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Journal of Natural Sciences Research www.iiste.org 
ISSN 2224-3186 (Paper) ISSN 2225-0921 (Online) 
Vol.3, No.15, 2013 
Study of Anisotropy Superconductor using Time-Dependent 
Ginzburg-Landau Equation 
Fuad Anwar1,2*, Pekik Nurwantoro1, Arief Hermanto1 
1. Department of Physics, University of Gadjah Mada, Sekip Utara, Bulaksumur, Yogyakarta 55281, 
Indonesia 
2. Department of Physics, University of Sebelas Maret, Jl. Ir. Sutami 36A, Kenthingan, Surakarta 57126, 
Indonesia 
* E-mail of the corresponding author: fuada70@yahoo.com 
Abstract 
We have observed an anisotropy superconductor which was immersed in vacuum medium in presence of an 
applied magnetic field. The anisotropy properties of superconductor were related with two principal values of the 
effective mass of the Cooper pairs, namely mc along the x-axis and mab in the yz-plane. Based on the time-dependent 
Ginzburg-Landau and yU methods, the problem was solved and made to be the numerical simulation. 
From study using this numerical simulation, we can find that the anisotropy properties can make the critical field 
to be lower or higher. 
Keywords: anisotropy, superconductor, time-dependent Ginzburg-Landau 
1. Introduction 
It is well known that the Time Dependent Ginzburg - Landau (TDGL) equations can be used to study the 
dynamics of superconductivity phenomenon (Tinkham 1996; Du 2005). These equations have nonlinear nature, 
so it will give results more completely to solve them numerically (Du 2005). One of the numerical solutions has 
been developed using the gauge invariant variables technique or to be called yU method (Bolech et al. 1995; 
Gropp et al. 1996; Winiecki & Adams 2002). In the last decade, the solution of TDGL equations using yU 
method has successfully been used to study the dynamics of superconductivity phenomenon in thin films (Barba 
et al. 2007; Barba et al. 2008; Barba-Ortega & Aguiar 2009; Barba-Ortega et al. 2010; Barba-Ortega et al. 2012; 
Barba-Ortega et al. 2013; Wisodo et al. 2013). However, these studies considered the superconductors having 
isotropy properties. 
It is also well known that the high Tc superconductors have anisotropy properties (Tinkham, 1996). These 
superconductors are viewed as the stack of layers, each layer comprises the ab planes and the c axis is normal to 
them. The effective mass of the Cooper pairs is different when measured in the ab planes or along the c axis. The 
results in earlier papers show that the anisotropy properties have influence on superconductivity phenomenon 
(Hao & Hu 1996; Chapman & Richardson 1998; Achalere & Dey 2008). 
In this paper, we study the dynamics of superconductivity phenomenon in an anisotropy superconductor using 
the TDGL equations and yU methods. We describe the theoretical formalism and numerical method used for 
solving the problem in section 2. The results and their analysis are discussed in section 3. Finally, we conclude in 
section 4. 
2. Numerical Methods 
2.1 The Time-dependent Ginzburg-Landau Equations 
The time-dependent Ginzburg-Landau (TDGL) equations are : 
m 
y y y y y s 
99 
(1) 
(2) 
e 
i 
ö 
æ 
ö 
( ) ( ) ( t ) ( t ) T ( t ) t ( t ) 
m 
Φ t t 
e 
i 
æ 
¶ 
m D t 
s 
s 
s 
s 
, , ( ) , ( , ) , 
2 
, , 
2 
2 
2 2 2 
r r r r r A r r y y b y a y y - + ÷ ÷ø 
ç çè 
- Ñ = ÷ ÷ø 
ç çè 
+ 
¶ 
h 
h 
h 
h 
( ( ) ( )) 
Ñ´ Ñ´ - 
A r H r 
( ) ( ) ( ) ( ) ( ) ( ) ( ) ( ) 
ö 
÷ø 
æ 
çè 
¶ 
÷ø 
ö 
¶ 
+ - Ñ - æ 
e 
= Ñ - Ñ - 
çè 
t 
t 
t t Φ t 
ie 
t t t t 
s 
m i 
t t 
s 
s 
ext 
, 
, , , 
2 
, , , , 
2 
, , 
1 
2 
0 
0 
A r 
r r r r r A r r 
m 
h 
h
Journal of Natural Sciences Research www.iiste.org 
ISSN 2224-3186 (Paper) ISSN 2225-0921 (Online) 
Vol.3, No.15, 2013 
where y is order parameter, A and Hext denote the vector potential and an external magnetic field, es and ms are 
the effective charge and the effective mass of the Cooper pairs, a dan b are phenomenological parameters, D is a 
phenomenological diffusion constant, F and s are the electrical potential and conductivity (Bolech et al. 1995; 
Tinkham 1996; Gropp et al. 1996; Winiecki & Adams 2002). 
In this study, we considered an anisotropic superconductor which is immersed in vacuum medium in presence of 
an applied magnetic field (The figure 1). Here, an anisotropic superconductor has layered structures, so it has 
two principal values of ms, D and s, namely : mc, Dc and sc 
ö 
æ 
¶ 
2 2 
ö 
æ 
¶ 
y y 
2 
2 2 
2 2 2 2 
ö 
æ 
¶ 
y y ay by y 
ö 
æ 
¶ 
2 2 
2 2 2 2 
æ 
¶ 
æ 
¶ 
- 
¶ 
¶ 
ö 
¶ 
- 
y x y x 
100 
along the x-axis and mab, Dab and sab in the yz-plane. 
The applied magnetic field is assumed in the z-direction, time-dependent, and spatially uniform, so we have 
Ñ´Hext(t)=0, B=Bz(x,y,t)z and A=Ax(x,y,t)x+Ay(x,y,t)y. 
