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Magnetism III: Magnetic Ordering 
Physics 355
So far... 
Magnetic moments originate, on an atomic scale, 
from the orbit and spin of electrons. These effects are 
also influenced by the particular electronic 
configuration of the different elements. 
Electrons in matter have two contributing properties - 
spin and orbit. 
In materials, the largest magnetic effects are due to 
the spins of electrons rather than their orbital 
moments. 
The orbital moments play a part as well, but when 
there are uncompensated spins present in a 
molecule, the orbital contribution is negligible.
Transition Metals
Spontaneous Magnetization 
ferromagnetic 
A paramagnetic 
material has an 
unordered magnetic 
structure, which 
fluctuates in time. 
Averaging over time 
yields no permanent 
magnetization. ferrimagnetic 
antiferromagnetic
Spontaneous Magnetization 
elements low T room T high T 
transition 
FM: Fe, Ni, 
FM: Fe, Ni, 
metals 
Co 
Co 
paramagnetic 
rare earths FM: Gd, Tb 
(below RT) 
and all 
others at 
very low Ts 
AFM, 
except Gd 
paramagnetic
Ferromagnetism 
 Ferromagnetism may be thought of as a special case of 
paramagnetism in which the individual spin magnetic moments 
interact (i.e. the moments are coupled). 
 The uncompensated spins in individual atoms of a 
ferromagnetic material may couple either directly (direct 
exchange) or through an intermediate anion - usually oxygen 
(super exchange). 
 In crystals of a ferromagnetic material, this gives rise to a net 
magnetic moment due to the coupling of spins in a preferred 
orientation (keep in mind that this coupling is quantum 
mechanical in nature and not purely due to the magnetic forces 
acting between neighboring atoms). 
 As with paramagnets, ferromagnets have strong, positive 
magnetic susceptibility. 
 Unlike paramagnets, when the applied field is removed, they 
retain a component of magnetization in the direction of the 
applied field - they are "permanently" magnetized (they do have 
hysteresis). 
 Also, their susceptibility is not dependent upon temperature in a 
way that follows the Curie Law.
Ferromagnetism 
Temperature Dependence of Ferromagnetism: 
Since ferromagnetism results from the interaction of 
atomic moments in materials, there is an exchange 
energy associated with coupling the spin moments. 
At room temperature, this exchange energy is much 
greater than the energy due to randomizing thermal 
effects (kBT). 
If thermal energy exceeds the spin coupling 
(exchange) energy, the coupling breaks down and 
the material behaves as a paramagnet. 
This temperature is dependent on the material and is 
called the Curie temperature (or, in the case of 
antiferromagnetic materials, the Neél temperature).
Ferromagnetism 
c 
TCurie 
T
Exchange and the Curie Temperature 
Start with a paramagnet consisting of N ions of spin 
S. 
Suppose there is some local interaction going on that 
behaves like a local magnetic field BE– the Exchange 
Field (or the Weiss Field). 
Mean-field approximation: 
BE = lM
Exchange and the Curie Temperature 
Continuing with a solid in the paramagnetic phase: If 
a magnetic field Bis applied, a finite magnetization 
A will occur, which, in turn, creates a finite exchange 
field. 
= c 
The magnetization will then be: 
( A E ) 
0 
M B + B 
m 
For the paramagnet, we have the Curie law: c=C/T, 
so 
C 
C 
M 
A T C 
T TCurie 
B 
- 
= 
- l 
c = =
Exchange and the Curie 
Temperature 
The Curie Temperature 
for iron is about 700 °C. 
This temperature is 
reached at about 20 km 
below the surface of the 
Earth, whereas at the outer boundary of the 
Core (about 2900 km depth) the temperature 
is about 2000 °C. This is well above the Curie 
temperature, so although the core is largely 
iron, that iron is no longer ferromagnetic, and 
the Earth's core cannot be a permanent 
magnet.
Exchange and the Curie Temperature 
The curie constant can be now written in terms we’ve 
used before: 
2 
B 
k T 
T 
Curie B Curie 
2 
ng S(S ) 
+1 m 
l = = 
C 
For Fe, TCurie is about 1000 K, g is about 2, S is 1, so 
l is about 5000. The saturation magnetization for 
iron is about 1700 units, so BE = (1700)(5000)=10 
million Gauss = 1000 T, a field stronger than that due 
to the other ions in the crystal (about 0.1 T for a near 
neighbor). So, BE is not really a magnetic field, but it 
acts like one.
