Page 228 - Engineering Electromagnetics, 8th Edition
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210                ENGINEERING ELECTROMAGNETICS

                                     7.6 THE SCALAR AND VECTOR
                                            MAGNETIC POTENTIALS
                                     The solution of electrostatic field problems is greatly simplified by the use of the
                                     scalar electrostatic potential V. Although this potential possesses a very real physical
                                     significance for us, it is mathematically no more than a stepping-stone which allows
                                     us to solve a problem by several smaller steps. Given a charge configuration, we may
                                     first find the potential and then from it the electric field intensity.
                                        We should question whether or not such assistance is available in magnetic fields.
                                     Can we define a potential function which may be found from the current distribution
                                     and from which the magnetic fields may be easily determined? Can a scalar magnetic
                                     potential be defined, similar to the scalar electrostatic potential? We will show in
                                     the next few pages that the answer to the first question is yes, but the second must
                                     be answered “sometimes.” Let us attack the second question first by assuming the
                                     existence of a scalar magnetic potential, which we designate V m , whose negative
                                     gradient gives the magnetic field intensity

                                                                  H =−∇V m

                                     The selection of the negative gradient provides a closer analogy to the electric potential
                                     and to problems which we have already solved.
                                        This definition must not conflict with our previous results for the magnetic field,
                                     and therefore

                                                           ∇× H = J =∇ × (−∇V m )

                                     However, the curl of the gradient of any scalar is identically zero, a vector identity
                                     the proof of which is left for a leisure moment. Therefore, we see that if H is to be
                                     defined as the gradient of a scalar magnetic potential, then current density must be
                                     zero throughout the region in which the scalar magnetic potential is so defined. We
                                     then have

                                                              H =−∇V m   (J = 0)                     (43)

                                     Because many magnetic problems involve geometries in which the current-carrying
                                     conductors occupy a relatively small fraction of the total region of interest, it is evident
                                     that a scalar magnetic potential can be useful. The scalar magnetic potential is also
                                     applicable in the case of permanent magnets. The dimensions of V m are obviously
                                     amperes.
                                        This scalar potential also satisfies Laplace’s equation. In free space,

                                                              ∇ · B = µ 0 ∇ · H = 0

                                     and hence

                                                               µ 0 ∇ · (−∇V m ) = 0
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