Figure. 1 An anisotropy superconductor in presence of an applied perpendicular uniform magnetic field 
If we apply the previous assumption to the time-dependent Ginzburg-Landau, we can obtain : 
(3) 
(4) 
æ 
¶ 
m m 
e 
e 
A 
¶ 
A 
s 
æ 
æ 
¶ 
¶ 
æ 
¶ 
Then, we scale y in y0=(|a|/b)½, t in tc 
= xc 
ö 
A 
A 
¶ 
¶ 
2/Dc, x and y in xc 
2 
ö 
¶ 
+ 
¶ 
+ 
ö 
A 
¶ 
Φ 
A 
¶ 
Φ 
ö 
æ 
ö 
ö 
æ 
ö 
=(ћ2/2mc|a|)½, Ax and Ay in A0x=μ0Hc2c xc 
, F in 
F0= xc 
A0x/ tc 
, sc 
and sab in s0c=1/( μ0 kc 
2Dc), and we choose F =0, so we can rewrite equations (3) and (4) in the 
following form : 
superconductor 
x 
z 
y 
Hext(t) 
y y ay by y 
2 2 
- + ÷ ÷ø 
ç çè 
- 
¶ 
+ ÷ø 
çè 
- 
¶ 
+ 
- + ÷ ÷ø 
ç çè 
- 
¶ 
+ ÷ø 
çè 
- 
¶ 
= 
÷ø 
çè 
+ 
¶ 
+ ÷ø 
çè 
+ 
¶ 
y 
s 
ab 
x 
s 
ab 
y 
s 
c 
x 
s 
c 
s 
ab ab 
s 
c c 
A 
e 
i 
m y 
A 
e 
i 
m x 
A 
e 
i 
m y 
A 
e 
i 
m x 
Φ 
e 
i 
m D t 
Φ 
e 
i 
m D t 
h 
h 
h 
h 
h 
h 
h 
h 
h 
h 
h 
h 
y 
t 
y 
A y 
ie 
im y y 
x 
t 
x 
A x 
ie 
im x x 
y 
y 
x 
x 
x 
y 
x 
y 
y 
y ab 
s 
ab 
x 
x c 
s 
c 
s 
ˆ ˆ 
2 
2 
ˆ ˆ 
2 
2 
ˆ 
1 
ˆ 
1 
2 
2 
0 0 
÷ ÷ 
ø 
ç ç 
è 
¶ 
¶ 
- ÷ ÷ø 
ç çè 
- 
¶ 
- 
¶ 
+ 
÷ø 
çè 
¶ 
¶ 
- ÷ø 
çè 
- 
¶ 
- 
¶ 
= 
÷ ÷ 
ø 
ç ç 
è 
¶ 
¶ 
¶ 
- ÷ ÷ 
ø 
ç ç 
è 
¶ 
¶ 
¶ 
y s 
y 
y 
y 
y 
y s 
y 
y 
y 
y 
h 
h 
h 
h
Journal of Natural Sciences Research www.iiste.org 
ISSN 2224-3186 (Paper) ISSN 2225-0921 (Online) 
Vol.3, No.15, 2013 
æ + 
+ ÷ø 
2 2 
2 2 
ö 
æ 
ö 
æ + 
= 
ö 
e e 2 
¶ 
æ 
¶ 
¶ 
æ + 
1 1 1 m D iA 
÷ + - ÷ø 
¶ 
c m 2m 
m = = 
l 
k = = 
c x 
Hc = Hc = 
a k 
2c c ab ab k 
l 
x 
2 = = = ab 
= = 
m 
2 
2 
2 
m Hc 
ab 
D D 
s 
ab 
s 
ò x x + = - 
( ( ) ) x y 
x 
i j U i A y d i N j N i 
, ò h h + = - 
exp , with = 1,2,…, +1 and = 1,2,…, 1 
- + 
y y y 
U t t t U t t 
( ) ( ) 2 ( ) ( ) ( ) 
+ - - 
, 1, , 1, 1, 
2 
x 
y y y 
æ 
æ 
- + 
U t t t U t t 
t 
, , 1 , , 1 , 1 
ö 
101 
(5) 
(6) 
y e 
¶ 
A 
¶ 
A 
In equations (5) and (6), we define : 
(7a) 
(7b) 
(7c) 
(7d) 
(7e) 
(7f) 
(7g) 
e 
ö 
¶ 
- 
A 
¶ 
- 
¶ 
A 
A 
¶ 
A 
1 
ö 
æ 
¶ 
ö 
¶ 
æ 
¶ 
æ 
¶ 
ö 
æ 
¶ 
b 
b 
ab 
c 
m 
2 
2 
ab 
c 
ab 
ab 
c 
ab 
where x is the coherence length, l is the penetration depth, and k is the Ginzburg-Landau parameter. 