Exchange and the Curie Temperature 
The exchange field is an approximation for the more 
correct exchange interaction determined via quantum 
mechanics. 
If ions i and j have spins Si and Sj, the energy of 
interaction contains a term: 
U = -2J Si ×Sj 
where J is called the exchange integral and is related 
to the overlap of the charge distributions for the two 
ions. This is fully developed in QM in what is called 
the Heisenberg Model.
Exchange and the Curie Temperature 
The exchange interaction depends on the spin 
orientation. 
Pauli prevents electrons of the same spin from getting 
too close to each other. 
Pauli allows two electrons of opposite spin to be in 
the same place. 
The result of this is that the electrostatic energy of the system depends on 
the relative orientation of the spins: the difference in energy defines the 
Exchange Energy.
Heisenberg Exchange Parameter 
ö 
æ 
2 E i j 1 S S × ÷ ÷ 
- = åi 
ç ç 
 The exchange energy of atom j is 
where the sum is over all atoms except atom j. 
 The dipole moment of atom j is 
ø 
U J 
è 
 
ö 
× ÷ ÷ 
ø 
S μ 
g 
= - m 
B 
μ S 
æ 
ç ç 
è 
g 
1 
 
m 
j 
U 
 
Þ = 
åi 
i 
J 
E 
B 
so the exchange interaction has been replaced by the 
interaction between a spin dipole moment and the 
Weiss field:
Heisenberg Exchange Parameter 
 The local field at atom j is 
B B S B E 
S 
ö 
J zJ 
= - å g 
- = ÷ ÷ 
ø 
i 
E applied 
m 
æ 
ç ç 
g i 
 B 
1 
B 
local applied 
è 
m 
where Bappied is the applied field and the sum is over 
all of the atoms, except j. 
 The form on the right is valid of all of the atoms have 
the same spin. 
 JE only includes z nearest neighbors.
Heisenberg Exchange Parameter 
 Since M = Nm, the effective exchange field can be 
expressed as (zJ/ng2 m2)M. 
EB 
 The Curie constant is then given by 
2 
B 
2 
0 
E 
zJ 
m m 
l = 
ng
Exchange: Example 
Use the experimental value of the Curie temperature to estimate the 
Heisenberg exchange integral for iron. The concentration of iron atoms 
is 8.5 × 1028 atoms/m3 and each iron atom has 12 nearest neighbors. 
Iron 
• The experimental value for the Curie temperature is 1043 K. 
• g = 2 and S¢ = 1 
B Curie 
n g S(S ) 
m + m 
1 
23 
2 
B 
( . ) ( ) 
= ´ 
- 
3 1 38 10 J/K 1043 K 
3 
2 
0 
( )( )( ) ( ) 
588 
7 28 3 2 24 2 
4 10 8 5 10 /m 2 1 9 27 10 J/T 
= 
p´ ´ ´ 
l = 
- - 
. ( ) . 
k T
Exchange: Example 
Iron 
• The experimental value for the Curie temperature is 1043 K. 
• g = 2 and S¢ = 1 
" l = 588 
2 
B 
2 
J n g 
= m 0 
m l 
z 
( )( )( )( ) 
28 3 7 2 24 2 
. . ( ) 
= ´ p´ ´ 
8 5 10 /m 4 10 2 9 27 10 J/T 588 
12 
21 3 
1.8 10 J 1.1 10 eV 
E 
- - 
- - 
= ´ = ´
Exchange in Rare Earths 
 Band overlap is small in f electron atoms – weak exchange 
field. 
 At low temperatures, exchange occurs between the f 
electrons and nearly free electrons that gives rise to FM in 
these materials. 
 Indirect exchange occurs in these atoms: 
 If f electrons around one atom are spin down, then an 
exchange interaction will lower the energies of nearby 
spin up free electrons. 
 These free electrons then move to other atoms, where 
exchange tends to lower the energy of spin down f 
electrons.
RKKY Interaction 
Indirect exchange couples moments 
over relatively large distances. It is 
the dominant exchange interaction in 
metals where there is little or no 
direct overlap between neighboring 
magnetic electrons. It therefore acts 
through an intermediary which in 
metals are the conduction electrons 
(itinerant electrons). This type of 
exchange was first proposed by 
Ruderman and Kittel and later 
extended by Kasuya and Yosida to 
give the theory now generally know 
as the RKKY interaction.
