Материал: Маслов ИНТРОДУЦТИОН ТО ПХЫСИЦС ОФ СЕЦОНД-ОРДЕР МАГНЕТИЦ 2015

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can denote

 

as

 

, the same for all j . Then the term

σjz

σz

/

 

 

 

 

 

in

the

 

Hamiltonian

 

takes

the

form

 

Jij σiz

σjz

 

 

 

i, j

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

/

 

 

 

N

N

 

Recall that Jij

= J (Ri Rj )= J (Rl ),

σz

 

Jij σiz

= σz ∑∑Jij σiz .

 

 

i, j

 

 

 

 

i=1

ji

 

 

 

 

 

 

 

 

where Rl

= Ri

Rj

is the vector drawn from j-th magnetic moment to i-

th, and convert the sum to in the interaction term

 

 

 

 

 

 

 

 

 

ji

l 0

 

 

 

 

 

 

 

 

 

 

 

 

N N

 

 

 

 

N

/

 

 

(11.7)

 

 

 

 

 

σz ∑∑J

(Ri Rj )σiz = σz

∑∑

 

J (Rl

)σiz ,

 

 

 

 

 

 

i=1

ji

 

 

 

 

i=1 l

 

 

 

 

where / is the sum for all vectors Rl

that drawn from arbitrary atom

 

 

 

l

 

 

 

 

 

 

 

 

 

 

 

 

 

(magnetic moment) to all other atoms (magnetic moments), the prime implies that Rl 0. This sum is the same for every atom, since we con-

sider that all atoms (magnetic moments) located periodically, i.e., they form the crystal. Thus, the interaction term takes the following form

 

/

 

N

 

where

/

J (Rl ) is the certain characteristic en-

σz

 

J (Rl )σiz ,

 

 

l

 

 

i=1

 

l

 

 

ergy (sum of the energies of exchange interactions of randomly selected atom with all other atoms). Taking into account that J (Rl ) falls off ex-

ponentially as the Rl increases, denote the J (Rl )= J for the nearest neighbors and considering that J (Rl )= 0 for other atoms, we obtain / J (Rl )zJ, where z is the number of nearest neighbors of each

l

 

atom (magnetic moment). Since J = (0.001÷0.1) eV, zJ

may take the

sufficiently large values zJ = (0.1÷1) eV. Denote this energy as

/ J (Rl )= kBθ,

(11.8)

l

 

26

where θ is the some characteristic temperature (next, we shall omit the Boltzmann constant).

Thus, taking into account the notation introduced, we can write down the Hamiltonian of the Ising model in the following form

 

 

N

N

= E0

 

N

(11.9)

H = E0′ −

σz

θσiz hσiz

(θ σz

+ h)σiz .

 

 

i=1

i=1

 

 

i=1

 

Denote the “effective field” heff

 

 

. So, the Hamiltonian of the

= h + θ σz

Ising model can be described as

N

 

 

 

 

 

 

E0′ − heff

 

 

(11.10)

 

 

H =

σiz .

 

i=1

The main differences between this Hamiltonian and the Hamiltonian

 

N

are the appearance

of noniteracting magnetic moments H0

= −hσiz

i=1

of the constant E0(note that E0does not affect on the σz calculation)

and the field h substituted by the “effective field” heff = h + θσz .

Finally, in the mean-field approximation system of interacting magnetic moments can be approximately described as the system of nonin-

teracting magnetic moments placed into the “effective field” heff h.

12. Curie-Weiss equation and Curie-Weiss law

We now apply the mean-field approximation to the system of magnetic moments with Jij 0 (i, j) . In particular, we assume Jij = J

for the nearest neighbors and Jij = 0 for other atomic pairs. Magnetization of such system (projection on the z-axis) equals to

 

 

 

 

N

 

 

 

 

 

 

 

 

M =

µz

=

NµB x

,

(12.1)

 

 

 

 

V

V

 

 

 

 

 

 

where

µB . The parameter x does not depend on i ,

x = σz

= µz

1x 1, and x = 0 in the case of µz = 0. Let us find x = x(T, H ).