The equations (5) and (6) can be solved by the yU method (Bolech et al. 1995; Gropp et al. 1996; Winiecki & 
Adams 2002). In this method, the sample is divided into Nx x Ny cells, with mesh spacings Dx 
and Dy. At the cell, 
there are three fundamental unknowns, namely y, Ux and Uy. The yi,j is order parameter at position (xi , yj), with i 
= 1,2,…Nx+1 and j = 1,2,…,Ny+1. The Ux and Uy are the complex link variables and are related to A by : 
(8a) 
(8b) 
x 
x x j 
Using the yU method and the Euler method and taking eD = 1, es = 1, sc 
=sab = 1, the equations (5) and (6) can 
be derived in the following form : 
(9) 
y ( y y) 
e 
y 
e 
e e 
2 
2 
2 
2 
2 2 
21 
ö 
ç çè 
- 
¶ 
÷ ÷ 
ø 
ç ç 
è 
ö 
çè 
- 
¶ 
÷ ÷ 
ø 
ç ç 
è 
¶ 
÷ ÷ 
ø 
ç ç 
è 
y 
m 
m 
x 
m 
m 
m D 
y 
iA 
t x 
y 
y 
x 
x 
i A y 
i y y 
x 
y 
x 
y 
i A x 
i x x 
y 
t 
x 
t 
y x 
y c 
m 
y x 
x c 
y 
ab 
x 
c 
2 ˆ ˆ 
2 
1 
2 ˆ ˆ 
2 
ˆ ˆ 
2 2 
2 
2 2 
÷ ÷ 
ø 
ç ç 
è 
¶ 
¶ 
¶ 
+ ÷ ÷ø 
ç çè 
- 
¶ 
- 
¶ 
+ 
÷ ÷ 
ø 
ç ç 
è 
¶ 
¶ 
¶ 
- ÷ø 
çè 
- 
¶ 
- 
¶ 
= 
¶ 
+ 
¶ 
y k 
y 
y 
y 
y 
e 
y k 
y 
y 
y 
s s y 
a 
x 
a 
x 
ab 
ab 
c 
and 
2 
2 
2 
2 
2 h h 
= = 
and 
2 
0 
2 
2 
0 
2 
m a 
l 
m a 
l 
s 
ab 
s 
c 
e 
e 
and 
2 
2 
2 
2 
ab 
ab 
c 
l 
k 
x 
2 
and 
2 
0 
2 
0 
m b 
a k 
m b 
c 
c 
c 
ab 
c 
Hc 
m 
2 
2 
2 
k 
l 
x 
e 
c 
D = 2 e 
c 
es = 2 
( ( ) ) exp , with = 1,2,…, and = 1,2,…, +1 1 
, x y 
i 
y 
y y i 
y 
i j U i A x d i N j N j 
j 
y 
1 ( ) ( ) 
æ 
1 
+ 
2 
ö 
( ) ( ) 2 ( ) ( ) ( ) 
( ) ( ) 
, 
2 
2 , 
2 
2 
, , 
e 
t t t 
t t t t 
i j i j 
m 
m 
i j 
y 
i j i j i j 
y 
i j 
i j 
x 
i j i j i j 
x 
i j 
i j i j 
y y 
e 
y y 
÷ø ö 
çè æ 
- ÷ ÷ 
ø 
ç ç 
è 
+ D 
ö 
÷ ÷ ÷ 
ø 
ç ç ç 
è 
D 
+ D 
÷ ÷ ÷ 
ø 
ç ç ç 
è 
D 
+ D = + D 
+ - -
Journal of Natural Sciences Research www.iiste.org 
ISSN 2224-3186 (Paper) ISSN 2225-0921 (Online) 
Vol.3, No.15, 2013 
+ D = - D 
( ) ˆ ( ) ˆ ( ) Im ( ) ( ) ( ) ˆ 
U t t x U t x i tU t U t t t x 
, , , , , 1, 
U t (L t L t )x 
D 
t 
y 
( ) ( ) ( ) Im ( ) ( ) ( ) ˆ 
U t U t t t y 
, , 2 , , , , 1 
i j i j L =U U U U » -iDxDyB + + 
é 
× - Ñ - ψ 
¶ 
B B y x 
ext z z ¶ 
j j y = y 
y = x 
y + 
y = y 
y 
i i y = y 
y i N + 
i N exp( ) 1, 2, 1, 1 1, ext;z 
U y 
»U y 
U x 
+ 
U x 
-iDxDyH j j 
j 
j 
» - D D + + 
y 
N j U U U U i x yH 
x 
i U »U U U -iDxDyH + 
» - D D + + 
x 
i N U U U U i x yH 
102 
(10) 
(11) 
where, 
(12) 
( ) 
D 
t 
2.2 The Boundary Conditions 
In this study, we considered the superconductor is immersed in vacuum medium in presence of an applied 
magnetic field, so we have the boundary condition for y and A, namely : 
(13) 
(14) 
ù 
A 
A 
where n denotes the unit normal to the superconductor–vacuum interface. 
If we apply the previous research assumptions and scale y in y0=(|a|/b)½, x and y in xc 
=(ћ2/2mc|a|)½, Ax and Ay in 
A0x=μ0Hc2c xc 
, Bz and Bext;z in μ0Hc2c, Hz and Hext;z in 
Hc2c, then we can use the yU method and the Euler method 
to rewrite equations (13) and (14) in the following form : 
at i = 1 : 
(15a) 
at i = Nx+1 : 
(15b) 
at j = 1 : 
(15c) 
at j = Ny+1 : 
(15d) 
and 
at i = 1 : 
(16a) 
at i = Nx+1 : 
(16b) 
at j = 1 : 
(16c) 
at j = Ny+1 : 
(16d) 
x 
2.3 The Numerical Simulation 
We begin the numerical simulation with determining the value of Nx, Ny, Dx, Dy, Dt, kc 
and em . We also assume 
the initial condition of superconductor as in a perfect Meissner state, so we have Hext;z=0, yi,j = 1, Ux 
i,j=1 and 
Uy 
i,j=1. Then, Hext;z is increased linearly with time and with small intervals of DHext;z. When we have a new value 
of Hext;z , we compute the new values of yi,j, Ux 
i,j and Uy 
i,j using equations (9), (10), (11), (15) and (16). 
Using this numerical simulation, we can also make magnetization curves. Magnetization can be calculated from : 
(17) 
where Mz is scaled in Hc2c and Bz is calculated by equation (12). 
i j i j 
x 
c i j 
i j i j 
x 
i j 
x 
i j 
x 
i j 
x 
i j 
( ) ( ) ( ) 1 ˆ 
2 , , , 1 
2 
- 
D 
- 
- 
+ 
k 
y y 
( ) 
( )( ( ) ( ) 1)ˆ 
2 , , 1, 
2 
U t L t L t y 
x 
i t 
U t t U t 
i j i j 
y 
c i j 
i j i j 
y 
i j 
y 
i j 
m 
y 
i j 
y 
i j 
- 
D 
- 
D 
+ D = - 
- 
+ 
k 
y y 
e 
y 
y 
x 
x 
exp( ) , 1, i , j 
i , j 
1 i , j 
z;i, j 
0 ˆ = úû 
êë 
e 
i s n A 
h 
y 
x 
¶ 
- 
¶ 
= = ; 
( ) ( ) ( ) 1, 1, 2, t U t t j 
( ) ( ) ( ) 1, , , t U t t N j 
N j N j x x x 
( ) ( ) ( ) ,1 ,1 ,2 t U t t i 
( ) ( ) ( ) , 1 , , t U t t 
y y y i N 
y 
x 
x 
exp( ) 1, N , j 
N , j 
1 N , j 
ext;z 
x x x x 
y 
y 
x 
exp( ) ,1 i 
1,1 i 
,1 i 
,2 ext;z 
y 
y 
x 
exp( ) , 1 i 1, N 
i , N 
i , N 
ext;z 
y y y y 
z z ext z M B H ; = -
Journal of Natural Sciences Research www.iiste.org 
ISSN 2224-3186 (Paper) ISSN 2225-0921 (Online) 
Vol.3, No.15, 2013 
3. Results and Discussion 
We try to run the numerical simulation with choosing five cases, namely : em = 1.0, em = 0.5, em = 0.8, em = 1.3, 
and em = 2.0. For each case, the values of another input are the same, namely : Nx = 32, Ny = 32, Dx 
103 
=0.5, Dy 
=0.5, 
Dt = 0.010, DHext;z= 0.000001, and kc 
= 2.0. When em = 1.0, it is the isotropy superconductor case and the others 
are the anisotropy superconductor cases. 
