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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 SS over a single period TT is given by S=12cμ0E02S = \dfrac{1}{{2c{\mu _0}}}{E_0}^2.

Explanation

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 Wm2W{m^{ - 2}} . We will use the general formula of flux density S=1μ0(E×B)\vec S = \dfrac{1}{{{\mu _0}}}(\vec E \times \vec B) where, E\vec E is the associated electric field component of the electromagnetic wave and B\vec B is the associated magnetic field component of electromagnetic wave, μ0{\mu _0} 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{\mu _0} permeability of free space and 0{ \in _0} permittivity of free space as c=1μ00c = \dfrac{1}{{\sqrt {{\mu _0}{ \in _0}} }} or we can write it as
c2=1μ00{c^2} = \dfrac{1}{{{\mu _0}{ \in _0}}}
1μ0=c20\Rightarrow \dfrac{1}{{{\mu _0}}} = {c^2}{ \in _0} .
Now, from the flux density formula S=1μ0(E×B)S = \dfrac{1}{{{\mu _0}}}(\vec E \times \vec B) we can write it’s as
S=c20(E×B)\vec S = {c^2}{ \in _0}(\vec E \times \vec 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(kxωt)j^\vec E = {E_0}\cos (kx - \omega t)\hat j
B=B0cos(kxωt)k^\Rightarrow \vec B = {B_0}\cos (kx - \omega t)\hat k

Taking the cross product of E=E0cos(kxωt)j^\vec E = {E_0}\cos (kx - \omega t)\hat j and B=B0cos(kxωt)k^\vec B = {B_0}\cos (kx - \omega t)\hat k we have,
E×B=E0B0cos2(kxωt)i^\vec E \times \vec B = {E_0}{B_0}{\cos ^2}(kx - \omega t)\hat i
Now, we have to take the average value of this flux density E×B=E0B0cos2(kxωt)i^\vec E \times \vec B = {E_0}{B_0}{\cos ^2}(kx - \omega t)\hat i over the time period of TT ,
Savg=c20E0B0×1T0Tcos2(kxωt)dt{S_{avg}} = {c^2}{ \in _0}{E_0}{B_0} \times \dfrac{1}{T}\int\limits_0^T {{{\cos }^2}(kx - \omega t)dt}
Now, we need to find the average value of 0Tcos2(kxωt)dt\int\limits_0^T {{{\cos }^2}(kx - \omega t)dt} over the time period of TT ,
Using cos(2θ)=2cos2(θ)1\cos (2\theta ) = 2{\cos ^2}(\theta ) - 1
So, 0Tcos2(kxωt)dt=120T(1+cos2(kxωt))dt\int\limits_0^T {{{\cos }^2}(kx - \omega t)dt} = \dfrac{1}{2}\int\limits_0^T {(1 + \cos 2(kx - \omega t))dt}
Since, dt=t\int {dt} = t and cos(kxωt)dt=sin(kxωt)(ω)\int {\cos (kx - \omega t)dt} = \dfrac{{\sin (kx - \omega t)}}{{( - \omega )}}
0Tcos2(kxωt)dt=12[tsin(kxωt)(ω)]\int\limits_0^T {{{\cos }^2}(kx - \omega t)dt} = \dfrac{1}{2}[t - \dfrac{{\sin (kx - \omega t)}}{{( - \omega )}}]

Putting the limits of t=0t = 0 to t=Tt = T we have,
Since sin(0)=0\sin (0) = 0 and sin(π)=0\sin (\pi ) = 0 so we have,
0Tcos2(kxωt)dt=12[T0]\int\limits_0^T {{{\cos }^2}(kx - \omega t)dt} = \dfrac{1}{2}[T - 0]
0Tcos2(kxωt)dt=T2\Rightarrow \int\limits_0^T {{{\cos }^2}(kx - \omega t)dt} = \dfrac{T}{2}
So put the value of 0Tcos2(kxωt)dt=T2\int\limits_0^T {{{\cos }^2}(kx - \omega t)dt} = \dfrac{T}{2} in the equation Savg=c20E0B0×1T0Tcos2(kxωt)dt{S_{avg}} = {c^2}{ \in _0}{E_0}{B_0} \times \dfrac{1}{T}\int\limits_0^T {{{\cos }^2}(kx - \omega t)dt} we get,
Savg=c20E0B0×1T[T2]{S_{avg}} = {c^2}{ \in _0}{E_0}{B_0} \times \dfrac{1}{T}[\dfrac{T}{2}]
Also we know that, B0=E0c{B_0} = \dfrac{{{E_0}}}{c} and put from equation 1μ0=c20(i)\dfrac{1}{{{\mu _0}}} = {c^2}{ \in _0} \to (i) in above equation we get,
Savg=1μ0E02×12c{S_{avg}} = \dfrac{1}{{{\mu _0}}}{E_0}^2 \times \dfrac{1}{{2c}}
Savg=12cμ0E02\therefore {S_{avg}} = \dfrac{1}{{2c{\mu _0}}}{E_0}^2

Hence, the average value of radiance flux density is proved which is Savg=12cμ0E02{S_{avg}} = \dfrac{1}{{2c{\mu _0}}}{E_0}^2.

Note: It should be remembered that while solving integrations of type f(ax)dx=F(x)a\int {f(ax)dx = \dfrac{{F(x)}}{a}} 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=E0B0c = \dfrac{{{E_0}}}{{{B_0}}}.