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Basic Equations of Electrodynamics
                             which is a wave equation for E
                             type                      with periodic solutions of the following
                                                             •
                                               E =  E g ωt –(  kr)                (4.11)
                                                     0
                             where the second derivatives of  g   are assumed to exist. Notice that
                             (4.11) requires   to be periodic but does not specify the exact form. The
                                         g
                             trigonometric sin, cosine and the exponential functions fit the specifica-
                             tions exactly.


                             4.1.1 Time-Dependent Potentials
                             Up to now the formulation for electromagnetics has been in terms of the
                             electric and magnetic field variables. We can go one step further by intro-
                             ducing potentials for the field variables. If a vector field is divergence
                             free, i.e., when ∇• B =  0   holds, then there exists a vector   such that
                                                                            A
                                                   B =  ∇× A                      (4.12)

                             A   is the vector potential. Insert this definition for   into the Faraday law
                                                                     B
                             (4.1a):

                                                   ∂A         ∂A 
                                         ∇× E =  – ∇×  ⇔  ∇×  E +  =  0           (4.13)
                                                    t ∂        t ∂ 

                             Whenever the curl of a quantity is zero (we say that it is irrotational or
                             rotation free), it can be written as the gradient of a scalar potential, say
                             Φ  , which provides us with a definition for the electric field entirely in
                             terms of the vector and scalar potentials


                                            ∂A                ∂A     
                                        E +    =  – ∇ Φ ⇔  E =  –  +  ∇ Φ         (4.14)
                                             t ∂               t ∂   
                             The two Maxwell equations that we started with are automatically satis-
                             fied by the potentials, and the remaining two now become (after a num-
                             ber of manipulation steps)





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