In figure 2(a), we show the square modulus order parameter curve as a function of magnetic field - Hext 2 y in 
the five cases. We can see in the figure, the |y(x,y)|2 will completely vanish at the higher value of the applied 
field Hext;z when the value of em increases. It means, by increasing em the value of the surface nucleation field Hc3 
will be higher. 
In figure 2(b), we show the magnetization curve as a function of magnetic field M-Hext in the five cases. We can 
see, as increasing the applied field Hext;z, the magnetization curve will decrease until the minimum value, then 
increase until the zero value. When the value of em increases, we find that the minimum value will be located at 
the higher value of the applied field Hext;z if em£1 and at the lower value of the applied field Hext;z if em³1. We 
also find that the zero value will be located at the higher value of the applied field Hext;z when the value of em 
increases. It means, by increasing em, if em£1 the value of the lower critical field Hc1 will be higher and if em³1 
the value of Hc1 will be lower. It also means, by increasing em, the value of Hc3 will be higher. 
We show the distribution of the square modulus order parameter |y(x,y)|2 on sample for five cases and for the 
several values of the applied field Hext;z in the figure 3-7. From these figures, we can see that in the low applied 
field Hext;z, |y(x,y)|2 has a high value. As increasing Hext;z, the magnetic field will penetrate into sample to form 
vortex and |y(x,y)|2 will decrease. When the value of em increases, we find that |y(x,y)|2 will vanish in the higher 
value of the applied field Hext;z, the vortex is formed in the higher value of the applied field Hext;z if em£1 and in 
the lower value of the applied field Hext;z if em³1. Once again, these results mean that by increasing em, the value 
of Hc3 will be higher, if em£1 the value of Hc1 will be higher and if em³1 the value of Hc1 will be lower. 
0 0.5 1 1.5 2 2.5 3 3.5 
0 
- 0.1 
- 0.2 
Hext 
M 
(b) 
Hext 
2 y 
0 0.5 1 1.5 2 2.5 3 3.5 
0.8 
0.6 
0.4 
0.2 
0 
(a) 
Figure 2. Plot of (a) ext -H 2 y and (b) M-Hext in the cases of : 
— : em = 0.5 — : em = 0.8 — : em = 1.0 — : em = 1.3 — : em = 2.0
Journal of Natural Sciences Research www.iiste.org 
ISSN 2224-3186 (Paper) ISSN 2225-0921 (Online) 
Vol.3, No.15, 2013 
Figure 3. Plot of |y(x,y)|2 in the case of em=0.5 and (a)Hext;z=0.10 (b)Hext;z=0.20 (c)Hext;z=0.30 (d)Hext;z=0.40 
(e)Hext;z=0.50 (f)Hext;z=0.80 
The white and the black colours indicate |y(x,y)|2=1 and |y(x,y)|2=0. 
Figure 4. Plot of |y(x,y)|2 in the case em=0.8 and (a)Hext;z=0.10 (b)Hext;z=0.20 (c)Hext;z=0.30 (d)Hext;z=0.40 
(e)Hext;z=0.50 (f)Hext;z=0.80 (g) Hext;z=1.60 
The white and the black colours indicate |y(x,y)|2=1 and |y(x,y)|2=0. 
Figure 5. Plot of |y(x,y)|2 in the case of em=1.0 and (a)Hext;z=0.10 (b)Hext;z=0.20 (c)Hext;z=0.30 (d)Hext;z=0.40 
(e)Hext;z=0.50 (f)Hext;z =0.80 (g) Hext;z=1.60 (h) Hext;z=2.20. 
The white and the black colours indicate |y(x,y)|2=1 and |y(x,y)|2=0. 
104
Journal of Natural Sciences Research www.iiste.org 
ISSN 2224-3186 (Paper) ISSN 2225-0921 (Online) 
Vol.3, No.15, 2013 
Figure 6. Plot of |y(x,y)|2 in the case of em=1.3 and (a)Hext;z=0.10 (b)Hext;z=0.20 (c)Hext;z=0.30 (d)Hext;z=0.40 
(e)Hext;z=0.50 (f)Hext;z =0.80 (g)Hext;z=1.60 (h)Hext;z=2.20 (i)Hext;z=2.80. 
The white and the black colours indicate |y(x,y)|2=1 and |y(x,y)|2=0. 
Figure 7. Plot of |y(x,y)|2 in the case of em=2.0 and (a)Hext;z=0.10 (b)Hext;z=0.20 (c)Hext;z=0.30 (d)Hext;z=0.40 
(e)Hext;z=0.50 (f)Hext;z =0.80 (g)Hext;z=1.60 (h)Hext;z=2.20 (i)Hext;z=2.80 (j)Hext;z=3.50 
The white and the black colours indicate |y(x,y)|2=1 and |y(x,y)|2=0. 
4. Conclusion 
We have made a numerical solution of the Time Dependent Ginzburg - Landau (TDGL) equations for 
anisotropic superconductor using yU methods. From this simulation, if we set kc 
105 
in the fixed value and 
increase em, we will obtain the value of Hc3 will be higher and the value of Hc1 will be higher if em£1and 
will be lower if em³1. 
Acknowledgements 
We thank to Direktorat Jenderal Pendidikan Tinggi (Ditjen Dikti)-Kementerian Pendidikan dan 
Kebudayaan (Kemdikbud)-Indonesia for the support of our research through BPPS scholarship. 
