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density ρ 0 (r) is introduced at time t = 0. The charge density must obey the continuity
                        equation

                                                                 ∂ρ(r, t)
                                                    ∇· J(r, t) =−      ;
                                                                   ∂t
                        since J = σE,wehave
                                                                  ∂ρ(r, t)
                                                   σ∇· E(r, t) =−       .
                                                                    ∂t
                        By Gauss’s law, ∇· E can be eliminated:
                                                     σ          ∂ρ(r, t)
                                                       ρ(r, t) =−      .
                                                     	             ∂t
                        Solving this differential equation for the unknown ρ(r, t) we have

                                                     ρ(r, t) = ρ 0 (r)e −σt/	 .                (3.22)
                        The charge density within a homogeneous, isotropic conducting body decreases exponen-
                        tially with time, regardless of the original charge distribution and shape of the body. Of
                        course, the total charge must be constant, and thus charge within the body travels to
                        the surface where it distributes itself in such a way that the field internal to the body
                        approaches zero at equilibrium. The rate at which the volume charge dissipates is deter-
                        mined by the relaxation time 	/σ; for copper (a good conductor)this is an astonishingly
                        small 10 −19  s. Even distilled water, a relatively poor conductor, has 	/σ = 10 −6  s. Thus
                        we see how rapidly static equilibrium can be approached.
                        3.1.3   Steady current

                          Since time-invariant fields must arise from time-invariant sources, we have from the
                        continuity equation

                                                         ∇· J(r) = 0.                          (3.23)
                        In large-scale form this is

                                                           J · dS = 0.                         (3.24)
                                                          S
                        A current with the property (3.23)is said to be a steady current. By (3.24), a steady
                        current must be completely lineal (and infinite in extent)or must form closed loops.
                        However, if a current forms loops then the individual moving charges must undergo
                        acceleration (from the change in direction of velocity). Since a single accelerating particle
                        radiates energy in the form of an electromagnetic wave, we might expect a large steady
                        loop current to produce a great deal of radiation. In fact, if we superpose the fields
                        produced by the many particles comprising a steady current, we find that a steady current
                        produces no radiation [91]. Remarkably, to obtain this result we must consider the exact
                        relativistic fields, and thus our finding is precise within the limits of our macroscopic
                        assumptions.
                          If we try to create a steady current in free space, the flowing charges will tend to
                        disperse because of the Lorentz force from the field set up by the charges, and the
                        resulting current will not form closed loops. A beam of electrons or ions will produce
                        both an electric field (because of the nonzero net charge of the beam)and a magnetic field
                        (because of the current). At nonrelativistic particle speeds, the electric field produces
                        an outward force on the charges that is much greater than the inward (or pinch)force
                        produced by the magnetic field. Application of an additional, external force will allow


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