Chapter 3
MAXWELL'S EQUATIONS IN MAGNETIC
MEDIA
The most striking feature of a magnetic material is the fact that it can
give rise by itself to a static magnetic field in outer space. According
to Maxwell's equations, a static magnetic field is produced by stationary
electric currents, and the problem arises of the nature of the currents
responsible for this field. The question is non trivial and poses deep
conceptual difficulties, as confirmed by the fact that the existence of
permanent magnets has been known to mankind since ancient times, but the
discovery of the relationship between this kind of magnetism and electric
currents is less than two centuries old, and Ampère's intuition
of the existence of molecular currents inside matter could be given a scientific
basis only with the advent of relativistic quantum mechanics.
The basic quantum nature of the magnetism of magnetic
materials raises the point of how these quantum effects should be treated
in the classical setting of macroscopic Maxwell's equations. An acceptable
solution is to postulate the existence in magnetized matter of elementary
pointlike and permanent magnetic moments, and to describe a magnetic
material as a collection of such moments. All quantum effects are lumped
in the properties of the individual moments. By accepting their existence
as an additional fact, to be added to the existence of electric charges,
one is able to describe the behavior of magnetic materials by purely classical
means, in terms of solutions of magnetostatic Maxwell's equations.
A second relevant point is that the motion of elementary
charge and moment carriers in magnetic bodies is extremely intricate and
irregular. A detailed treatment would be hopeless. However, if we are interested
in effects taking place on a sufficiently coarse scale, we can get rid
of these complications by taking convenient space averages over elementary
volumes, small enough with respect to the characteristic scale of interest,
but still large enough to contain at any time a substantial number of particles.
[...] By working with these local averages, one looses the fine details
of the processes occurring inside each elementary volume, but one obtains
a description in terms of smooth quantities, perfectly suited to the study
of phenomena taking place over a scale much larger than that of the elementary
volumes.
In the following sections, we shall concentrate
on those aspects of Maxwell's equations that are of direct relevance to
magnetic materials. No attempt is made to give a comprehensive presentation
of the general properties of Maxwell's equations, for which many texts
can be found in the literature, nor to give detailed derivations of all
the relations that will be stated. In Section 3.1, we briefly summarize
Maxwell's equations, we discuss magnetostatic equations and we introduce
the concept of elementary magnetic moment. Section 3.2 discusses how the
magnetic state of a body can be characterized in terms of the magnetization
vector. Finally, Section 3.3 discusses energy conservation and energy dissipation
caused by eddy currents.
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3.1 Magnetostatics
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3.1.1 Maxwell's equations
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3.1.2 Stationary currents
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3.1.3 Magnetic moments
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3.2 Magnetized media
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3.2.1 Magnetic moments and magnetization
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3.2.2 Electrostatic analogy
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3.2.3 Demagnetizing fields
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3.3 Energy relations
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3.3.1 Energy of stationary current distributions
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3.3.2 Energy of individual magnetic moments
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3.3.3 Poynting theorem
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3.3.4 Eddy-current dissipation
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3.4 Bibliographical notes
Giorgio Bertotti
Materials Department, IEN Galileo Ferraris Corso Massimo d'Azeglio 42, I-10125 Torino, Italy