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Superconducting Films, Physical Review B, 52, 22, R15719-R15722. 
Chapman, S. J., & Richardson, G. (1998). Motion and Homogenization of Vortices in Anisotropic Type II 
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Du, Q. (2005). Numerical Approximations of The Ginzburg–Landau Models for Superconductivity. J. Math. 
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Orientation. Jurnal of Law Temperature Physics, 104, 3/4, 265-274. 
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Square of Variable Surface. Physica C, 470, 206-211. 
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Behaviors for Homogeneous Type II Superconductors. Physica C, 492, 75-79. 
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Winiecki, T., & Adams, C. S. (2002). A Fast Semi-Implicit Finite Difference Method for The TDGL Equations. 
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Antivortex Pair in Mesoscopic Superconductor. Journal of Natural Sciences Research, 3, 9, 140-146. 
106
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Study of Anisotropy Superconductor using Time-Dependent Ginzburg-Landau Equation

  • 1. Journal of Natural Sciences Research www.iiste.org ISSN 2224-3186 (Paper) ISSN 2225-0921 (Online) Vol.3, No.15, 2013 Study of Anisotropy Superconductor using Time-Dependent Ginzburg-Landau Equation Fuad Anwar1,2*, Pekik Nurwantoro1, Arief Hermanto1 1. Department of Physics, University of Gadjah Mada, Sekip Utara, Bulaksumur, Yogyakarta 55281, Indonesia 2. Department of Physics, University of Sebelas Maret, Jl. Ir. Sutami 36A, Kenthingan, Surakarta 57126, Indonesia * E-mail of the corresponding author: fuada70@yahoo.com Abstract We have observed an anisotropy superconductor which was immersed in vacuum medium in presence of an applied magnetic field. The anisotropy properties of superconductor were related with two principal values of the effective mass of the Cooper pairs, namely mc along the x-axis and mab in the yz-plane. Based on the time-dependent Ginzburg-Landau and yU methods, the problem was solved and made to be the numerical simulation. From study using this numerical simulation, we can find that the anisotropy properties can make the critical field to be lower or higher. Keywords: anisotropy, superconductor, time-dependent Ginzburg-Landau 1. Introduction It is well known that the Time Dependent Ginzburg - Landau (TDGL) equations can be used to study the dynamics of superconductivity phenomenon (Tinkham 1996; Du 2005). These equations have nonlinear nature, so it will give results more completely to solve them numerically (Du 2005). One of the numerical solutions has been developed using the gauge invariant variables technique or to be called yU method (Bolech et al. 1995; Gropp et al. 1996; Winiecki & Adams 2002). In the last decade, the solution of TDGL equations using yU method has successfully been used to study the dynamics of superconductivity phenomenon in thin films (Barba et al. 2007; Barba et al. 2008; Barba-Ortega & Aguiar 2009; Barba-Ortega et al. 2010; Barba-Ortega et al. 2012; Barba-Ortega et al. 2013; Wisodo et al. 2013). However, these studies considered the superconductors having isotropy properties. It is also well known that the high Tc superconductors have anisotropy properties (Tinkham, 1996). These superconductors are viewed as the stack of layers, each layer comprises the ab planes and the c axis is normal to them. The effective mass of the Cooper pairs is different when measured in the ab planes or along the c axis. The results in earlier papers show that the anisotropy properties have influence on superconductivity phenomenon (Hao & Hu 1996; Chapman & Richardson 1998; Achalere & Dey 2008). In this paper, we study the dynamics of superconductivity phenomenon in an anisotropy superconductor using the TDGL equations and yU methods. We describe the theoretical formalism and numerical method used for solving the problem in section 2. The results and their analysis are discussed in section 3. Finally, we conclude in section 4. 2. Numerical Methods 2.1 The Time-dependent Ginzburg-Landau Equations The time-dependent Ginzburg-Landau (TDGL) equations are : m y y y y y s 99 (1) (2) e i ö æ ö ( ) ( ) ( t ) ( t ) T ( t ) t ( t ) m Φ t t e i æ ¶ m D t s s s s , , ( ) , ( , ) , 2 , , 2 2 2 2 2 r r r r r A r r y y b y a y y - + ÷ ÷ø ç çè - Ñ = ÷ ÷ø ç çè + ¶ h h h h ( ( ) ( )) Ñ´ Ñ´ - A r H r ( ) ( ) ( ) ( ) ( ) ( ) ( ) ( ) ö ÷ø æ çè ¶ ÷ø ö ¶ + - Ñ - æ e = Ñ - Ñ - çè t t t t Φ t ie t t t t s m i t t s s ext , , , , 2 , , , , 2 , , 1 2 0 0 A r r r r r r A r r m h h
