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Darboux Transformation and Exact Solutions of the Continuous Heisenberg Spin Chain Equation

Ai-Hua Chenaand Fan-Fan Wangb

aCollege of Science, University of Shanghai for Science and Technology, Shanghai, 200093, People’s Republic of China

bDepartment of Mathematics, East China University of Science and Technology, Shanghai, 200237, People’s Republic of China

Reprint requests to F.-F. W.; E-mail:ffwang@ecust.edu.cn Z. Naturforsch.69a,9 – 16 (2014) / DOI: 10.5560/ZNA.2013-0067

Received March 11, 2013 / revised September 10, 2013 / published online October 30, 2013 In this paper, we give theN-fold Darboux transformation (DT) for the continuous Heisenberg spin chain which describes the motion of the isotropic ferromagnets in the complex case. By using this DT, we getN-soliton solutions and a new exact solution of the spin chain from a trivial seed solution and a plane wave seed solution, respectively.

Key words:Darboux Transformation; Heisenberg Spin Chain; Breather Solution; Rational Solution.

PACS numbers:02.30.Ik; 02.30.Jr

1. Introduction

In the 1970s, the continuous Heisenberg spin chain which describes the motion of the magnetization vec- tor of the isotropic ferromagnets has attracted much attention [1–4]. In [3], the explicit single-soliton so- lutions in the isotropic case were presented. In [4], the inverse scattering method was applied to the continu- ous Heisenberg spin chain and its Lax representation was obtained. In [5], the N-soliton solution was ob- tained by applying the Wadati gauge transformation to the inverse scattering problem of a nonlinear evolu- tion equation. In [6], theN-soltion solution was given explicitly according to the bilinear equations obtained by Hirota. Since the 1970s, the continuous Heisenberg spin chain also received much attention. In [7], the higher-order Heisenberg spin chain equations were de- duced by Chen and Li and they proved that these equa- tions are equivalent to the evolution equations of the Ablowitz–Kaup–Newell–Segur (AKNS) By using the nonlinearization method, Qiao [8] presented a finite- dimensional integrable system and the involutive so- lutions of the higher-order Heisenberg spin chain. In [9], the relation among the different systems associated with the Heisenberg magnetic equation was studied by the reduction procedure.

The Darboux transformation (DT) as a useful method to get explicit solutions of nonlinear partial differential equations has been utilized to obtain so- lutions of the continuous Heisenberg spin chain. In [10,11], for the spectral problem related to the con- tinuous Heisenberg spin chain, explicit one-fold Dar- boux transformations were constructed to obtain its soliton solutions. In [12], Cie´sli´nski and Czarnecka constructed the Darboux–Bäcklund transformation for the two-dimensional Heisenberg chain. In [13], Saleem and Hassan constructed the Darboux transformation for the generalized Heisenberg magnet model and ob- tained multi-soliton solutions in terms of quasidetermi- nants.

In [11], the soliton solutions were obtained for the continuous Heisenberg spin chain equation by the one- fold DT, and the iterative relationship between theNth solution and the (N+1)st solution can be derived by applying the one-fold DTNtimes. However, the rela- tionships between the new solutions and the seed solu- tions are not given. In this paper, according to the de- terminant representation of DT [14–17], we directly construct the N-fold Darboux transformation for the continuous Heisenberg spin chain by using a similar method as in [18]. By using of theN-fold DT, we can obtain the relationships between the new solutions and

© 2014 Verlag der Zeitschrift für Naturforschung, Tübingen·http://znaturforsch.com

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the seed solutions without tedious and complicated it- erations.

In this paper, we study the continuous Heisenberg spin chain introduced in [4], where Takhtajan consid- ered an infinite linear chain with spin-densitysj(x,t) for j=1,2,3 and length of the spins equal to 1, i.e.

s21(x,t) +s22(x,t) +s23(x,t) =1. The motion equation of the continuous Heisenberg spin chain is

St= 1

2i(SSxxSxxS), (1)

whereS=s1σ1+s2σ2+s3σ3, andσj(j=1,2,3)are the Pauli matrices

σ1=

0 1 1 0

, σ2=

0 −i

i 0

,

σ3=

1 0 0 −1

.

