Liquid ferromagnets do not exist: all known ferromagnetic and ferrimagnetic
materials undergo a change to a paramagnetic state at a temperature called
the Curie temperature, which is below the melting temperature of the material.
For example, for iron the Curie temperature is 770°C and the melting point
is 1535°C. Nevertheless, fluids do exist which behave very much like a
molten ferromagnet [1-4]. These magnetic fluids, also called ferrofluids, are
actually stable colloidal suspensions of small magnetic particles with a typical
diameter of about 10 nm. Materials such as magnetite (Fe3O4) or metallic iron
generally contain magnetic multidomains, but when the particles are sufficiently
small they can accommodate only one single domain. Such a single domain particle
has a net magnetic moment (proportional to its volume) and a colloidal
dispersion of the particles may be visualized as a collection of small permanent
magnets which exhibit translational and rotational Brownian motion in the
carrier solvent.
Usually Brownian motion in colloidal sols has to compete with an external
force in the form of gravity, leading to the familiar sedimentation-diffusion (Boltzmann) distribution of colloids in a gravitational or
centrifugal field. Equally familiar is the equilibrium shape of a
conventional colloidal bulk fluid in the gravity field, namely a flat
meniscus, parallel to the surface of the earth. A ferrofluid offers some
refreshing changes: it responds to an external magnetic field gradient
which deforms the meniscus of the fluid and may create exotic equilibrium
shapes due to the balance between magnetic and gravitational forces [1].
Though this behaviour certainly mimics a liquid ferromagnet, we should
realize that ultimately the colloidal stability of the suspended particles
is responsible for this mimicry. If the particles aggregate into large
clusters (by the addition of flocculating electrolyte or a poor solvent
for the particle coatings) a magnet will drag out the dispersed material,
leaving behind a clear supernatant. This is equivalent to the collapse of
a sedimentation-diffusion equilibrium when (non-magnetic) colloids
aggregate and settle to the bottom of the vessel. Clearly for applications
of a ferrofluid as a liquid magnet (for example in an airtight seal
between rotating parts [1]) colloidal stability is essential. Ferrofluids
with long term stability have already been available for many years,
giving a firm practical basis for the many studies on the continuum
hydrodynamics of magnetic fluids [1]. However, the understanding of what
happens on the level of the discrete colloidal particles is still very
limited. What sort of spatial structures are present in a stable fluid in
zero field; does chain formation really occur? What sort of phase
transitions may take place; does a liquid-gas coexistence exist for pure
dipolar interactions or does that require the (for real colloids ever
present) Van der Waals attractions? What does the pair potential in a
typical ferrofluid look like; below what particle size is magnetic
interaction insignificant [5]? These are just some of the widely debated
topics [6-11] and the reader will certainly identify more discussion
topics in the contributions to this special issue, or the references
therein. The reader will also notice that the joint focus of these
contributions is actually much broader than the interaction of particles
with each other or an external field. The field of magnetic colloids is
becoming quite a colourful mix of disciplines, and meetings where, for
example, chemical synthesis experts and theoretical physicists share a
bench, are not uncommon.
The purpose of this special issue is certainly not to provide an overview of the
field of dipolar colloids and ferrofluids which is large and diverse (see
for example [1, 8, 11]). The aim is merely to illustrate this diversity
with contributions on the preparation, experimental study, simulation and
theory of dipolar particles. For didactic support the reader may wish to
consult figure 1 which represents a dipolar hard sphere fluid, all be it
one at zero temperature. I thank Peter de Graaf for the skilful manufacture
of the marbles in figure 1 and Jan den Boesterd for the photography.

Figure 1: Glass marbles (radius 1 cm) with an embedded magnet. The magnet poles are slightly below the glass surface such that the magnetic interaction is fairly weak, modelling hard spheres with dipolar perturbation. The anisotropic attraction is nevertheless sufficiently strong to cause chain formation at low density (A) whereas the net attraction is too weak to orient dipoles in a random sphere packing (B). The dipole distribution can be observed more clearly when the glass marbles are optically matched by toluene (C).
A PhilipseGuest Editor
References
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