  • 2. Journal of Natural Sciences Research www.iiste.org ISSN 2224-3186 (Paper) ISSN 2225-0921 (Online) Vol.3, No.15, 2013 where y is order parameter, A and Hext denote the vector potential and an external magnetic field, es and ms are the effective charge and the effective mass of the Cooper pairs, a dan b are phenomenological parameters, D is a phenomenological diffusion constant, F and s are the electrical potential and conductivity (Bolech et al. 1995; Tinkham 1996; Gropp et al. 1996; Winiecki & Adams 2002). In this study, we considered an anisotropic superconductor which is immersed in vacuum medium in presence of an applied magnetic field (The figure 1). Here, an anisotropic superconductor has layered structures, so it has two principal values of ms, D and s, namely : mc, Dc and sc ö æ ¶ 2 2 ö æ ¶ y y 2 2 2 2 2 2 2 ö æ ¶ y y ay by y ö æ ¶ 2 2 2 2 2 2 æ ¶ æ ¶ - ¶ ¶ ö ¶ - y x y x 100 along the x-axis and mab, Dab and sab in the yz-plane. The applied magnetic field is assumed in the z-direction, time-dependent, and spatially uniform, so we have Ñ´Hext(t)=0, B=Bz(x,y,t)z and A=Ax(x,y,t)x+Ay(x,y,t)y. Figure. 1 An anisotropy superconductor in presence of an applied perpendicular uniform magnetic field If we apply the previous assumption to the time-dependent Ginzburg-Landau, we can obtain : (3) (4) æ ¶ m m e e A ¶ A s æ æ ¶ ¶ æ ¶ Then, we scale y in y0=(|a|/b)½, t in tc = xc ö A A ¶ ¶ 2/Dc, x and y in xc 2 ö ¶ + ¶ + ö A ¶ Φ A ¶ Φ ö æ ö ö æ ö =(ћ2/2mc|a|)½, Ax and Ay in A0x=μ0Hc2c xc , F in F0= xc A0x/ tc , sc and sab in s0c=1/( μ0 kc 2Dc), and we choose F =0, so we can rewrite equations (3) and (4) in the following form : superconductor x z y Hext(t) y y ay by y 2 2 - + ÷ ÷ø ç çè - ¶ + ÷ø çè - ¶ + - + ÷ ÷ø ç çè - ¶ + ÷ø çè - ¶ = ÷ø çè + ¶ + ÷ø çè + ¶ y s ab x s ab y s c x s c s ab ab s c c A e i m y A e i m x A e i m y A e i m x Φ e i m D t Φ e i m D t h h h h h h h h h h h h y t y A y ie im y y x t x A x ie im x x y y x x x y x y y y ab s ab x x c s c s ˆ ˆ 2 2 ˆ ˆ 2 2 ˆ 1 ˆ 1 2 2 0 0 ÷ ÷ ø ç ç è ¶ ¶ - ÷ ÷ø ç çè - ¶ - ¶ + ÷ø çè ¶ ¶ - ÷ø çè - ¶ - ¶ = ÷ ÷ ø ç ç è ¶ ¶ ¶ - ÷ ÷ ø ç ç è ¶ ¶ ¶ y s y y y y y s y y y y h h h h
  • 3. Journal of Natural Sciences Research www.iiste.org ISSN 2224-3186 (Paper) ISSN 2225-0921 (Online) Vol.3, No.15, 2013 æ + + ÷ø 2 2 2 2 ö æ ö æ + = ö e e 2 ¶ æ ¶ ¶ æ + 1 1 1 m D iA ÷ + - ÷ø ¶ c m 2m m = = l k = = c x Hc = Hc = a k 2c c ab ab k l x 2 = = = ab = = m 2 2 2 m Hc ab D D s ab s ò x x + = - ( ( ) ) x y x i j U i A y d i N j N i , ò h h + = - exp , with = 1,2,…, +1 and = 1,2,…, 1 - + y y y U t t t U t t ( ) ( ) 2 ( ) ( ) ( ) + - - , 1, , 1, 1, 2 x y y y æ æ - + U t t t U t t t , , 1 , , 1 , 1 ö 101 (5) (6) y e ¶ A ¶ A In equations (5) and (6), we define : (7a) (7b) (7c) (7d) (7e) (7f) (7g) e ö ¶ - A ¶ - ¶ A A ¶ A 1 ö æ ¶ ö ¶ æ ¶ æ ¶ ö æ ¶ b b ab c m 2 2 ab c ab ab c ab where x is the coherence length, l is the penetration depth, and k is the Ginzburg-Landau parameter. The equations (5) and (6) can be solved by the yU method (Bolech et al. 1995; Gropp et al. 1996; Winiecki & Adams 2002). In this method, the sample is divided into Nx x Ny cells, with mesh spacings Dx and Dy. At the cell, there are three fundamental unknowns, namely y, Ux and Uy. The yi,j is order parameter at position (xi , yj), with i = 1,2,…Nx+1 and j = 1,2,…,Ny+1. The Ux and Uy are the complex link variables and are related to A by : (8a) (8b) x x x j Using the yU method and the Euler method and taking eD = 1, es = 1, sc =sab = 1, the equations (5) and (6) can be derived in the following form : (9) y ( y y) e y e e e 2 2 2 2 2 2 21 ö ç çè - ¶ ÷ ÷ ø ç ç è ö çè - ¶ ÷ ÷ ø ç ç è ¶ ÷ ÷ ø ç ç è y m m x m m m D y iA t x y y x x i A y i y y x y x y i A x i x x y t x t y x y c m y x x c y ab x c 2 ˆ ˆ 2 1 2 ˆ ˆ 2 ˆ ˆ 2 2 2 2 2 ÷ ÷ ø ç ç è ¶ ¶ ¶ + ÷ ÷ø ç çè - ¶ - ¶ + ÷ ÷ ø ç ç è ¶ ¶ ¶ - ÷ø çè - ¶ - ¶ = ¶ + ¶ y k y y y y e y k y y y s s y a x a x ab ab c and 2 2 2 2 2 h h = = and 2 0 2 2 0 2 m a l m a l s ab s c e e and 2 2 2 2 ab ab c l k x 2 and 2 0 2 0 m b a k m b c c c ab c Hc m 2 2 2 k l x e c D = 2 e c es = 2 ( ( ) ) exp , with = 1,2,…, and = 1,2,…, +1 1 , x y i y y y i y i j U i A x d i N j N j j y 1 ( ) ( ) æ 1 + 2 ö ( ) ( ) 2 ( ) ( ) ( ) ( ) ( ) , 2 2 , 2 2 , , e t t t t t t t i j i j m m i j y i j i j i j y i j i j x i j i j i j x i j i j i j y y e y y ÷ø ö çè æ - ÷ ÷ ø ç ç è + D ö ÷ ÷ ÷ ø ç ç ç è D + D ÷ ÷ ÷ ø ç ç ç è D + D = + D + - -
