Lorenz Gauge and Inhomogeneous Wave Equation PDF

Summary

These lecture notes cover Lorenz gauge and inhomogeneous wave equations. The notes provide formulas and equations related to electromagnetism, describing static and time-varying sources. They are suitable for undergraduate students.

Full Transcript

3 Lorenz gauge and inhomogeneous wave equa- z ρ(r′ ) ′...

3 Lorenz gauge and inhomogeneous wave equa- z ρ(r′ ) ′ r−r tion J(r′) r r′ Last lecture we found out that given the static sources ρ = ρ(r) and J = J(r), y O static fields x E = −∇V and B = ∇ × A satisfying ✬ ✬ ✩ ✩ Electrostatics: (curl-free) Magnetostatics: (divergence-free) ∇·D = ρ ∇·B = 0 ∇×E = 0 ∇×H = J ✫ D = ϵo E ✪ ✫ B = µo H ✪ can be computed using the potentials ✬ ✩ ✬ ✩ ρ(r ) d r, µoJ(r′ ) 3 ′ ′ A(r) = ! V (r) = d3 r′ , ! ′ 4π|r − r′| 4πϵo|r − r | the solution of the solution of ρ ✫ ∇2A = −µoJ. ✪ ∇2 V = −. ✫ ϵo ✪ 1 Over the next two lectures we will explain why in case of time-varying sources ρ = ρ(r, t) and J = J(r, t), ∇·D = ρ the full set of Maxwell’s equations (see margin) can be satisfied by ∇·B = 0 ∂A ∂B ∂t ∇×E = − ∂t E = −∇V − and B = ∇ × A ∂D in terms of delayed or retarded potentials specified as ∂t ∇×H = J+ ✬ ✩ ✬ ✩ ′ ′ | | c d r, µoJ(r′, t − |r−r d r, A(r, t) = c ) 3 ′ ρ(r′ , t − |r−r V (r, t) = ) 3 ′ ! ! 4πϵo|r − r′| 4π|r − r′ | the solution of inhomogeneous wave equation the solution of inhomogeneous wave equation 2 ∂ 2V ρ ∂ 2A ∂t2 ∇ 2 A − µ o ϵo = −µoJ ∂t ∇ V − µ o ϵo 2 = − ✫ ϵo ✫ ✪ ✪ 1 z ρ(r′ , t) is the speed of light in free space. r − r′ µ o ϵo where c ≡ √ ′ J(r′ , t) Note that retarded potentials r r V (r, t) and A(r, t) y are essentially weighted and delayed sums of charge and current densi- O ties x 2 ρ(r, t) and J(r, t), while the fields E and B are obtained by spatial and temporal deriva- z ρ(r′ , t) tives of the potentials. r − r′ ′ J(r′ , t) Alternatively, we can first use r r ′ | c y µoJ(r′, t − |r−r A(r, t) = ) 3 ′ ! d r ⇒ B=∇×A 4π|r − r′ | O and then find the anti-derivative of Ampere’s law x J⇒A⇒B⇒E B ∂E = ϵo ∂t ∇× µo to determine E outside the region where J is non-zero, bypassing the use of scalar retarded potential V (r, t) — that is the most common approach used in radiation studies. We will next verify the procedure outlined above and the start discussing its applications in radiation studies. 3 The full set of Maxwell’s equations is repeated in the margin for con- venience. Divergence-free nature of B compels us to define a vector ∇·D = ρ potential A via ∇·B = 0 ∂B ∂t B=∇×A ∇×E = − just as before. Inserting this in Faraday’s law we get ∂D ∂t ∇×H = J+ ∂ ∂A ) = 0. ∂t ∂t ∇×E=− ∇×A ⇒ ∇ × (E + Evidently ∂A ∂A E+ is curl free, so it must be true that E + ∂t ∂t = −∇V, or ∂A ∂t E = −∇V − in terms of some scalar potential V. Main difference from statics appears to be the need for two poten- tials, instead of one, to represent the electric field E under time- varying conditions. We continue.... Now substitute ∂A ∂t B = ∇ × A and E = −∇V − 4 in the remaining two Maxwell’s equations — Gauss’s and Ampere’s laws ∂ o B) = J + (ϵoE), ∂t ∇ · (ϵoE) = ρ and ∇ × (µ−1 that we have not touched yet. Upon substitutions we get ∂A ∂ ∂A ), ∂t ∂t ∂t ϵo∇ · (−∇V − ) = ρ and ∇ " × #$ ∇ × A% = µoJ + µoϵo (−∇V − ∇(∇ · A) − ∇2A which looks like a big mess. But if we specify ∂V (Lorenz gauge) ∂t ∇ · A = −µoϵo these messy equations simplify as ∂ 2V ρ 2 ∂ 2A = and A µ o ϵ o ∂t2 ∂t2 ∇ 2 V − µ o ϵo − ∇ − = −µoJ ϵo which we recognize as the inhomogeneous or “forced” wave equations for V and A stated earlier on. – The derivation of the decoupled wave equations above hinged upon our use of Lorenz gauge which reduces to the Coulomb gauge, ∇ · A = 0, in static situations. – Note also that the forced wave equations reduce to Poisson’s equa- tions under time-static conditions. 5 – Since we know how to solve the unforced wave equation from ECE 329, and since we know how to solve the Poisson’s equation, it is now a matter of combining those methods to solve the forced wave equations obtained above. Just a few additional comments on gauge selection before we go on (next lecture): Gauge selection amounts to deciding what to assign to ∇ · A. We can make any assignment that pleases us. This is like choosing the ground node in a circuit problem. Whatever simplifies the problem the most is the best gauge to use. – Lorenz gauge is clearly a good one since it led to decoupled wave equations which are very convenient to work with. We can attack the decoupled equations for V and A one at a time. 6

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