namely |
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Ψ |
0 |
= |
+1,+1,+1 |
+1 |
+1,+1 ≡ |
↑,↑,↑ ↑ ↑,↑ . The |
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slightest excitement will be |
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↑,↑,↑ ↓ ↑,↑ , |
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1 |
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≡ |
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" " |
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+1, |
i ≠ k; |
Therefore for the energy |
E1 we obtain |
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i.e., σiz = |
i = k. |
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−1, |
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E1 = − 1 ∑ |
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N |
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/ Jij σiz σjz |
= −1 ∑Jij σiz σjz = |
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i≠ j |
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1 ∑Jij σiz σjz |
− 1 ∑J j σ zσjz − |
1 ∑Ji |
σizσ z = |
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ij≠≠ |
+1 |
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= −1 |
∑Jij |
+ 1 ∑J j + 1 ∑Ji = − 1 |
∑Jij − |
1 ∑J j − |
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2 i≠ j |
2 j≠ |
2 i≠ |
2 i≠ j |
2 j≠ |
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ij≠≠ |
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− 1 ∑Ji + ∑J j + ∑Ji = − 1 ∑/ Jij + 2∑J j . |
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2 i≠ |
j≠ |
i≠ |
2 i, j |
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Finally, for the energy of the first excited state we find
E1 = E0 + 2θ.
(15.9)
(15.10)
Thus, the energy spectrum has the gap, i.e., the first excited level of energy is separated from the ground level by 2θ.
16. Free energy of a ferromagnet in the Ising model
Helmholtz free energy is defined as F = E −TS , where E is the internal energy of the system and S is the entropy. Note that there is heat exchange with the environment (T = const ), the free energy must be
minimal. The internal energy can be described as E =
Hˆ
. Taking into
36
account |
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that |
Hamiltonian |
in |
the |
Ising |
model |
is |
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∑ |
/ |
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, for internal energy we obtain |
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H = − |
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Jij σiz σjz − h∑σiz |
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2 i, j |
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i |
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E = − |
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Jij |
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(16.1) |
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σiz σjz |
σiz . |
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2 i, j |
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i |
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Considering the mean-field approximation (see § 11) we can rewrite the mean of the product as the product of the means
σiz σjz
≈
σiz 
σjz
.
Taking into account that
σiz
= x is the order parameter, we obtain for the internal energy
E = − |
1 ∑/ Jij x2 − h∑x = −1 x2 |
∑∑Jij − xh∑1 = |
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i j≠i |
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(16.2) |
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x2 |
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= − |
Nθ− xhN. |
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2 |
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Let us find the entropy |
S = ln Γ , where |
Γ is the number of possible |
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states of the system at a given temperature (here and after we omit the Boltzmann constant). Denote N↑ and N↓ as the number of magnetic
moments aligned along or against the selected axis z, respectively.
Therefore the total number |
of magnetic moments is equal to |
N = N↑ + N↓ . The difference |
N↑ − N↓ defines the total magnetic mo- |
ment of the system, i.e., magnetization:
µB N↑ +(−µB )N↓ = µB (N↑ − N↓ ).
On the other hand, the total magnetic moment of the system can be de-
scribed as |
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N = xµB N . Thus, we can rewrite the order |
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µiz |
N = µB σiz |
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parameter in the following form |
N↑ − N↓ |
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x = |
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(16.3) |
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N |
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Actually, if N↑ = N↓ , then x = 0 , therefore the order is missing; on the
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= 0 x =1; |
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other hand, if |
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then the “apple-pie order” |
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x = −1, |
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37
is presented. Since x = x(T ), the difference N↑ − N↓ depends on tem-
perature as well. This fact imposes a limitation on Γ, i.e., the number of possible states of the system at a given temperature implies the number of possible states of the system at a given difference N↑ − N↓ . Let us
find the Γ
Γ = CNN↑ = |
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N ! |
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= |
N ! |
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= CNN↓ . |
(16.4) |
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N↑ |
!(N − N↑ )! |
N↑ !N↓ ! |
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Taking into account the Stirling’s formula ln(n!)≈ nln n −n we obtain for the entropy
S = ln Γ = ln (N !)−ln (N↑ !)−ln (N↓ !)≈ |
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≈ N ln |
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ln |
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= N |
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Express |
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and |
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= |
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N − N↓ |
− |
N↓ |
=1− 2 |
N↓ |
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Finally, for the entropy we obtain |
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S = −N |
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ln |
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1− x |
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38
Note that at x = 0 (no order), S = N ln 2 , so, Γ = 2N – every magnetic moment has an arbitrary direction. Ultimately the Helmholtz free energy is described as
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1+ x |
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1+ x |
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1− x |
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1− x |
(16.9) |
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F = N − |
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θ− xh +T |
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ln |
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In general, we must include in the Eq. (16.9) the term F0 (T, H ), which
does not depend on the order parameter, i.e., it is not associated with magnetic subsystem, but includes phonon contribution, etc.
So, we obtained F = F (x,T, H ). Let us find F = F (T, H ). To do this, we should find x = x(T, H ) from the conditions of F = F (x,T, H )
minimum at T = const and H = const . So, let us find |
∂F (x,T, H ) |
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∂F0 |
(T, H ) |
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considering that |
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= N −xθ− h + |
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= |
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∂x |
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= N −xθ− h + |
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ln |
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− x |
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From the condition on the extremum ∂F (x,T, H ) = 0 , we obtain
∂x
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T |
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ln |
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1− x |
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(xθ+h) =1+ x; |
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eT |
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2(xθ+h)
x = eT2 (xθ+h) −1;
eT +1
x = tanh xθT+ h .
Finally, we obtain the Curie-Weiss equation for the order parameter. We already know that this equation for H = 0 and T > θ has only one solu-
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x = 0 , and for H = 0 and T < θ there are three solutions x = 0 , |
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x > 0 |
and x < 0 , i.e., |
∂F (x,T, H ) |
= 0 |
at three different |
x . To obtain |
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∂x |
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∂2 F (x,T ) |
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the minimum, let us find the second derivative |
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∂x2 |
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sume that the magnetic field is zero). Recall that the condition on the
minimum is |
∂2 F (x,T ) |
> 0 |
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∂x2 |
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∂2 F (x,T ) |
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T 1 |
− x (1 |
− x)+(1+ x) |
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= N |
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T |
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= N |
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Let us check the results obtained. At T > θ we have only one solution
x = 0 , thus |
∂2 F (x,T ) |
= N [−θ+T ]> 0 , therefore this is minimum. At |
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