27

Recall that the Hamiltonian of the Ising model in the mean-field approximation is

 

N

(12.2)

H

= E0′ − heff σiz .

i=1

N

Constant E0does not affect on the σz calculation, term heff σiz is

i=1

the operators sum of the interaction between each magnetic moment and “effective field”. In other words, in our approximation magnetic moments do not depend on each other, but they located in the “effective

field” heff . Therefore, the value σz for arbitrary magnetic moment can be obtained in terms of single magnetic moment located in the field

heff . Hamiltonian for the single moment located in the field

 

 

 

 

 

can be obtained as follows

H

= −heff σz . Therefore

σz

 

 

 

 

 

H T

 

 

 

 

 

 

)

 

 

 

 

Tr (σze

 

 

 

)

 

 

Tr (σze

 

 

 

 

 

 

ˆ

 

 

heff σz T

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

σz =

 

 

 

 

 

 

 

=

 

 

 

 

 

 

=

 

 

 

Tr

(eH T )

 

 

 

Tr (eheff σz

T )

 

 

 

 

eheff

T

eheff

T

 

heff

 

 

 

 

=

 

 

 

 

 

 

 

= tanh

 

 

 

.

 

 

 

 

h

T

+ e

h

T

 

T

 

 

 

 

e eff

 

 

eff

 

 

 

 

 

 

 

heff is

(12.3)

Recall that the heff = h + θσz h + θx . Therefore the Eq. (12.3) takes the form

h + θx

(12.4)

x = tanh

T

 

 

 

 

Such dependence of x is referred to as Curie-Weiss equation.

Let us find the magnetization and magnetic susceptibility at high

temperatures T h + xθ . At high temperatures

h + θx

h + θx

,

tanh

T

 

T

 

 

 

 

 

 

 

therefore

x h + θx

. Finally, we obtain

 

 

 

 

 

 

 

T

 

 

 

 

 

 

 

28

x =

 

 

h

 

 

 

=

 

µB H

,

 

 

(12.5)

 

T −θ

 

T −θ

 

 

 

 

 

 

 

 

 

 

 

 

 

M =

Nµ

B

x

=

 

Nµ2

H

,

(12.6)

 

 

 

 

 

 

 

 

 

 

B

 

 

 

 

 

 

V

 

 

 

 

V

 

T

−θ

 

 

 

 

 

 

 

 

 

 

 

 

 

 

χ =

M

 

=

 

NµB2

1

 

.

 

(12.7)

H

 

 

 

V

 

 

 

T −θ

 

The latter temperature dependence of χ is referred to as Curie-Weiss law. Note that if the exchange interaction is absent ( Jij = 0 ), then

θ = 0 , so, we obtain the Curie law. The value θ is called the Curie temperature.

13. Ferromagnetic transition in the Ising model. Curie temperature. Order parameter

In the previous paragraph we have shown that at high temperatures

magnetic susceptibility χ =

NµB2

1

. One can see that the value of χ

 

V

 

 

T −θ

diverges at T → ∞.

This is due to a violation of the conditions of ap-

plicability

of our solution. Indeed, we obtained that x =

µB H

, i.e.,

T −θ

 

T → θ.

 

 

 

 

 

 

 

 

 

 

 

x → ∞ at

Therefore

the

condition

T h + xθ

is

not

valid.

However,

one can

see that

some

“critical”

temperature

θ

exists at

which something happens. Maybe it is a transition to ferromagnetic state? Let us study the Curie-Weiss equation in more detail.

Consider the h = 0 in the Curie-Weiss equation, thus the latter takes the following form

 

θ

(13.1)

x = tanh x

 

.

 

 

T

 

This equation can not be solved analytically. We shall try to solve it graphically. From the Fig. 13.1 and 13.2 one can see that at T > θ the Curie-Weiss equation has only one solution ( x = 0 ), but at T < θ it has three solutions ( x = 0; x 0 ).

29

Fig. 13.1. Graphic solution of the Curie-Weiss equation at T > θ

Fig. 13.2. Graphic solution of the Curie-Weiss equation at T < θ

Thus, the main conclusion is that at T = θ = / J (Rl )(10 ÷1000) K

l

the phase transition into ferromagnetic state occurs, i.e., at T > θ and H = 0 we obtain M = 0 (paramagnetic phase), and at T < θ and H = 0

30

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