µ3

3ε t − µεt) ,

which agrees with the result obtained by the bilinearmethod in [20]. Ulteriorly, other choices of β and c1offer a class of one-soliton solutions with similar prop-erties.

4. Infinite Number of Conservation Laws

The rigidity in the structures of the solitons revealsthat the system has a bulk underlying symmetry mani-fested by the existence of an infinite number of conser-vation laws, which provides a compelling evidence toshow the integrability of (4) in the Liouville sense [30].In this section, we will show that through the BT, notonly the one-soliton solution can be derived, but alsoan infinite number of conservation laws can be con-structed.

Firstly, we can write the auxiliary field Φ in thecomponent form [20],

Φ =

φ1

φ2φ3

. (26)

Inserting (26) into (9), the following three equationscan be obtained based on the 3×3 matrices:

φ1x = −iλ φ1 + kqφ2 + k∗pφ3, (27)

φ2x = −k∗pφ1 + iλ φ2, (28)φ3x = −kqφ1 + iλ φ3. (29)

Defining another two associated Riccati variables interms of T1 = φ2/φ1 and T2 = φ3/φ1, we derive the fol-lowing two Riccati equations by eliminating T1 and T2from (27) – (29):

T1x = −k∗p + 2iλ T1− kqT21 − k∗pT1T2, (30)

T2x = −kq + 2iλ T2− k∗pT 22 − kqT1T2. (31)

In order to search for series of solutions of (30)and (31), T1 and T2 are assumed in the forms

T1 =∞

∑n=0

cnλ−n, (32)

T2 =∞

∑n=0

dnλ−n. (33)

Substituting the above expressions into (30), the recur-sion relations are given by

c0 = 0, c1 =k∗p2i

,

2icn+2 = cn+1,x

+n+1

∑m=0

(cmcn−m+1kq + cmdn−m+1k∗p).

(34)

Correspondingly, via (31), the similar recursion rela-tions can be found as

d0 = 0, d1 =kq2i

,

2idn+2 = dn+1,x

+n+1

∑m=0

(dmdn−m+1k∗p + dmcn−m+1kq).

(35)

T1 and T2 can be explicitly expressed by substitutingthe aforementioned recursion relations of cn and dninto Expressions (32) and (33).

Afterwards, inserting T1 and T2 into the equation(lnφ1)xt = (lnφ1)tx, an infinite number of conservationlaws can be generated as [4, 39]

∂Di

∂ t=

∂Fi

∂x(i = 1,2, . . .), (36)

where Di and Fi are called the conserved density andflux, respectively. Thus, the first three conserved quan-tities are given as:

D1 = −ipq,

F1 =ip2q2

ε− pxq

2+

ipxxq6ε

+pqx

2

− ipxqx

6ε+

ipqxx

6ε,

D2 =14(−qpx − pqx),

F2 =qqx p2

2ε+

q2 px p2ε

− 18

iqxx p +qxxx p24ε

+18

iqpxx +qpxxx

24ε,

D3 =12

ip2q2 − 14

ipε2q− 14

ε pxq

+18

ipxxq +18

ipqx +14

pεqx,

Page 6: Soliton Solution, Backlund Transformation, and Conservation … · 2016-06-28 · Soliton Solution, Backlund Transformation, and Conservation Laws¨ for the Sasa-Satsuma Equation

296 Y. Liu et al. · Soliton Solution, Backlund Transformation, and Conservation Laws for the Sasa-Satsuma Equation

(a) (b)

(c) (d)

Fig. 1. Numerical simulation of the propagation of the initial pulses Q(x,0) with the parameters chosen as β = 0.1 andc1 = 1+ i. (a) ε = 0.17; (b) ε = 0.2; (c) ε = 0.5; (d) ε = 1.

F3 = −2ip3q3

3ε− 5ip2

xq2

48ε+

12

ip2εq2 +34

ppxq2

− 5ippxxq2

12ε− 1

8ε2 pxq +

16

iε pxxq +5pxxxq

48

− ipxxxxq48ε

− 34

p2qxq− 7ippxqxq24ε

− 5ip2qxxq12ε

− 5ip2q2x

48ε+

18

pε2qx − 724

iε pxqx

− 7pxxqx

48+

ipxxxqx

48ε− 5pqxx

48+

16

ipεqxx

+7pxqxx

48− ipxxqxx

24ε+

ipxqxxx

48ε− ipqxxxx

48ε. (37)

5. Numerical Simulation of the PulsePropagations

In this section, we will employ the numerical simu-lation to analyze the propagations of the one-solitonand two adjacent solitary pulses. In details, the fol-lowing two aspects will be considered: one is thepropagation of Solution (24) under the finite initial

perturbation, and the other are the interactions be-tween two adjacent pulses with the relevant parametersvarying.