(2)

If we letw=s3andu=s1−is2, then from (1), we get ut=i(uwxx−wuxx), wt= i

2(uuxx−uuxx), (3) where w is a real-valued function, u is a complex- valued function, andudenotes the complex conjugate ofu. According to the length constraint condition, we have

|u|2+w2=1. (4)

In Section2, according to the spectral problems in [7–11], we give the Lax pair of (3) and (4). Then we construct the N-fold Darboux transformation for the Heisenberg spin chain (1). In Section3, using different seed solutions, we get exact solutions of (1). From the trivial seed solution, we get breather solutions for the first two components and soliton solution for the third component of the spin chain. These solutions are sim- ilar with those in [10,11]. From the plane wave seed solution, we get a new exact solution of the spin chain.

In Section4, we make our conclusion.

2. Darboux Transformation

The spectral problem of the system (3) and (4) (cf.

[7–11]) is given by φx==iλ

w u u −w

φ with |u|2+w2=1,

(5)

and the corresponding auxiliary spectral problem is given by

φt=Vφ (6)

= 2iwλ2+12(uuxuux 2iuλ2+ (wuxuwx 2iuλ2+ (uwx−wux −2iwλ212(uuxuux

! φ,

whereφ= (φ12)T.λis a constant spectral parameter, uandware functions ofxandt.

We want to find a transformation ¯φ=Tφ, such that the Lax pair

φx=, φt=Vφ (7) is transformed into

φ¯x=U¯φ¯, φ¯t=V¯φ¯, (8) where ¯U and ¯V have the same forms asU andV re- spectively, which are obtained by replacingu,u,w, ux,ux,wx with ¯u, ¯u, ¯w, ¯ux, ¯ux, ¯wx, respectively, inU andV. Then the matrixT satisfies

Tx+TU=U T¯ , Tt+TV=V T¯ . (9) According to the zero curvature equation, if(u,w)sat- isfies (3),(u,¯ w)¯ also satisfies (3). The transformation φ¯=Tφ is a Darboux transformation for the Lax pair (5) and (6).

In the following, we first construct the Darboux transformation for the Lax pair (5) and (6). Then we give the relationship between(u,w)and(u,¯w).¯

Firstly, the Lax pair (5) and (6) satisfies the loop group conditions

U(λ) =σ2U(λ)σ2, V) =σ2V(λ)σ2, (10) whereσ2 is the Pauli matrix defined in (2). Equation (10) implies thatT satisfiesT) =σ2T(λ)σ2(con- straints imposed by reduction groups, see [19–21]).

Then from (9), we have to demandT(0) =const. in order to preserve the conditionsU(0) =V(0) =0 and U(0) =¯ V¯(0) =0. For simplicity, we supposeT(0) =I.

So we let

T =

 1+

N

k=1

Akλk

N

k=1

Bkλk

N

k=1

Bkλk 1+

N

k=1

Akλk

(11)

(3)

whereAkandBk(1≤kN)are functions ofxandt. Let Φ(j) = (ϕ1j),ϕ2j))T and Ψ(j) = (ψ1j),ψ2j))T be two basic solutions of (5) and (6) withλ =λj (j=1,2, . . . ,N). ThenΦ(j) = (−ϕ2j),ϕ1j))T and Ψj = (−ψ2j),ψ1j))T be two basic solutions of (5) and (6) with λ =λj (j=1,2, . . . ,N). Ak and Bk (1≤kN) satisfy the following two algebraic systems:

N

k=1

(AkjBkjk=−1, (12)

N k=1

(−BkjAkjk=−ηj, (13)

where

ηj2j)−rjψ2j)

ϕ1j)−rjψ1j), 1≤ jN. (14) Note that complex λj and real rj should be suitably chosen such that the determinants of the coefficient matrices of systems (12) and (13) are nonzero and thus AkandBk(1≤kN)can be uniquely determined.

