
resonance and capture phenomenon, represented by
an absorption cross-section, s
a
. Except for some iso-
topes (
113
Cd,
157
Gd,
164
Dy, etc.), for most elements
the corresponding cross-section remains negligible. It
should be noted that the absorption is minimal far
from the resonance energy.
The two main scattering processes of thermal neu-
trons in solid-state materials that exhibit magnetic
properties are of the dipolar type.
The first process is nuclear scattering. This results
from the interaction of the neutron spin, n
s
¼
1
2
, with
the nuclear spin, I. The corresponding nuclear po-
tential is effective at a distance of the same magnitude
as that of the nucleus dimensions. Two intermediate
scattering lengths, a
þ
and a
–
, are associated with the
final states I þ
1
2
and I
1
2
. Together they establish the
coherent part of the scattering length b
c
¼a
þ
(I þ1)/
(2I þ1) þa
(I)/(2I þ1) and the incoherent part
b
i
¼(a
þ
a
)/(2I þ1). Practically, the coherent scat-
tering process in combination with structured mul-
ticentered materials yields discrete intensities
depending on the structure factor that is determined
by the atomic arrangement. These scattering intensi-
ties can interfere constructively, whereas the incoher-
ent scattering, which has isotropically distributed
diffuse intensities, cannot interfere. However, con-
sidering the dynamic diffusion of a light element (e.g.,
hydrogen as a proton), incoherent scattering by this
particle can be analyzed using a time and position
resolving technique.
The second process is magnetic electron scattering.
This results from the interaction of the neutron spin
with the spin, s, and orbital, l (if any), vectors at-
tached to the electrons. It can be described in terms of
the total atomic spin, S, and orbital, L, components.
The diffusion length is f
M
¼2m/_
2
(M
n
4e) (M
e
4e),
where e is the unit vector and M
n
and M
e
are the
magnetic moments of the neutron and the electron,
respectively, along the scattering vector (e.g., perpen-
dicular to the diffraction plane). The magnetically
scattered amplitude strongly depends on the orienta-
tion of the easy magnetic axis in relation to the nor-
mal of the diffraction plane (in-plane vs. out-of-plane
components of the moments). If the magnetic field is
strong enough to align the moments along the scat-
tering vector, the magnetic contribution to diffraction
can vanish.
If the neutron beam polarization level is r
n
(e.g., as
diffracted on a ferromagnetic single-domain single
crystal), coherency effects can be observed between
both the nuclear and the magnetically scattered waves.
This can be expressed by the total cross-section:
s
t
¼ b
2
c
þ p
2
M
q
2
2b
c
p
M
q r
n
where p
M
is proportional to f
M
and q is the scattering
vector.
There are several important peculiarities to point
out. Because of the point-type potential of the
nuclear interaction, the nuclear cross-section of dif-
fusion results in a quasi-constant diffusion (Fermi)
length. Since it is a nuclear characteristic (isotope
characteristic), very large differences exist between
the elemental Fermi lengths, revealing marked con-
trasts, e.g., for crystal structure determination. Suc-
cessive d (and f) metals are different from each other
and, in the same manner, most of the interstitial light
elements are good scatterers. Table 2 compares se-
lected cross-section amplitudes (Sears 1984).
Contrary to the nuclear scattering, the magnetic
scattering related to the magnetic electron density, i.e.,
the magnetic scattering cross-section, decreases with
the momentum transfer, Q, well approximated by
Gaussian profiles (Brown 1992), which may reveal
localized to itinerant aspects of the electron density.
For a completely disordered moment distribution
(paramagnetic state with no short-range correlations),
independent of the initial polarization state of the
beam, a diffuse magnetic (incoherent) scattered inten-
sity is found that adds to the nuclear contribution.
For a polarized neutron beam, successive measure-
ments of the scattered intensity for two states of po-
larization (up and down, the scattering vector being
horizontal) allow one to determine very accurately the
spatial spin density, if the nuclear crystal structure is
known. It should be noted that, if the magnetic struc-
ture exhibits unpolarized components, a depolariza-
tion effect is induced that can be successfully adopted
in the polarization analysis technique to detect weak
deviations from ferromagnetism.
The scattering processes as described above are of
the elastic type (no energy exchange). Since the ki-
netic energy of thermal neutrons is of the same order
of magnitude as that of the excitation processes of
matter (phonons, atom diffusion, magnons, crystal
field levels, etc.), inelastic scattering experiments can
provide valuable information on the correlation en-
ergies or the dynamics of atom movements. Inelastic
scattering leads to a change (initial to final states) of
the neutron energy, where the opposite energy cor-
responds to the phonon or magnon frequency change
ho. Q ¼k
f
k
i
¼2jR þq allows one to localize scat-
tered neutrons with a typical intensity given by a
double differential (space and energy resolved) scat-
tering cross-section. Q is the scattering vector, R a
reciprocal lattice vector, q the wave vector of the
excitation, and k
i
and k
f
are the initial and final wave
vectors. For such purposes, an analyzer is placed
behind the sample to check the spatial and energy
dispersion profile.
2. Applications of Neutron Scattering to Hard
Magnetic Materials
Except for anomalously absorbing nuclei, the pene-
tration depth of neutrons is particularly large (a few
centimeters), several orders of magnitude larger than
1018
Permanent Magnet Materials: Neutron Experiments