5.1. Stability of the One-Soliton Solution Under theFinite Initial Perturbation

Generally speaking, propagation of the soliton pulsegoverned by (4) is influenced by the combination of thehigher-order effects such as the TOD, SS, and SRS.The balance among those effects provides the possibil-ity for the existence of the solitons, or solitary waves,both bright and dark ones [11, 14, 40, 41]. Further, thestability of the soliton pulse under the finite initial per-turbation has been commonly discussed for its theoret-ical and practical applications [42 – 44]. One noticesthat with the variation of the factor 1/(6ε) in (4), dif-ferent situations of the higher-order terms can be mod-eled. Therefore in the following content, our interestwill be devoted to the propagation of Solution (24)under the finite initial perturbation (10 % perturbation

Page 7: Soliton Solution, Backlund Transformation, and Conservation … · 2016-06-28 · Soliton Solution, Backlund Transformation, and Conservation Laws¨ for the Sasa-Satsuma Equation

Y. Liu et al. · Soliton Solution, Backlund Transformation, and Conservation Laws for the Sasa-Satsuma Equation 297

(a) (b)

(c) (d)

Fig. 2. Interaction of two pulses with the parameter chosen as β = 0.1. For ε = 0.17, (a) the separation distance T0 = 10;(b) T0 = 15. For ε = 1, (c) T0 = 25; (d) T0 = 60.

of the amplitude) with ε varying in the appropriaterange.

Perturbed initial pulse is chosen as

Q(x,0) = 1.1

√2β c∗1|c1|

· sech[

2β x + ln( |c1|√

2

)]exp(iεx).

(38)

Numerical simulation is carried out in the MATLABsoftware environment by using the split-step Fourier(SSF) method [11]. The computational domain for x ischosen as [−350,350] and 7000 grid points are used.The propagation distance with respect to t is takenas 100 with a step size of 0.05. In the simulation, weaccept the assumption that 0 < 1/(6ε) < 1, i. e., therange of ε > 0.167 [26]. The parameters in the ini-tial pulse (38) are taken as β = 0.1 and c1 = 1 + i.Figures 1a – d present the numerical results with ε in-creasing, which demonstrate that the perturbed initialpulses propagate in different manners depending on thechoices of ε . When the value of ε is small, the initialpulse is distorted such that it becomes asymmetric with

several humps emerging (see Fig. 1a) and the pulsebroadening is remarkable for the long time propaga-tion. On the other hand, the higher-order effects, suchas the TOD, which can make the intensity amplitudeasymmetric and introduce a long oscillating tail [11],will contribute to the stability of the pulse propagationas the factor 1/(6ε) is not small. As ε increases, theshape of perturbed pulse tends to be smooth and ex-hibits only the broadening effect (see Figs. 1b – d). Fur-ther, the perturbed pulse seems to acquire an increasingvelocity along the x propagation direction as ε grow-ing. For a larger value of ε , the influence of the higher-order effects is weakening and the pulse can propagatemore stably (with weaker broadening) within the samedistance along x.

5.2. Interaction Between Two Adjacent Pulses

For the models governed by the NLS-typed equa-tions, the interaction between the two adjacent ini-tial pulses have attracted considerable interest [41,43 – 47]. Those interactions include a variety of pat-terns, such as the periodic merger and separation, re-

Page 8: Soliton Solution, Backlund Transformation, and Conservation … · 2016-06-28 · Soliton Solution, Backlund Transformation, and Conservation Laws¨ for the Sasa-Satsuma Equation

298 Y. Liu et al. · Soliton Solution, Backlund Transformation, and Conservation Laws for the Sasa-Satsuma Equation

pulsion and fusion, depending on the initial conditionsto some extent [43, 45]. In this section, the two adja-cent pulses with different separation distances and rel-evant parameters will be studied on their interactionprocess through numerical simulation. Although theanalytic expression of the two-soliton solutions for (4)exist [26], it requires the two wavenumbers to be realand satisfy an exact dispersion relation, which is notgeneric enough in generating the initial pulses in theoptical fiber communications. Here the initial pulse canbe given as

Q(x,0) =

β sech[

2β(

x +T0

2

)]exp

[iε

(x +

T0

2

)]

+ β sech[

2β(

x− T0

2

)]exp

[iε

(x− T0

2

)],

(39)

where T0 is the initial separation distance of the twopulses with respect to x, β and ε are the parametersintroduced in Solution (24) and (4), respectively. Theabove form of the pulse is based on the analytic Solu-tion (24), but convenient and general for the numericalsimulation.