From the form ofT in (11), we find that detT(λ) = (|AN|2+|BN|2)

N

j=1

(λ−λj)(λ−λj), (15) which means that λj andλj are roots of detT(λ) = 0. At the same time, from T(0) = I, we know that detT(0) =1= (|AN|2+B2N)|λ1|22|2· · · |λN|2, i.e.

|AN|2+|BN|2= 1

1|22|2· · · |λN|2. (16) In the following theorem, we give the relationship between(u,w)and(u,¯ w).¯

Theorem 1. If(u,w)is a solution of (3) and (4),(u,¯ w)¯ with

¯

u=uA2NuB2N−2wANBN

|AN|2+|BN|2 ,u[N], w¯=w(|AN|2− |BN|2) +uANBN+uANBN

|AN|2+|BN|2 ,w[N]

(17)

is a new solution of (3) and (4), where AN and BN are determined by (12) and (13).

Proof. From (17), it can be verified by a straightfor- ward calculation that|u|¯2+w¯2=1. In order to prove that(u,¯ w)¯ is a new solution of (3), we need to verify the validity of (9).

Step 1: We verify the validity of the first part of (9), i.e.Tx+TU=U T¯ .

LetT−1=adj(T)/detT and (Tx+TU)·adj(T) =

f11(λ) f12(λ) f21(λ) f22(λ)

,F(λ). (18) A direct calculation shows that λ−1f11(λ), λ−1f12(λ),λ−1f21(λ), andλ−1f22(λ)are all 2Nth- order polynomials inλ, andF(λ) =σ2F(λ)σ2. By using (5), (12), (13), and (14), we get

ηjx=iuλj−2iwλjηj−iuλjη2j, 1≤jN. (19) We can verify thatλjandλj (1≤jN)are roots of

fkl(λ) =0 fork,l=1,2. Therefore, we have

(Tx+TU)·adj(T) =detT·P(λ) (20) withP(λ) =σ2P(λ)σ2, i.e.

P(λ) = p(1)11λ p(1)12λ

−p(1)12λ p(1)11

λ

!

, (21)

wherep(1)11 andp(1)12 are independent ofλ. We can fur- ther rewrite (20) as

Tx+TU=P(λ)T. (22)

Comparing the coefficients ofλN+1in (22), we find iwAN+iuBN=p(1)11ANp(1)12BN,

iuAN−iwBN=p(1)11BN+p(1)12AN.

(23) From (17) and (23), we have

p(1)11 =i ¯w, p(1)12 =i ¯u. (24) Then we obtainTx+TU=U T¯ .

Step 2: As in Step 1, we verify the validity of the second part of (9), i.e.Tt+TV=V T¯ similarly.

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LetT−1=adj(T)/detT and (Tt+TV)·adj(T) =

g11(λ) g12(λ) g21(λ) g22(λ)

,G(λ). (25) A direct calculation shows that λ−1g11(λ), λ−1g12(λ), λ−1g21(λ), and λ−1g22(λ) are all (2N + 1)st-order polynomials in λ and G(λ) = σ2G(λ)σ2. By using (6), (12), (13), and (14), we result in

ηjt=2iuλj2+ (uwxwuxj

4iwλ2j + (uuxuux) ηj

2iuλ2j+ (wuxuwxj

η2j, 1≤jN. (26)

We can verify thatλjandλj(1≤jN)are roots of gkl(λ) =0 fork,l=1,2. Therefore, we have

(Tt+TV)·adj(T) =detT·Q(λ) (27) withQ(λ) =σ2Q(λ)σ2, i.e.

Q(λ) = (28)

q(2)11λ2+q(1)11λ q(2)12λ2+q(1)12λ

−q(2)12λ2q(1)12λ q(2)11λ2+q(1)11λ

! ,

whereq(k)11 andq(k)12 (k=1,2)are independent ofλ. We can further rewrite (27) as

Tt+TV=Q(λ)T. (29)

Comparing the coefficients ofλN+2in (29), we get 2iwAN+2iuBN =q(2)11ANq(2)12BN, 2iuAN−2iwBN=q(2)11BN+q(2)12AN.

