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Chapter 2



                        Maxwell’s theory of electromagnetism
















                        2.1   The postulate
                          In 1864, James Clerk Maxwell proposed one of the most successful theories in the
                        history of science. In a famous memoir to the Royal Society [125] he presented nine
                        equations summarizing all known laws on electricity and magnetism. This was more
                        than a mere cataloging of the laws of nature. By postulating the need for an additional
                        term to make the set of equations self-consistent, Maxwell was able to put forth what
                        is still considered a complete theory of macroscopic electromagnetism. The beauty of
                        Maxwell’s equations led Boltzmann to ask, “Was it a god who wrote these lines ... ?”
                        [185].
                          Since that time authors have struggled to find the best way to present Maxwell’s
                        theory. Although it is possible to study electromagnetics from an “empirical–inductive”
                        viewpoint (roughly following the historical order of development beginning with static
                        fields), it is only by postulating the complete theory that we can do justice to Maxwell’s
                        vision. His concept of the existence of an electromagnetic “field” (as introduced by
                        Faraday) is fundamental to this theory, and has become one of the most significant
                        principles of modern science.
                          We find controversy even over the best way to present Maxwell’s equations. Maxwell
                        worked at a time before vector notation was completely in place, and thus chose to
                        use scalar variables and equations to represent the fields. Certainly the true beauty
                        of Maxwell’s equations emerges when they are written in vector form, and the use of
                        tensors reduces the equations to their underlying physical simplicity. We shall use vector
                        notation in this book because of its wide acceptance by engineers, but we still must
                        decide whether it is more appropriate to present the vector equations in integral or point
                        form.
                          On one side of this debate, the brilliant mathematician David Hilbert felt that the
                        fundamental natural laws should be posited as axioms, each best described in terms
                        of integral equations [154]. This idea has been championed by Truesdell and Toupin
                        [199]. On the other side, we may quote from the great physicist Arnold Sommerfeld:
                        “The general development of Maxwell’s theory must proceed from its differential form;
                        for special problems the integral form may, however, be more advantageous” ([185], p.
                        23). Special relativity flows naturally from the point forms, with fields easily converted
                        between moving reference frames. For stationary media, it seems to us that the only
                        difference between the two approaches arises in how we handle discontinuities in sources
                        and materials. If we choose to use the point forms of Maxwell’s equations, then we must
                        also postulate the boundary conditions at surfaces of discontinuity. This is pointed out




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