Results with the typical values of ε are demonstratedin Figure 2 for the separation distances T0 = 10, 15, 25,and 60. In the case of ε = 0.17, most of the two initialpulses are overlapped for T0 = 10 and the pulses in-teract asymmetrically with t propagating (see Fig. 2a).The amplitude of one pulse exhibits gradually atten-uation and its energy is transformed to the coherentpulse, the width of which is induced to broaden dur-ing the 100 propagating distance with respect to t.When T0 = 15, the similar attenuation and broaden-ing for each pulse exist in like manner, however, thetwo pulses repel each other at the propagating dis-tance of approximately 40 and the left pulse appearsto propagate parallel to axis t (see Fig. 2b). For ε = 1,the pulse interactions for T0 = 10 and 15 are analog-ical to those in Figures 2a and b, but the repulsionfor T0 = 15 is not visible. Figures 2c and d presentthe interactions for larger separation distances T0 = 25and 60 in the case of ε = 1. When T0 = 25, the twosolitary pulses begin to evolve into one pulse whoseamplitude increases promptly after about 25 propa-gating distance, and at the same time, the two ini-tial pulses attenuate with the width broadening (seeFig. 2c). The numerical calculation for ε = 0.17 re-veals that the fusion-like interaction occurs for T0 =35 ∼ 40, but some small oscillations exist on the pro-

file surface, which can be viewed as the similar effectto that in Figure 1a. When T0 = 60, the two pulsescan propagate for a longer distance along t, exhibit-ing the width broadening before their interaction. Afterabout 75 propagating distance, the multi-hump struc-ture is formed through the interaction (see Fig. 2d),and such humps are more disordered in the case ofε = 0.17.

Therefore, one notices that due to the combined ef-fects of the TOD, self-steepening, and SRS, the inter-actions between the two adjacent pulses have certainfeatures similar to those in the propagation of the one-soliton solution under finite initial perturbation, suchas the pulse broadening and formation of the multi-hump structures. Considering that, the analytic solu-tions need some strict balances and restrains amongthe terms in (4) and relevant parameters, respectively,which would be difficult to produce, the above numeri-cal simulation might provide some necessary informa-tion for the understanding of the propagation and inter-action of the solitary pulses.

6. Conclusions

In this paper, considering the role of the SS equa-tion, i. e., Equation (4), in describing the evolutionof ultra short pulses, which can benefit the high ca-pacity transmission in the optical fiber communica-tions, we have investigated the SS equation from theintegrable point of view. Following the AKNS pro-cedure, we have constructed the 3 × 3 matrix Laxpair and further obtained the BT. Based on the BT,the one-soliton solution has been derived, which canbe viewed as the generalized form of the one ob-tained by the bilinear method under certain paramet-ric conditions. In addition, by the symmetrical Ric-cati equations, an infinite number of conservation lawshave been presented, as a proof of the integrabilityin the Liouville sense. Furthermore, propagation ofthe one-soliton pulse under the finite initial perturba-tion has been analyzed with the SSF method. Syn-chronously, interaction processes of the two adjacentpulses with different separation distances and rele-vant parameters have been studied through numeri-cal simulation. It is expected that the analytic resultsdiscussed in this paper would be helpful in studyingthe linear eigenvalue problems with the 3 × 3 ma-trix and similar integrable properties of the mod-els in optical fiber communications. Meanwhile, nu-merical simulation for the propagation of the one-

Page 9: Soliton Solution, Backlund Transformation, and Conservation … · 2016-06-28 · Soliton Solution, Backlund Transformation, and Conservation Laws¨ for the Sasa-Satsuma Equation

Y. Liu et al. · Soliton Solution, Backlund Transformation, and Conservation Laws for the Sasa-Satsuma Equation 299

soliton and two adjacent solitary pulses could pro-vide certain applications in those nonlinear opticalfields.

