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In this course we shall investigate the classical theory of
electromagnetism in Euclidian space-time. This theory is valid over a
huge range of different conditions, but, nevertheless,
breaks down under certain
circumstances. On very large length-scales (or close to collapsed objects
such as black holes) the theory must be modified to take general relativistic
effects into account.
On the other hand, the theory breaks
down completely on very small length-scales
because of quantum effects. It is
legitimate to
treat a gas of photons as a classical electromagnetic field provided that
we only attempt to
resolve space-time into elements that contain a great many photons.
In conventional applications of electromagnetic theory
(e.g., the generation and
propagation of radio waves) this is not a particularly
onerous constraint.
Richard Fitzpatrick
2002-05-18