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The Wave Equation: Initial Value Example

17th March 2007

We start with the wave equation in 3 dimensions:

∇·~E

−∇2~E=−ω2µε~E which has the solution

~E(~r,t) = Z Z Z h

~A(~k)ej(kct~k·~r) +~B(~k)ej(kct~k·~r)i

d3k (1)

Suppose we are given that at t=0,

~E = 2 sin(k0z)xˆ+3 cos(k1yz η~H = cos(k1y)x−ˆ sin(k2x)yˆ How do we find the fields at later time? At t=0 we have

~E= Z Z Z h

~A(~k)ej(~k·~r) +~B(~k)ej(~k·~r)i d3k and we have from Faraday’s law that

~H=−∇×~E

±jωµ

~H= Z Z Z "

~k×~A(~k)

ωµ ej(~k·~r)−~k×~B(~k) ωµ ej(~k·~r)

# d3k

where the minus sign comes from the time derivitive. We can also write this as η~H=

Z Z Z h

ˆk×~Aej(~k·~r)−ˆk×~Bej(~k·~r)i d3k

If~A and~B had constant directions, clearly, we can write from Eq. 1

~E(~r,t) =~f(~k·~rkct) +~g(~k·~r+kct) Then, the magnetic field is given by

~H(~r,t) = 1 η

k×~f(~k·~rkct)−ˆk×~g(~k·~r+kct)i

Then,

~E×~H=1 η

~f+~g

× ˆk×

~f−~g

=1 η

h~f× ˆk×~f

−~g× ˆk×~gi

1

(2)

where we have ignored the cross terms assuming them to have zero mean. For a uni- form medium, the fields are perpendicular to~k, and the result is

~f×

~k×~f

= εi jlxˆifjlmnkmfn)

= (δimδjn−δinδjm)xˆifjkmfn

= ~k|f|2−~f

~f·~k

= ~k|f|2 So,

~E×H~ = ˆk η

|f|2− |g|2

as expected. The net flux of power along~k is the difference in the power flux in the forward going wave and the backward going wave.

Now consider the initial conditions. There are only three k values present, namely k0ˆz, k1y and kˆ 2x. The directions are got from the multiplying coordinate, since it hasˆ to come out of~k·~r. Since the equation is linear, we can break the problem into three problems, one in each k value.

k0ˆz: ~E=2 sin(k0z)xH~ =0 (H must be along ˆz~ ×xˆ=y

k1y:ˆ ~E=3 cos(k1yz,η~H=cos(k1y)x (The directions ofˆ ~E and~H are consistent with each other)

k2x:ˆ ~E=0,η~H=−sin(k2x)y (ˆ ~E must be along ˆz, so that ˆx׈z=−ˆy) We now solve these problems in turn.

1. For k0ˆz: Since~H is zero at t=0, we require AB=0, i.e., A(k0) =B(k0)and A(−k0) =B(−k0). By inspection we can write

~E(~r,t) = (sin(k0z−ωt) +sin(k0zt))xˆ Then, the magnetic field is given by

η~H(~r,t) = (sin(k0z−ωt)−sin(k0zt))yˆ

2. For k2x:ˆ ηH~ =−sin(k2x)y.ˆ ~E must be along ˆz, and is zero at t=0. Hence,

~A(k2) =−~B(k2). Again, by inspection, we can write

η~H(~r,t) = (−sin(k2x−ωt)−sin(k2xt))yˆ 2 with

~E(~r,t) = (sin(k2x−ωt)−sin(k2xt))ˆz 2 where I have used ˆz× −yˆ=x to obtain the direction ofˆ ~E.

3. For k1y: We have ˆzˆ ×xˆ=y, so the directions ofˆ ~E andH are consistent with each~ other. At t=0,

~E = 3 cos(k1yz H~ = cos(k1y)xˆ

2

(3)

Thus, at k1,

A+B = 3 AB = 1 which yields A(k1) =2, B(k1) =1. Thus

~E(~r,t) = [2 cos(k1y−ωt) +cos(k1yt)]ˆz

~H(~r,t) = [2 cos(k1y−ωt)−cos(k1yt)]xˆ

4. Suppose that in part 3,~H(~r,0) =cos(k1yz. What then? If the wave is to prop- agate along~y, the Ez requires a Hxand a Hzrequires a−Ex. Thus the solution then have been

~E(~r,t) = 3

2[cos(k1y−ωt) +cos(k1yt)]ˆz

−1

2[cos(k1y−ωt)−cos(k1yt)]xˆ ηH(~ ~r,t) = 3

2[cos(k1y−ωt)−cos(k1yt)]xˆ +1

2[cos(k1y−ωt) +cos(k1yt)]ˆz Thus the missing components of the fields would have appeared once t>0.

5. Suppose that in part 3,H(~ ~r,0) =sin(k1y)x. Then, we would have hadˆ f(z) +g(z) = 3 cos(k1y)

f(z)−g(z) = sin(k1y) Clearly the solution is

f(z) = 3

2cos(k1y) +1

2sin(k1y) g(z) = 3

2cos(k1y)−1

2sin(k1y) i.e.,

~E(~r,t) = 3

2[cos(k1y−ωt) +cos(k1yt)]ˆz +1

2[sin(k1y−ωt)−sin(k1yt)]ˆz

~H(~r,t) = 3

2[cos(k1y−ωt)−cos(k1yt)]xˆ +1

2[sin(k1y−ωt) +sin(k1yt)]xˆ

3

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