5. Preparing for Maxwell’s Equations 5.1 The incomplete set.
Before Maxwell could unify the fundamental equations governing electromagnetism he had to add a crucial piece to one of them. We have already collected three complete Maxwell equations (available either in differential or integral forms): Gauss’ law (1.21)
∇.D = ρ f ;
Faraday’s law of induction (1.32)
∇×E = −
∂B ∂t
“No magnetic monopoles” (1.28) ∇.B = 0 . But Ampere’s law is incomplete in the forms we have seen so far, e.g. (2.12) ∇×H = J f . This only describes a system with steady currents but is inadequate to cope even with such a simple time-dependent problem as the charging of a capacitor see section 5.3 below. 5.2 What is missing from Ampere’s Law (formally) Take the divergence of both sides of (2.12)
∇.∇ × H = ∇.J f
(5.1)
.But for any vector (see Tools) ∇.∇ × A = 0 , so if (2.12) is true the divergence of the free
current density J f is everywhere zero. That would forbid a small local concentration of negative charge (say) from streaming outward into the space around it. Such an outflow must happen because of the Coulomb repulsion between like charges, and it has to satisfy the conservation of charge equation ∂ρ ∇.J f = − f , (5.2) ∂t sometimes called the continuity equation. Free charge densities must be able to change with time, so current densities can have divergence, so (2.12) must be incomplete. This paradox implies there is something missing from the physics. [ Derivation of (5.2): For any volume τ , the net outflow of current through its surface S ∂Q ∂ is equal to the rate of decrease of charge Q inside it; v∫ J.dS = − = − ∫ ρ f dτ . ∂t ∂t τ S
Gauss’ divergence theorem is
∂
v∫ A.dS = ∫τ ∇.Adτ . So v∫ J.dS = ∫τ ∇.Jdτ = − ∫τ ∂t ρ S
2B29 Prep’n for Maxwell’s Equations. Spring 2004
f
dτ .
S
Section 5
1