(30) From (17) and (30), we obtain

q(2)11 =2i ¯w, q(2)12 =2i ¯u. (31) If we further compare the coefficients ofλN+1of (29), by using (31), we have

1

2(uux−uxu)AN+2iwAN−1+ (uwxwux)BN (32) +2iuBN−1=q(1)11AN+2i ¯wAN−1q(1)12BN−2i ¯uBN−1,

−1

2(uuxuxu)BN−2iwBN−1+ (wux−wxu)AN +2iuAN−1=q(1)11BN+2i ¯wBN−1+q(1)12AN+2i ¯uAN−1.

According to step 1, by comparing the coefficients of λNinTx+TU=U T¯ , we find

ANx+iwAN−1+iuBN−1=i ¯wAN−1−i ¯uBN−1, BNx+iuAN−1−iwBN−1=i ¯wBN−1+i ¯uAN−1. (33)

By using (32), (33), and the expressions of ¯u and

¯

w, through tedious calculation (which can also be done easily by using the Mathematica software), we achieve

q(1)11 =1

2(u¯u¯xu¯u¯x), q(1)12 =1

2(w¯u¯xu¯w¯x). (34) Then we have Tt+TV =V T¯ . The proof is com- plete.

From Theorem1and the transformationw=s3,u= s1+is2, we find that

s¯1= (u¯+u¯)/2, s¯2=i(u¯−u¯)/2, s¯3=w¯ (35) is a new real-valued solution of the Heisenberg equa- tion (1).

In the following section, we will obtain exact so- lutions of (3) and (4) by the use of Theorem1. Then through (35), we will obtain real-valued exact solutions of the Heisenberg equation (1).

3. Exact Solutions

In this section, we will take a trivial solution and a plane wave solution as the seed solution, respectively, to obtain exact solutions of the Heisenberg equation (1).

3.1. Trivial Seed Solution

In this subsection, by using the N-fold Darboux transformation and taking a trivial solution as seed so- lution, we give the breather and soliton solutions of (1).

It is easy to see that(u,w) = (0,1)is a trivial solution of (3) and (4), and we take it as the seed solution. From (16) and (17), the solution of (3) and (4) is given by

u[N] =−2|λ1|22|2· · · |λN|2ANBN,

w[N] =1−2|λ1|22|2· · · |λN|2|BN|2. (36)

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From (35), we can obtain a series of solutions of the Heisenberg equation (1) which are given by

s1[N] = u[N] +u[N]

2 =−|λ1|22|2· · · |λN|2

·(ANBN+ANBN), s2[N] = i(u[N]−u[N])

2 =i|λ1|22|2· · · |λN|2

·(ANBNANBN),

s3[N] =w[N] =1−2|λ1|22|2· · · |λN|2|BN|2. (37) We choose two basic solutions of (5) and (6) as

ϕ(λj) = (ei(λjx+2λ2jt),0)T, ψ(λj) = (0,e−i(λjx+2λ2jt))T.

(38) For simplicity we letrj=−1(j=1,2, . . . ,N)in (14).

Then we have

ηj=e−2i(λjx+2λ2jt), j=1,2, . . . ,N. (39) From the linear system (12), (13) and the expression of (39), we find that ifλj(j=1,2, . . . ,N)are real, the obtained solutions are trivial. To get non-trivial solu- tions, we chooseλj(j=1,2, . . . ,N)as complex.

WhenN=1, takingλ11+iτ2, whereτ1andτ2

are real, the solution of (3) and (4) is u[1] =−e2i(τ1x+2(τ12−τ22)t)

τ1222

·h

22tanh(2τ2(x+4τ1t))−2iτ1τ2 i

·sech(2τ2(x+4τ1t)), w[1] =1− 2τ22

τ1222

sech2(2τ2(x+4τ1t)).

