Scalar and Vector Potentials, Gauge Conditions
Andersen Ang First created: 2013. Last updated: 2017-Feb-1
1 The vector potential A
Consider EM fields in free space ∂B ∇ × E = − ∂t ∂D ∇ × H = + J ∂t c ∇ · D = ρ ∇ · B = 0 Since B field is non-divergent ( ∇ · B = 0 ), so we can define
B = ∇ × A What A means : The close loop line integral of A = flux pass through that loop. Unlike electrostatics that E is created by charges, in electrodynamics E is created by charges and induced by B, thus a single potential is not sufficient to describe E ∂B ∇ × E = − ∂t ∂A = −∇ × ∂t
∂A ⇐⇒ ∇ × E + = 0 ∂t ∂A ⇐⇒ E + is curl-less ∂t ∂A ⇐⇒ E + = −∇φ ∂t ∂A E = −∇φ − ∂t Thus ∂A B = ∇ × AE = −∇φ − ∂t Vector potential A and scalar potential φ now descripe B and E. * The φ now is not the electric potential. Thus when frequency is high, the electric potential in electrostatic case is not valid anymore. 1 2 Gauge
It is necessary to force some constraints on the definition of A such that the potentials can uniquely describe E and B. Without such constraint, the description is not unique. For example, consider potentials A and φ ∂A B = ∇ × AE = −∇φ − ∂t Now consider another paris of potentials A0 and φ0
A0 = A + ∇ψ
∂ψ φ0 = φ − ∂t Then because curl grad = 0
∇ × A0 = ∇ × A + ∇ × ∇ψ = B | {z } 0 ∂f ∂f And because of mixed derivative equality = ∂x1∂x2 ∂x2∂x1 ∂A0 ∂ψ ∂A ∂ −∇φ0 − = −∇φ + ∇ − + ∇ψ ∂t ∂t ∂t ∂t ∂A ∂ψ ∂ = −∇φ − + ∇ − ∇ψ ∂t ∂t ∂t | {z } 0 = E Thus two potentials are describing the same thing and there is no way to differentiate them.
From observation, such non-uniqueness exists because there is no limitation on the divergence of A. Since B and E do not enforce any limitation on ∇·A , thus we have many different ways to define ∇·A. Different limitation on ∇ · A fits different problem. Thus , a Gauge , is a imposed limitations that cope with the redundant extra degrees of freedom. There are 2 famous gauge in electromagnetics, 1 ∂φ the Coulomb gauge ∇ · A = 0 and the Lorenz gauge ∇ · A + = 0. c2 ∂t 3 d’Alembert equations and the Gauges
With these equations ∂B ∇ × E = − ∂t ∂D B = ∇ × A ∇ × H = + J ∂t c ∂A E = −∇φ − ∇ · D = ρ ∂t ∇ · B = 0 The Ampere’s Law thus becomes
2 ∂D ∇ × H = + J ∂t c ∂E ∇ × B = µ ε + µ J 0 0 ∂t 0 c ∂ ∂A ∇ × ∇ × A = µ ε −∇φ − + µ J 0 0 ∂t ∂t 0 c ∂ ∂2A ∇(∇ · A) − ∇2A = −µ ε ∇φ − µ ε + µ J 0 0 ∂t 0 0 ∂t2 0 c
Rearrange
∂2A ∂φ ∇2A − µ ε − ∇ ∇ · A + µ ε = −µ J 0 0 ∂t2 0 0 ∂t 0 Next, consider the Gauss’s Law for electric field
∇ · D = ρ ρ ∇ · E = ε ∂A ρ ∇ · −∇φ − = ∂t ε ∂ ρ −∇2φ − ∇ · A = ∂t ε
Thus we have the following 2 d’alembert equations
∂2A ∂φ ∇2A − µ ε − ∇ ∇ · A + µ ε = −µ J 0 0 ∂t2 0 0 ∂t 0 ∂ ρ −∇2φ − ∇ · A = ∂t ε Just by looking at the second equation, if ∇ · A = 0 ( Coulomb gauge ) :
2 2 ∂ A ∂ ∇ A − µ0ε0 2 − µ0ε0 ∇φ = −µ0J ∂t ρ∂t ∇2φ = − ε The second equation is the same Laplace equation in electrostatics. ∂φ If Lorenz gauge is used ∇ · A + µ ε = 0, the d’Alembert equations become a symmetric form : 0 0 ∂t ∂2A ∇2A − µ ε = −µ J Current generated 0 0 ∂t2 0 2 2 ∂ φ ρ ∇ φ − µ0ε0 = − Charge generated ∂t ε −END−
3