Question
Question: Show that the average value of radiant flux density \(S\) over a single period \(T\) is given by \(S...
Show that the average value of radiant flux density S over a single period T is given by S=2cμ01E02.
Solution
In electromagnetism, the radiant flux density simple means the net power of an electromagnetic wave passing through a unit area of surface and its SI unit is Wm−2 . We will use the general formula of flux density S=μ01(E×B) where, E is the associated electric field component of the electromagnetic wave and B is the associated magnetic field component of electromagnetic wave, μ0 is called the permeability of the free space.
Complete step by step answer:
As we know that, the speed of light is related with μ0 permeability of free space and ∈0 permittivity of free space as c=μ0∈01 or we can write it as
c2=μ0∈01
⇒μ01=c2∈0 .
Now, from the flux density formula S=μ01(E×B) we can write it’s as
S=c2∈0(E×B)
Let the electromagnetic wave is travelling across the X axes the, electric field and magnetic field component will travel in Y and Z direction and can be written as:
E=E0cos(kx−ωt)j^
⇒B=B0cos(kx−ωt)k^
Taking the cross product of E=E0cos(kx−ωt)j^ and B=B0cos(kx−ωt)k^ we have,
E×B=E0B0cos2(kx−ωt)i^
Now, we have to take the average value of this flux density E×B=E0B0cos2(kx−ωt)i^ over the time period of T ,
Savg=c2∈0E0B0×T10∫Tcos2(kx−ωt)dt
Now, we need to find the average value of 0∫Tcos2(kx−ωt)dt over the time period of T ,
Using cos(2θ)=2cos2(θ)−1
So, 0∫Tcos2(kx−ωt)dt=210∫T(1+cos2(kx−ωt))dt
Since, ∫dt=t and ∫cos(kx−ωt)dt=(−ω)sin(kx−ωt)
0∫Tcos2(kx−ωt)dt=21[t−(−ω)sin(kx−ωt)]
Putting the limits of t=0 to t=T we have,
Since sin(0)=0 and sin(π)=0 so we have,
0∫Tcos2(kx−ωt)dt=21[T−0]
⇒0∫Tcos2(kx−ωt)dt=2T
So put the value of 0∫Tcos2(kx−ωt)dt=2T in the equation Savg=c2∈0E0B0×T10∫Tcos2(kx−ωt)dt we get,
Savg=c2∈0E0B0×T1[2T]
Also we know that, B0=cE0 and put from equation μ01=c2∈0→(i) in above equation we get,
Savg=μ01E02×2c1
∴Savg=2cμ01E02
Hence, the average value of radiance flux density is proved which is Savg=2cμ01E02.
Note: It should be remembered that while solving integrations of type ∫f(ax)dx=aF(x) the constant which is in multiple of integral function will be divided by its integration and the speed of light is a ratio of magnitude of electric field component to the magnetic field component of the electromagnetic wave travelling in free space which can be written as c=B0E0.