Title: Magnetism and Magnetic Materials
1Magnetism and Magnetic Materials DTU (10313)
10 ECTS KU 7.5 ECTS
Module 4 11/02/2001 Interactions
2Intended Learning Outcomes (ILO)
(for todays module)
- List the various forms of exchange interactions
between spins - Estimate the influence of dipolar interactions
between spins - Explain how exchange interactions can favor
either FM or AFM alignment - Describe the continuum-limit of exchange
3Flashback
- Arrange the electronic wave function so as to
maximize S. In this way, the Coulomb energy is
minimized because of the Pauli exclusion
principle, which prevents electrons with parallel
spins being in the same place, and this reduces
Coulomb repulsion. - The next step is to maximize L. This also
minimizes the energy and can be understood by
imagining that electrons in orbits rotating in
the same direction can avoid each other more
effectively. - Finally, the value of J is found using JL-S if
the shell is less than half-filled, JLS is the
shell is more than half-filled, JS (L0) if the
shell is exactly half-filled (obviously). This
third rule arises from an attempt to minimize the
spin-orbit energy.
Spin-orbit -S and L not independent -Hunds
third rule
Hunds rules -How to determine the ground state
of an ion
The fine structure of energy levels -Apply
Hunds rules to given ions
Co2 ion 3d7 S3/2, L3, J9/2, gJ5/3, 4F9/2
4Data and comparison (4f and 3d)
Hunds rules seem to work well for 4f ions. Not
so for many 3d ions. Why?
How do we measure the effective moment?
5Origin of crystal fields
When an ion is part of a crystal, the
surroundings (the crystal field) play a role in
establishing the actual electronic structure
(energy levels, degeneracy lifting, orbital
shapes etc.).
Not good any longer!
6A new set of orbitals
Octahedral
Tetrahedral
7Crystal field splitting low/high spin states
The crystal field results in a new set of
orbitals where to distribute electrons.
Occupancy, as usual, from the lowest to the
highest energy. But, crystal field acts in
competition with the remaining contributions to
the Hamiltonian. This drives occupancy and may
result in low-spin or high-spin states.
8Orbital quenching
Examine again the 3d ions. We notice a peculiar
trend the measured effective moment seems to be
S-only. L is quenched. This is a consequence of
the crystal field and its symmetry.
Is real. No differential (momentum-related)
operators. Hence, we need real eigenfunctions.
Therefore, we need to combine ml states to yield
real functions. This means, combining plus or
minus ml, which gives zero net angular momentum.
Examples
9Jahn-Teller effect
In some cases, it may be energetically favorable
to shuffle things around than to squeeze
electrons within degenerate levels.
10Dipolar interaction
Dipolar interaction is the key to explain most of
the macroscopic features of magnetism, but on the
atomic scale, it is almost always negligible
(except at mK temperatures).
Dipolar interaction energy
m1
m2
- Estimate the magnitude of the dipolar energy
between two aligned moments (1 mB) separated by
0.1 nm. - Now think of the moments as tiny magnetized
spheres each carrying N Bohr magnetons and
separated by 10 nm. How large is N if we want an
energy of the order of 1000 K?
r
11Exchange symmetry
This is, instead, the real thing underpinning
long range magnetic ordering. Effectively, its
strength is enormous.
Singlet, antisymmetric
Triplet, symmetric
Singlet, total wave function (antisymmetric)
Triplet, total wave function (antisymmetric)
Singlet, energy
Triplet, energy
12Exchange Hamiltonian
Key observation even if H does not include spin
terms, the energy levels depend on the alignment
of spins via symmetry of the wave function.
Remember this (and correct a mistake in M1)
If we construct this operator
with
It happens to produce the same energy splitting
of the real Hamiltonian. We take this, remove the
constant, and use it as spin Hamiltonian
the exchange constant (or exchange integral)
13Generalization and general features
A positive exchange constant favors parallel
spins, while a negative value favors antiparallel
alignment
The Heisemberg Hamiltonian
Exchange coupling between electrons belonging to
the same atom can be interpreted as underpinning
Hunds first rule (with Jgt0)
Suppose J is about 1000 K. How strong is the
effective exchange field?
Coupling between electrons in different atoms,
where bonding and/or antibonding orbitals may
exist. In this case, Jgt0 is more likely.
14Indirect exchange superexchange
Oxygen mediated, typical of MnO and similar
compounds, mainly antiferromagnetic
- When two cations have loves of singly occupied
3d-orbitals which point towards each other giving
a large overlap and hopping integrals, the
exchange is strong and antiferromagnetic (Jlt0).
This is the usual case for 120-180 degrees M-O-M
bonds. - When two cations have an overlap integral between
singly occupied 3d-orbitals which is zero by
symmetry, the exchange is ferromagnetic and
relatively weak. This is the case for about 90
degree M-O-M bonds - When to cations have an overlap between singly
occupied 3d-orbitals and empty or doubly occupied
orbitals of the same type, the exchange is also
ferromagnetic, and relatively weak.
t is the hopping integral and U is the Coulomb
energy
15Indirect exchange double exchange
Typical of mixed-valence compounds, like
Mn3/Mn4 (manganites) or Fe2/Fe3 (magnetite).
Double exchange is essentially ferromagnetic
superexchange in an extended system.
16The continuum approximation
Is the exchange stiffness, with c a
crystal-structure-dependent factor, and a the
nearest-neighbour distance
17Sneak peek
Ferromagnetism (Weiss)
18Wrapping up
- Crystal fields (from last module)
- Exchange (and dipolar) interaction
- Spin Hamiltonian
- Superexchange
- Double exchange
- The continuum limit
Next lecture Tuesday February 15, 1315, KU
Auditorium 9 Magnetic order (MB)