(40)

-2 -1

0 1

2 x

-0.4 -0.2

0 0.2

0.4

t -11-20

2

s1 1 -2

-1 0 x 1

(a)

-3 -2

-1 0 x

0 0.2

0.4 0.6

0.81 t -11-20

2

s2 1 -3

-2 x -1

(b)

-0.5 0 x 0.5

-0.2 -0.1

0 0.1

0.2

t -11-20

s3 1 -0.5

0 x 0.5

(c)

Fig. 1 (colour online). Plots of solution (41) of Heisenberg equation (1) whenτ1=1 andτ2=2.

Then a solution of the Heisenberg equation (1) is s1[1] = −1

τ1222 h

22tanh(2τ2(x+4τ1t))

·cos(2τ1x+4(τ12−τ22)t) +2τ1τ2sin(2τ1x+4(τ12−τ22)t)i

·sech(2τ2(x+4τ1t)), s2[1] = 1

τ1222 h

22tanh(2τ2(x+4τ1t)) (41)

·sin(2τ1x+4(τ12−τ22)t)

−2τ1τ2cos(2τ1x+4(τ12−τ22)t)i

·sech(2τ2(x+4τ1t)), s3[1] =1− 2τ22

τ1222

sech2(2τ2(x+4τ1t)).

For given values of τ1=1 and τ2=2, we give the plots of s1[1], s2[1], and s3[1] in Figure 1. We find that s3[1] is a bell-shaped single-soliton solu- tion, and s1[1] and s2[1] are single-soliton solutions with exchange interactions, i.e. they are breather so- lutions.

WhenN=2, for simplicity, taking λ11+iτ2, λ2=−τ1+iτ2, whereτ1andτ2are real, the solution of (3) and (4) is

u[2] =−4τ1τ2

θ12 h

θ2+2iτ1τ2(e1−e2)i

3+iθ4),

w[2] =1−8τ12τ22 θ12

·

(eα1+eα1+2α2)2+ (eα2+e12)2−2θ5 (42)

(6)

-2 0

x 2 -0.5

0 0.5 t -2

0 2 s1 2

-2 0 x 2

(a)

-2 0

x 2 -0.5

0 0.5 t -2

0 2 s2 2

-2 0 x 2

(b)

-1 0

x 1 -0.2

0 0.2 t -11-20

2 s3 2

-1 0 x 1

(c)

Fig. 2 (colour online). Plots of solution (43) of Heisenberg equation (1) whenτ1=1 andτ2=2.

and the solution of (1) is s1[2] =4τ1τ2

θ12

−θ2θ3+2τ1τ2(e1−e24 , s2[2] =4τ1τ2

θ12

θ2θ4+2τ1τ2(e1−e23 ,

s3[2] =1−8τ12τ22 θ12

(eα1+eα1+2α2)2 + (eα2+e12)2−2θ5

,

(43) where

θ1= (e1+1)(e2+1)τ12−(2 eα12cos(β1−β2)

−e1−e222,

θ2= (e1+1)(e2+1)τ12+ (2 eα12cos(β1−β2)

−e1−e222,

θ3= (eα2+e12)sinβ2−(eα1+eα1+2α2)sinβ1, θ4= (eα2+e12)cosβ2−(eα1+eα1+2α2)cosβ1, θ5= (eα1+eα1+2α2)(eα2+e12)cos(β1−β2) with

α1=2τ2(x+4τ1t), β1=−2(τ1x+2 τ12−τ22)t , α2=2τ2(x−4τ1t), β2=2(τ1x−2(τ12−τ22)t).

For given values ofτ1=1 andτ2=2, we give the plots of (43) in Figure2. We find thats1[2]ands2[2]

are two head-on breather solutions, ands3[2]is a bell- shaped two-soliton solution.

3.2. Plane Wave Seed Solution

In this subsection, by the modified Darboux trans- formation method [22–24], we can get rational solu- tions of (3) and (4) by the one-fold Darboux transfor- mation. Then, new exact solutions of (1) can be ob- tained.

In order to get rational solutions, we take a plane wave solution as the seed solution. It is easy to see that(u,w) = (bei(2x+4at),a)satisfies (3), wherea and b(b6=0)are real. To satisfy (4), we havea2+b2=1.