Hysteresis B = m0 (H + M)
Ferrimagnets and Antiferromagnetism 
 Ions in most ferrimagnets and antiferromagnets are 
positioned on two sublattices, such that the spins on each 
sublattice tend to be aligned with each other, but spins on 
different sublattices tend be to oriented in opposite 
directions. 
Unit cell and magnetic 
structure of the 
ferrimagnetic 
intermetallic compound 
GdCo5. The magnetic 
moments of Gd (blue) 
are directed 
antiparallel to the 
moments of Co 
(green).
Ferrimagnets and Antiferromagnetism 
Crystal Structure of Magnetite 
Magnetite, Fe3O4 crystallizes in 
the spinel structure. Large oxygen 
ions are close packed in a cubic 
arrangement and the smaller iron 
ions fill in the gaps. 
The lattice sites come in two flavors: 
• tetrahedral site: Fe ion is surrounded by 4 oxygen ions 
• octahedral site: Fe ion is surrounded by 6 oxygen ions 
The tetrahedral and octahedral sites form the two magnetic sublattices, A and 
B, respectively. The spins on the A sublattice are antiparallel to those on the B 
sublattice. The two crystal sites are very different and result in complex forms of 
exchange interactions of the iron ions between and within the two types of sites.
Magnetization & Susceptibility 
Paramagnetic State of Two Sublattices 
( ) 
M = M + M = C + C T - l 
C C 
A B A B 
m - 
C C T C C 
c = m = + - l 
A B A B 
0 
Antiferromagnets 
( ) 
( ) 
( 2 
2 ) 
Curie 
Applied 
2 Applied 
Curie 
2 
0 
A B 
2 
2 
T T 
B 
M 
B 
T T 
- 
M C 
( T T 
) 
m + 
0 Neel 
c = m 0 
= 
B 
Applied 
C 
T T 
B 
M 
+ 
Applied Neel 
=
Antiferromagnets 
Some Examples: Cr, Mn, Cr2O3, CoO, Fe2O3
22 magnetism3

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22 magnetism3

  • 1. Magnetism III: Magnetic Ordering Physics 355
  • 2. So far... Magnetic moments originate, on an atomic scale, from the orbit and spin of electrons. These effects are also influenced by the particular electronic configuration of the different elements. Electrons in matter have two contributing properties - spin and orbit. In materials, the largest magnetic effects are due to the spins of electrons rather than their orbital moments. The orbital moments play a part as well, but when there are uncompensated spins present in a molecule, the orbital contribution is negligible.
  • 4. Spontaneous Magnetization ferromagnetic A paramagnetic material has an unordered magnetic structure, which fluctuates in time. Averaging over time yields no permanent magnetization. ferrimagnetic antiferromagnetic
  • 5. Spontaneous Magnetization elements low T room T high T transition FM: Fe, Ni, FM: Fe, Ni, metals Co Co paramagnetic rare earths FM: Gd, Tb (below RT) and all others at very low Ts AFM, except Gd paramagnetic
  • 6. Ferromagnetism  Ferromagnetism may be thought of as a special case of paramagnetism in which the individual spin magnetic moments interact (i.e. the moments are coupled).  The uncompensated spins in individual atoms of a ferromagnetic material may couple either directly (direct exchange) or through an intermediate anion - usually oxygen (super exchange).  In crystals of a ferromagnetic material, this gives rise to a net magnetic moment due to the coupling of spins in a preferred orientation (keep in mind that this coupling is quantum mechanical in nature and not purely due to the magnetic forces acting between neighboring atoms).  As with paramagnets, ferromagnets have strong, positive magnetic susceptibility.  Unlike paramagnets, when the applied field is removed, they retain a component of magnetization in the direction of the applied field - they are "permanently" magnetized (they do have hysteresis).  Also, their susceptibility is not dependent upon temperature in a way that follows the Curie Law.
  • 7. Ferromagnetism Temperature Dependence of Ferromagnetism: Since ferromagnetism results from the interaction of atomic moments in materials, there is an exchange energy associated with coupling the spin moments. At room temperature, this exchange energy is much greater than the energy due to randomizing thermal effects (kBT). If thermal energy exceeds the spin coupling (exchange) energy, the coupling breaks down and the material behaves as a paramagnet. This temperature is dependent on the material and is called the Curie temperature (or, in the case of antiferromagnetic materials, the Neél temperature).