  • 4. Journal of Natural Sciences Research www.iiste.org ISSN 2224-3186 (Paper) ISSN 2225-0921 (Online) Vol.3, No.15, 2013 + D = - D ( ) ˆ ( ) ˆ ( ) Im ( ) ( ) ( ) ˆ U t t x U t x i tU t U t t t x , , , , , 1, U t (L t L t )x D t y ( ) ( ) ( ) Im ( ) ( ) ( ) ˆ U t U t t t y , , 2 , , , , 1 i j i j L =U U U U » -iDxDyB + + é × - Ñ - ψ ¶ B B y x ext z z ¶ j j y = y y = x y + y = y y i i y = y y i N + i N exp( ) 1, 2, 1, 1 1, ext;z U y »U y U x + U x -iDxDyH j j j j » - D D + + y N j U U U U i x yH x i U »U U U -iDxDyH + » - D D + + x i N U U U U i x yH 102 (10) (11) where, (12) ( ) D t 2.2 The Boundary Conditions In this study, we considered the superconductor is immersed in vacuum medium in presence of an applied magnetic field, so we have the boundary condition for y and A, namely : (13) (14) ù A A where n denotes the unit normal to the superconductor–vacuum interface. If we apply the previous research assumptions and scale y in y0=(|a|/b)½, x and y in xc =(ћ2/2mc|a|)½, Ax and Ay in A0x=μ0Hc2c xc , Bz and Bext;z in μ0Hc2c, Hz and Hext;z in Hc2c, then we can use the yU method and the Euler method to rewrite equations (13) and (14) in the following form : at i = 1 : (15a) at i = Nx+1 : (15b) at j = 1 : (15c) at j = Ny+1 : (15d) and at i = 1 : (16a) at i = Nx+1 : (16b) at j = 1 : (16c) at j = Ny+1 : (16d) x 2.3 The Numerical Simulation We begin the numerical simulation with determining the value of Nx, Ny, Dx, Dy, Dt, kc and em . We also assume the initial condition of superconductor as in a perfect Meissner state, so we have Hext;z=0, yi,j = 1, Ux i,j=1 and Uy i,j=1. Then, Hext;z is increased linearly with time and with small intervals of DHext;z. When we have a new value of Hext;z , we compute the new values of yi,j, Ux i,j and Uy i,j using equations (9), (10), (11), (15) and (16). Using this numerical simulation, we can also make magnetization curves. Magnetization can be calculated from : (17) where Mz is scaled in Hc2c and Bz is calculated by equation (12). i j i j x c i j i j i j x i j x i j x i j x i j ( ) ( ) ( ) 1 ˆ 2 , , , 1 2 - D - - + k y y ( ) ( )( ( ) ( ) 1)ˆ 2 , , 1, 2 U t L t L t y x i t U t t U t i j i j y c i j i j i j y i j y i j m y i j y i j - D - D + D = - - + k y y e y y x x exp( ) , 1, i , j i , j 1 i , j z;i, j 0 ˆ = úû êë e i s n A h y x ¶ - ¶ = = ; ( ) ( ) ( ) 1, 1, 2, t U t t j ( ) ( ) ( ) 1, , , t U t t N j N j N j x x x ( ) ( ) ( ) ,1 ,1 ,2 t U t t i ( ) ( ) ( ) , 1 , , t U t t y y y i N y x x exp( ) 1, N , j N , j 1 N , j ext;z x x x x y y x exp( ) ,1 i 1,1 i ,1 i ,2 ext;z y y x exp( ) , 1 i 1, N i , N i , N ext;z y y y y z z ext z M B H ; = -
  • 5. Journal of Natural Sciences Research www.iiste.org ISSN 2224-3186 (Paper) ISSN 2225-0921 (Online) Vol.3, No.15, 2013 3. Results and Discussion We try to run the numerical simulation with choosing five cases, namely : em = 1.0, em = 0.5, em = 0.8, em = 1.3, and em = 2.0. For each case, the values of another input are the same, namely : Nx = 32, Ny = 32, Dx 103 =0.5, Dy =0.5, Dt = 0.010, DHext;z= 0.000001, and kc = 2.0. When em = 1.0, it is the isotropy superconductor case and the others are the anisotropy superconductor cases. In figure 2(a), we show the square modulus order parameter curve as a function of magnetic field - Hext 2 y in the five cases. We can see in the figure, the |y(x,y)|2 will completely vanish at the higher value of the applied field Hext;z when the value of em increases. It means, by increasing em the value of the surface nucleation field Hc3 will be higher. In figure 2(b), we show the magnetization curve as a function of magnetic field M-Hext in the five cases. We can see, as increasing the applied field Hext;z, the magnetization curve will decrease until the minimum value, then increase until the zero value. When the value of em increases, we find that the minimum value will be located at the higher value of the applied field Hext;z if em£1 and at the lower value of the applied field Hext;z if em³1. We also find that the zero value will be located at the higher value of the applied field Hext;z when the value of em increases. It means, by increasing em, if em£1 the value of the lower critical field Hc1 will be higher and if em³1 the value of Hc1 will be lower. It also means, by increasing em, the value of Hc3 will be higher. We show the distribution of the square modulus order parameter |y(x,y)|2 on sample for five cases and for the several values of the applied field Hext;z in the figure 3-7. From these figures, we can see that in the low applied field Hext;z, |y(x,y)|2 has a high value. As increasing Hext;z, the magnetic field will penetrate into sample to form vortex and |y(x,y)|2 will decrease. When the value of em increases, we find that |y(x,y)|2 will vanish in the higher value of the applied field Hext;z, the vortex is formed in the higher value of the applied field Hext;z if em£1 and in the lower value of the applied field Hext;z if em³1. Once again, these results mean that by increasing em, the value of Hc3 will be higher, if em£1 the value of Hc1 will be higher and if em³1 the value of Hc1 will be lower. 0 0.5 1 1.5 2 2.5 3 3.5 0 - 0.1 - 0.2 Hext M (b) Hext 2 y 0 0.5 1 1.5 2 2.5 3 3.5 0.8 0.6 0.4 0.2 0 (a) Figure 2. Plot of (a) ext -H 2 y and (b) M-Hext in the cases of : — : em = 0.5 — : em = 0.8 — : em = 1.0 — : em = 1.3 — : em = 2.0