Taking(u,w)as the seed solution, we suppose that the basic solutions of (5) and (6) have the following forms:

φ1(λ),φ1(x,t)

= (a1x+b1t+c1xt+d1)ei(x+2at), φ2(λ),φ2(x,t)

= (a2x+b2t+c2xt+d2)e−i(x+2at),

(44)

whereai,bi,ci, anddi(i=1,2)are complex, andλ= a+ib. Substituting (44) into the Lax pair (5) and (6) and comparing all the coefficients, we have

a1=ia2,b1= (−2b+4ia)a2, b2= (4a+2ib)a2,

c1=c2=0,d2=a−ib

b a2−id1.

(45)

In order to preserve the positivity of|φ1|2+|φ2|2and get some solutions with simple forms, we choosea2= i,d1=a−ib

2b . Then, φ1(x,t) =h

x−(4a+2ib)t+a−ib 2b

i

ei(x+2at), φ2(x,t) =h

ix−(2b−4ia)t+b+ia 2b

i

e−i(x+2at). (46)

For simplicity, we letr1=0 in (14), and we get η1(λ),η1(x,t) =φ2(x,t)

φ1(x,t)

=

ix−(2b−4ia)t+b+ia 2b

−x−(4a+2ib)t+a−ib 2b

e−2i(x+2at). (47)

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-2 -1

0 1

2

x -5

-2.5 0 52.5

t -1-2210 s1 1

-2 -1

0 1

2

x -1-210

(a)

-2 0

2 x -5

-2.5 0 52.5

t -1-2210 s2 1

-2 0

2 x -1-210

(b)

-1 0

1 x -1

-0.5 0 0.5 1

t -1

0 1 s3 1

-1 0

1 x -1

0 1

(c)

Fig. 3 (colour online). Plots of solution (51) of Heisenberg equation (1).

Then from the linear systems (12) and (13), we ob- tain

A1=−a−ib+ (a+ib)|η1|2

1+|η1|2 , B1= 2ibη1

1+|η1|2. (48) From (16) and (17), the solution of (3) and (4) is given by

u[1] =uA21uB21−2wA1B1,

w[1] =w(|A1|2− |B1|2) +uA1B1+uA1B1. (49)

Now from (35), we obtain the solution of the Heisen- berg equation (1) which is given by

s1[1] =1 2 h

u(A21B12) +u(A12−B21)

−2w(A1B1+A1B1)i , s2[1] =i

2 h

u(A21+B12)−u(A12+B21)

−2w(A1B1A1B1)i ,

s3[1] =w(|A1|2− |B1|2) +uA1B1+uA1B1.

(50)

If we further leta=0, b=1, the solution of the Heisenberg equation (1) is

s1[1] =− h

(4x2+16t2+1)2−32x2i

cos 2x−8x(4x2+16t2−1)sin 2x (4x2+16t2+1)2 , s2[1] =

8x(4x2+16t2−1)cos 2x+h

(4x2+16t2+1)2−32x2 i

sin 2x (4x2+16t2+1)2 , s3[1] =− 64xt

(4x2+16t2+1)2.

(51)

The plots of (51) are given in Figure3. Note that s3[1]is a rational solution. To the best of our knowledge, (51) is a new solution of the Heisenberg equation (1).

Since the seed solution is related toλ, we cannot ap- ply theN-fold DT whenN=2,3, . . .. Although we can iterate the one-fold DT to get new solutions, it would be much more complicated.

4. Conclusions

In this paper, we construct the N-fold DT of the Heisenberg equation (1). By the use of the obtained DT, from the trivial seed solution (u,w) = (0,1), we get breather solutions for the first two components and

soliton solution for the third component of the spin chain (s1,s2,s3). From the plane wave seed solution (u,w) = (bei(2x+4at),a)witha2+b2=1, we get a new exact solution of the spin chain(s1,s2,s3). Particularly, the third component of the spin chain is a rational so- lution.

Acknowledgements

We are most grateful to the anonymous referee for pointing out much relevant literature and crucial help in improving the original manuscript. The work de- scribed in this paper was supported by the Fundamen- tal Research Funds for the Central Universities.

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