  • 9. Exchange and the Curie Temperature Start with a paramagnet consisting of N ions of spin S. Suppose there is some local interaction going on that behaves like a local magnetic field BE– the Exchange Field (or the Weiss Field). Mean-field approximation: BE = lM
  • 10. Exchange and the Curie Temperature Continuing with a solid in the paramagnetic phase: If a magnetic field Bis applied, a finite magnetization A will occur, which, in turn, creates a finite exchange field. = c The magnetization will then be: ( A E ) 0 M B + B m For the paramagnet, we have the Curie law: c=C/T, so C C M A T C T TCurie B - = - l c = =
  • 11. Exchange and the Curie Temperature The Curie Temperature for iron is about 700 °C. This temperature is reached at about 20 km below the surface of the Earth, whereas at the outer boundary of the Core (about 2900 km depth) the temperature is about 2000 °C. This is well above the Curie temperature, so although the core is largely iron, that iron is no longer ferromagnetic, and the Earth's core cannot be a permanent magnet.
  • 12. Exchange and the Curie Temperature The curie constant can be now written in terms we’ve used before: 2 B k T T Curie B Curie 2 ng S(S ) +1 m l = = C For Fe, TCurie is about 1000 K, g is about 2, S is 1, so l is about 5000. The saturation magnetization for iron is about 1700 units, so BE = (1700)(5000)=10 million Gauss = 1000 T, a field stronger than that due to the other ions in the crystal (about 0.1 T for a near neighbor). So, BE is not really a magnetic field, but it acts like one.
  • 13. Exchange and the Curie Temperature The exchange field is an approximation for the more correct exchange interaction determined via quantum mechanics. If ions i and j have spins Si and Sj, the energy of interaction contains a term: U = -2J Si ×Sj where J is called the exchange integral and is related to the overlap of the charge distributions for the two ions. This is fully developed in QM in what is called the Heisenberg Model.
  • 14. Exchange and the Curie Temperature The exchange interaction depends on the spin orientation. Pauli prevents electrons of the same spin from getting too close to each other. Pauli allows two electrons of opposite spin to be in the same place. The result of this is that the electrostatic energy of the system depends on the relative orientation of the spins: the difference in energy defines the Exchange Energy.
  • 15. Heisenberg Exchange Parameter ö æ 2 E i j 1 S S × ÷ ÷ - = åi ç ç  The exchange energy of atom j is where the sum is over all atoms except atom j.  The dipole moment of atom j is ø U J è  ö × ÷ ÷ ø S μ g = - m B μ S æ ç ç è g 1  m j U  Þ = åi i J E B so the exchange interaction has been replaced by the interaction between a spin dipole moment and the Weiss field:
  • 16. Heisenberg Exchange Parameter  The local field at atom j is B B S B E S ö J zJ = - å g - = ÷ ÷ ø i E applied m æ ç ç g i  B 1 B local applied è m where Bappied is the applied field and the sum is over all of the atoms, except j.  The form on the right is valid of all of the atoms have the same spin.  JE only includes z nearest neighbors.
  • 17. Heisenberg Exchange Parameter  Since M = Nm, the effective exchange field can be expressed as (zJ/ng2 m2)M. EB  The Curie constant is then given by 2 B 2 0 E zJ m m l = ng
  • 18. Exchange: Example Use the experimental value of the Curie temperature to estimate the Heisenberg exchange integral for iron. The concentration of iron atoms is 8.5 × 1028 atoms/m3 and each iron atom has 12 nearest neighbors. Iron • The experimental value for the Curie temperature is 1043 K. • g = 2 and S¢ = 1 B Curie n g S(S ) m + m 1 23 2 B ( . ) ( ) = ´ - 3 1 38 10 J/K 1043 K 3 2 0 ( )( )( ) ( ) 588 7 28 3 2 24 2 4 10 8 5 10 /m 2 1 9 27 10 J/T = p´ ´ ´ l = - - . ( ) . k T
  • 19. Exchange: Example Iron • The experimental value for the Curie temperature is 1043 K. • g = 2 and S¢ = 1 " l = 588 2 B 2 J n g = m 0 m l z ( )( )( )( ) 28 3 7 2 24 2 . . ( ) = ´ p´ ´ 8 5 10 /m 4 10 2 9 27 10 J/T 588 12 21 3 1.8 10 J 1.1 10 eV E - - - - = ´ = ´
  • 20. Exchange in Rare Earths  Band overlap is small in f electron atoms – weak exchange field.  At low temperatures, exchange occurs between the f electrons and nearly free electrons that gives rise to FM in these materials.  Indirect exchange occurs in these atoms:  If f electrons around one atom are spin down, then an exchange interaction will lower the energies of nearby spin up free electrons.  These free electrons then move to other atoms, where exchange tends to lower the energy of spin down f electrons.