On the other hand, the coupled HNLS (CHNLS)equations have been derived from the vector formof (4) with �Q as a sum of the left- and right-handedpolarized waves [18], which have the relevant applica-tions in the electromagnetic pulse propagations in thecoupled optical waveguides and in a weakly relativis-tic plasma with the nonlinear coupling of two polar-ized transverse waves [18]. Considering the similari-ties between (4) and the coupled ones, the same ana-lytic and numerical procedures can be addressed to dis-cuss the relevant integrable properties for the CHNLSequations.

Acknowledgements

We express our sincere thanks to all the membersof our discussion group for their valuable comments.This work has been supported by the National Nat-ural Science Foundation of China under Grant No.60772023, by the Open Fund of the State Key Lab-oratory of Software Development Environment underGrant No. BUAA-SKLSDE-09KF-04, Beijing Univer-sity of Aeronautics and Astronautics, by the NationalBasic Research Program of China (973 Program) un-der Grant No. 2005CB321901 and by the SpecializedResearch Fund for the Doctoral Program of Higher Ed-ucation (Nos. 20060006024 and 200800130006), Chi-nese Ministry of Education.

[1] Y. S. Kachanov, O. S. Ryzhov, and F. T. Smith, J.Fluid Mech. 251, 273 (1993); K. W. Chow, N. W. Ko,R. C. Leung, and S. K. Tang, Phys. Fluids 10, 1111(1998).

[2] M. P. Barnett, J. F. Capitani, J. von zur Gathen, andJ. Gerhard, Int. J. Quantum Chem. 100, 80 (2004);W. P. Hong, Phys. Lett. A 361, 520 (2007); B. Tianand Y. T. Gao, Phys. Lett. A 340, 243 (2005); 362, 283(2007).

[3] G. Das and J. Sarma, Phys. Plasmas 6, 4394 (1999);Y. T. Gao and B. Tian, Phys. Lett. A 349, 314 (2006);Phys. Plasmas 13, 112901 (2006); Phys. Plasmas(Lett.) 13, 120703 (2006); Europhys. Lett. 77, 15001(2007).

[4] T. Xu, B. Tian, L. L. Li, X. Lu, and C. Zhang, Phys.Plasmas 15, 102307 (2008).

[5] B. Tian and Y. T. Gao, Phys. Plasmas (Lett.) 12, 070703(2005); Eur. Phys. J. D 33, 59 (2005); Y. T. Gao andB. Tian, Phys. Lett. A 361, 523 (2007).

[6] Y. Kivshar and G. P. Agrawal, Optical Solitons, FromFibers to Photonic Crystals, Academic Press, NewYork 2003.

[7] K. Nakkeeran, K. Porsezian, P. S. Sundaram, andA. Mahalingam, Phys. Rev. Lett. 80, 1425 (1998).

[8] T. Brugarino and M. Sciacca, Opt. Commun. 262, 250(2006).

[9] B. Tian, W. R. Shan, C. Y. Zhang, G. M. Wei, and Y. T.Gao, Eur. Phys. J. B (Rapid Not.) 47, 329 (2005);B. Tian and Y. T. Gao, Phys. Lett. A 342, 228 (2005);359, 241 (2006).

[10] B. Tian, Y. T. Gao, and H. W. Zhu, Phys. Lett. A 366,223 (2007); W. J. Liu, B. Tian, H. Q. Zhang, L. L. Liand Y. S. Xue, Phys. Rev. E 77, 066605 (2008); W. J.Liu, B. Tian, and H. Q. Zhang, Phys. Rev. E 78, 066613(2008) .

[11] G. P. Agrawal, Nonlinear Fiber Optics, 3rd ed., Aca-demic Press, San Diego 2001.

[12] A. Hesegawa and F. D. Tappert, Appl. Phys. Lett. 23,142 (1973); L. F. Mollenauer, R. H. Stolen, and J. P.Gordon, Phys. Rev. Lett. 45, 1095 (1980).

[13] N. Sasa and J. Satsuma, J. Phys. Soc. Jpn. 60, 409(1991).

[14] A. Mahalingam and K. Porsezian, Phys. Rev. E 64,046608 (2001).

[15] J. Li, H. Q. Zhang, T. Xu, Y. X. Zhang, and B. Tian,J. Phys. A 40, 13299 (2007).