  • 6. Journal of Natural Sciences Research www.iiste.org ISSN 2224-3186 (Paper) ISSN 2225-0921 (Online) Vol.3, No.15, 2013 Figure 3. Plot of |y(x,y)|2 in the case of em=0.5 and (a)Hext;z=0.10 (b)Hext;z=0.20 (c)Hext;z=0.30 (d)Hext;z=0.40 (e)Hext;z=0.50 (f)Hext;z=0.80 The white and the black colours indicate |y(x,y)|2=1 and |y(x,y)|2=0. Figure 4. Plot of |y(x,y)|2 in the case em=0.8 and (a)Hext;z=0.10 (b)Hext;z=0.20 (c)Hext;z=0.30 (d)Hext;z=0.40 (e)Hext;z=0.50 (f)Hext;z=0.80 (g) Hext;z=1.60 The white and the black colours indicate |y(x,y)|2=1 and |y(x,y)|2=0. Figure 5. Plot of |y(x,y)|2 in the case of em=1.0 and (a)Hext;z=0.10 (b)Hext;z=0.20 (c)Hext;z=0.30 (d)Hext;z=0.40 (e)Hext;z=0.50 (f)Hext;z =0.80 (g) Hext;z=1.60 (h) Hext;z=2.20. The white and the black colours indicate |y(x,y)|2=1 and |y(x,y)|2=0. 104
  • 7. Journal of Natural Sciences Research www.iiste.org ISSN 2224-3186 (Paper) ISSN 2225-0921 (Online) Vol.3, No.15, 2013 Figure 6. Plot of |y(x,y)|2 in the case of em=1.3 and (a)Hext;z=0.10 (b)Hext;z=0.20 (c)Hext;z=0.30 (d)Hext;z=0.40 (e)Hext;z=0.50 (f)Hext;z =0.80 (g)Hext;z=1.60 (h)Hext;z=2.20 (i)Hext;z=2.80. The white and the black colours indicate |y(x,y)|2=1 and |y(x,y)|2=0. Figure 7. Plot of |y(x,y)|2 in the case of em=2.0 and (a)Hext;z=0.10 (b)Hext;z=0.20 (c)Hext;z=0.30 (d)Hext;z=0.40 (e)Hext;z=0.50 (f)Hext;z =0.80 (g)Hext;z=1.60 (h)Hext;z=2.20 (i)Hext;z=2.80 (j)Hext;z=3.50 The white and the black colours indicate |y(x,y)|2=1 and |y(x,y)|2=0. 4. Conclusion We have made a numerical solution of the Time Dependent Ginzburg - Landau (TDGL) equations for anisotropic superconductor using yU methods. From this simulation, if we set kc 105 in the fixed value and increase em, we will obtain the value of Hc3 will be higher and the value of Hc1 will be higher if em£1and will be lower if em³1. Acknowledgements We thank to Direktorat Jenderal Pendidikan Tinggi (Ditjen Dikti)-Kementerian Pendidikan dan Kebudayaan (Kemdikbud)-Indonesia for the support of our research through BPPS scholarship. References Achalere, A. & Dey, B. (2008). Effect of c-axis Anisotropy on the Properties of High-Tc Superconductor Films of Finite Thickness. Physica C, 468, 2241-2249. Barba, J. J., Cabral, L. R. E. & Aguiar, J. A. (2007). Vortex Arrays in Superconducting Cylinders. Physica C,
  • 8. Journal of Natural Sciences Research www.iiste.org ISSN 2224-3186 (Paper) ISSN 2225-0921 (Online) Vol.3, No.15, 2013 460-462, 1272-1273. Barba, J. J., de Souza Silva, C. C., Cabral, L. R. E. & Aguiar, J. A. (2008). Flux Trapping and Paramagnetic Effects in Superconducting Thin Films : The Role of de Gennes Boundary Conditions. Physica C, 468, 718-721. Barba-Ortega, J. & Aguiar, J. A. (2009). De Gennes Parameter Limit for The Occurrence of a Single Vortex in a Square Mesoscopic Superconductor. Physica C, 469, 754-755. Barba-Ortega, J., Becerra, A. & Aguiar, J. A. (2010). Two Dimensional Vortex Structures in a Superconductor Slab at Low Temperatures. Physica C, 470, 225-230. Barba-Ortega, J., Sardella, E., Aguiar, J. A. & Brandt, E. H. (2012). Vortex State in a Mesoscopic Flat Disk with Rough Surface. Physica C, 479, 49-52. Barba-Ortega, J., Sardella, E. & Aguiar, J. A. (2013). Triangular Arrangement of Defects in a Mesoscopic Superconductor. Physica C, 485, 107-114. Bolech, C., Buscaglia, G. C. & Lopez, A. (1995). Numerical Simulation of Vortex Arrays in Thin Superconducting Films, Physical Review B, 52, 22, R15719-R15722. Chapman, S. J., & Richardson, G. (1998). Motion and Homogenization of Vortices in Anisotropic Type II Superconductors. SIAM J. APPL. MATH., 58, 2, 587-606. Du, Q. (2005). Numerical Approximations of The Ginzburg–Landau Models for Superconductivity. J. Math. Phys., 46, 095109-1 - 095109-22. Gropp, W. D., Kaper, H. G., Leaf, G. K., Levine, D. M., Palumbo, M., & Vinokur, V. M. (1996). Numerical Simulation of Vortex Dynamics in Type-II Superconductors, Journal of Computational Physics, 123, 254-266. Hao, Z. & Hu, C. R. (1996). Flux Motion in Anisotropic Type II Superconductors near Hc2 with Arbitrary Vortex Orientation. Jurnal of Law Temperature Physics, 104, 3/4, 265-274. Pascolati, M. C. V., Sardella, E. & Lisboa-Filho, P. N. (2010). Vortex Dynamics in Mesoscopic Superconducting Square of Variable Surface. Physica C, 470, 206-211. Presotto, A., Sardella, E. & Zadorosny, R. (2013). Study of The Threshold Line between Macroscopic and Bulk Behaviors for Homogeneous Type II Superconductors. Physica C, 492, 75-79. Tinkham, M. (1996). Introduction to Superconductivity. (2nd ed.). New York : McGraw-Hill, Inc. Winiecki, T., & Adams, C. S. (2002). A Fast Semi-Implicit Finite Difference Method for The TDGL Equations. Journal of Computational Physics, 179, 127-139. Wisodo, H., Nurwantoro, P., & Utomo, A. B. S. (2013). Voltage Curve for Annihilation Dynamics of A Vortex- Antivortex Pair in Mesoscopic Superconductor. Journal of Natural Sciences Research, 3, 9, 140-146. 106
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