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The Electromagnetic System
                             in following the usage established by Albert Einstein (1879–1955), in his
                             seminal work on the photoelectric effect, that we now call the governing
                             electrodynamic equations the Maxwell equations. Einstein went on to
                             unify space-time electromagnetic theory in his work on relativity, result-
                             ing in a single expression for the Maxwell equations.

                             At interaction dimensions of the order of atomic spacings and smaller,
                             we have to also include the rules of quantum mechanics. We consider
                             both viewpoints.

                Chapter Goal Our goal for this chapter is first to obtain a complete description of classi-
                             cal electrodynamics, and then to extend this model of radiation to a quan-
                             tum viewpoint.

                Chapter      Our road map is as follows: to state the Maxwell equations, quantify the
                Roadmap      concepts leading to electro-quasi-statics and magneto-quasi-statics, and
                             to their completely static counterparts. Next, we take a closer look at
                             light, which is that part of the electromagnetic spectrum that ranges from
                             the near infrared all the way through to the near ultraviolet, by treating
                             both its wave-like and particle-like characteristics. There will be practi-
                             cally no “optics” here, and the interaction between light and matter will
                             appear only later in the book.




                             4.1 Basic Equations of Electrodynamics

                             The Maxwell equations are remarkably structured. If it were not for the
                             absence of magnetic “charges” in nature, we would be able to exchange
                             the roles of the electric field E   and the magnetic field H  , as well as the
                             electric displacement D   and the magnetic induction  . We first write the
                                                                       B
                             Maxwell equations in differential form; each equation must be satisfied
                             in every point of space:






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