[16] Z. H. Li, L. Li, H. P. Tian, and G. S. Zhou, Phys. Rev.Lett. 84, 4096 (2000).

[17] D. Mihalache, L. Torner, F. Moldoveanu, N. C. Panoiu,and N. Truta, Phys. Rev. E 48, 4699 (1993).

[18] K. Porsezian, P. Shanmugha Sundaram, and A. Ma-halingam, Phys. Rev. E 50, 1543 (1994).

[19] Y. Kodama and A. Hasegawa, Phys. Rev. E 23, 510(1987).

[20] S. Ghosh, A. Kundu, and S. Nandy, J. Math. Phys. 40,1993 (1999).

[21] D. Anderson and M. Lisak, Phys. Rev. A 27, 1393(1983).

[22] H. H. Chen, Y. C. Lee, and C. S. Liu, Phys. Scr. 20, 490(1979).

[23] R. Hirota, J. Math. Phys. 14, 805 (1973).[24] A. Hasegawa and Y. Kodama, Solitons in Optical Com-

munications, Clarendon Press, Oxford 1995.[25] K. Porsezian, P. Shanmugha Sundaram, and A. Ma-

halingam, J. Phys. A 32, 8731 (1999).[26] M. Daniel and M. M. Latha, Physica A 298, 351

(2001).[27] M. J. Ablowitz and P. A. Clarkson, Solitons, Nonlin-

ear Evolution Equations, Inverse Scattering, CambrigeUniversity Press, Cambrige 1991.

Page 10: Soliton Solution, Backlund Transformation, and Conservation … · 2016-06-28 · Soliton Solution, Backlund Transformation, and Conservation Laws¨ for the Sasa-Satsuma Equation

300 Y. Liu et al. · Soliton Solution, Backlund Transformation, and Conservation Laws for the Sasa-Satsuma Equation

[28] P. A. Clarkson, IMA J. Appl. Math. 44, 27 (1990).[29] K. Porsezian, J. Phys. A 24, L337 (1991).[30] S. Ghosh and S. Nandy, Nucl. Phys. B 561, 451 (1999).[31] C. Gilson, J. Hietarinta, J. Nimmo, and Y. Ohta, Phys.

Rev. E 68, 016614 (2003).[32] J. Kim, Q. H. Park, and H. J. Shin, Phys. Rev. E 58,

6746 (1998).[33] M. J. Ablowitz, D. J. Kaup, A. C. Newell, and H. Segur,

Phys. Rev. Lett. 31, 125 (1973).[34] D. Mihalache, N. Truta, and L. C. Crasovan, Phys. Rev.

E 56, 1064 (1997).[35] J. Weiss, M. Tabor, and G. Carnevale, J. Math. Phys.

24, 522 (1983).[36] C. Y. Zhang, Y. T. Gao, T. Xu, L. L. Li, F. W. Sun, J. Li,

X. H. Meng, and G. M. Wei, Commun. Theor. Phys. 49,673 (2008).

[37] X. Lu, H. W. Zhu, X. H. Meng, Z. C. Yang, and B. Tian,J. Math. Anal. Appl. 336, 1305 (2007).

[38] X. H. Meng, B. Tian, T. Xu, H. Q. Zhang, and Q. Feng,Phys. A 388, 209 (2009).

[39] M. Wadati, H. Sanuki, and K. Konno, Prog. Theor.Phys. 53, 419 (1975).

[40] H. P. Tian, Z. H. Li, and G. S. Zhou, Opt. Commun.205, 221 (2002).

[41] J. P. Tian, and G. S. Zhou, Phys. Scr. 73, 56 (2006).[42] X. J. Shi, L. Li, R. Y. Hao, Z. H. Li, and G. S. Zhou,

Opt. Commun. 241, 185 (2004).[43] R. Grimshaw, K. Nakkeeran, C. K. Poon, and K. W.

Chow, Phys. Scr. 75, 620 (2007).[44] F. Fang and Y. Xiao, Opt. Commun. 268, 305 (2006).[45] G. I. Stegeman and M. Segev, Sci. 286, 1518 (1999).[46] T. Kanna, M. Lakshmanan, P. T. Dinda, and N. Akhme-

diev, Phys. Rev. E 73, 026604 (2006).[47] J. Yang, Phys. Rev. E 64, 026607 (2001).