  • 21. RKKY Interaction Indirect exchange couples moments over relatively large distances. It is the dominant exchange interaction in metals where there is little or no direct overlap between neighboring magnetic electrons. It therefore acts through an intermediary which in metals are the conduction electrons (itinerant electrons). This type of exchange was first proposed by Ruderman and Kittel and later extended by Kasuya and Yosida to give the theory now generally know as the RKKY interaction.
  • 22. Hysteresis B = m0 (H + M)
  • 23. Ferrimagnets and Antiferromagnetism  Ions in most ferrimagnets and antiferromagnets are positioned on two sublattices, such that the spins on each sublattice tend to be aligned with each other, but spins on different sublattices tend be to oriented in opposite directions. Unit cell and magnetic structure of the ferrimagnetic intermetallic compound GdCo5. The magnetic moments of Gd (blue) are directed antiparallel to the moments of Co (green).
  • 24. Ferrimagnets and Antiferromagnetism Crystal Structure of Magnetite Magnetite, Fe3O4 crystallizes in the spinel structure. Large oxygen ions are close packed in a cubic arrangement and the smaller iron ions fill in the gaps. The lattice sites come in two flavors: • tetrahedral site: Fe ion is surrounded by 4 oxygen ions • octahedral site: Fe ion is surrounded by 6 oxygen ions The tetrahedral and octahedral sites form the two magnetic sublattices, A and B, respectively. The spins on the A sublattice are antiparallel to those on the B sublattice. The two crystal sites are very different and result in complex forms of exchange interactions of the iron ions between and within the two types of sites.
  • 25. Magnetization & Susceptibility Paramagnetic State of Two Sublattices ( ) M = M + M = C + C T - l C C A B A B m - C C T C C c = m = + - l A B A B 0 Antiferromagnets ( ) ( ) ( 2 2 ) Curie Applied 2 Applied Curie 2 0 A B 2 2 T T B M B T T - M C ( T T ) m + 0 Neel c = m 0 = B Applied C T T B M + Applied Neel =
  • 26. Antiferromagnets Some Examples: Cr, Mn, Cr2O3, CoO, Fe2O3

Editor's Notes

  1. The exchange field can be as high as 1000 T. The magnetization is defined as the magnetic dipole moment per unit volume. If domains are present in the material, the magnetization refers to the value within that region. Domains are regions within the solid in which the dipole moments are aligned in a particular direction. Lambda is a temperature-independent constant. According to the equation, each ion experiences the average magnetization due to the average of the other dipole moments from the other ions. In reality, this may be limited to nearest neighbors.
  2. The susceptibility has a singularity at T = C. At this temperature (and below), there is a spontaneous magnetization, which allows a finite M for a zero B.
  3. The interaction is characterized by a coupling coefficient, j... where kF is the radius of the conduction electron Fermi surface, Rl is the lattice position of the point moment, EF is the Fermi energy and F(x) is... The RKKY exchange coefficient oscillates from positive to negative as the separation of the ions changes and has the damped oscillatory nature shown in the figure. Therefore, depending upon the separation between a pair of ions their magnetic coupling can be ferromagnetic or antiferromagnetic. A magnetic ion induces a spin polarization in the conduction electrons in its neighborhood. This spin polarization in the itinerant electrons is felt by the moments of other magnetic ions within range, leading to an indirect coupling.
  4. When a ferromagnetic material is magnetized in one direction, it will not relax back to zero magnetization when the imposed magnetizing field is removed. It must be driven back to zero by a field in the opposite direction. If an alternating magnetic field is applied to the material, its magnetization will trace out a loop called a hysteresis loop. The lack of retraceability of the magnetization curve is the property called hysteresis and it is related to the magnetic domains in the material. Once the magnetic domains are reoriented, it takes some energy to turn them back again. This property of ferrromagnetic materials is useful as a magnetic "memory". Some compositions of ferromagnetic materials will retain an imposed magnetization indefinitely and are useful as "permanent magnets". The magnetic memory aspects of iron and chromium oxides make them useful in audio tape recording and for the magnetic storage of data on computer disks.