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Question: A thin film of refractive index 1.5 and thickness \[4 \times {10^{ - 5}}cm\]illuminated by light nor...

A thin film of refractive index 1.5 and thickness 4×105cm4 \times {10^{ - 5}}cmilluminated by light normal to the surface. What wavelength within the visible spectrum will be intensified in the reflected beam?
A) 4800 Ao\mathop A\limits^o
B) 5800 Ao\mathop A\limits^o
C) 6000 Ao\mathop A\limits^o
D) 6800 Ao\mathop A\limits^o

Explanation

Solution

When light falls on a thin film then it reflects back from two different surfaces. First, from the upper surface at the time of entering into the film some light reflects back. Then, at the other boundary where the light tries to exit from the film again it reflects back into the first medium. Now, this two reflected beams interfere due to the extra path length covered by the second reflected beam.

Formula Used: If a light ray reflects back while entering a denser medium from a rarer one its phase changes by an angle π\pi . Hence, in case of thin film to have constructive interference required phase and path difference relation is given as:
2dn2n1cosr=(m12)λ2d\dfrac{{{n_2}}}{{{n_1}}}\cos r = \left( {m - \dfrac{1}{2}} \right)\lambda (1)
Where,
d is the thickness of the film,
n2{n_2} is Refractive index(RI) of the film,
n1{n_1} is the refractive index of the rarer medium,
r is the angle of refraction,
m is order of interference,
λ\lambda is the wavelength of interfering light

Complete step by step answer:
Given:
1. RI of the thin film is n2=1.5{n_2} = 1.5, where RI of air is n1=1{n_1} = 1.
2. Thickness of the thin film is d=4×105cm=4×107md = 4 \times {10^{ - 5}}cm = 4 \times {10^{ - 7}}m.
3. The light enters normally into the surface. Hence, i=r=90i = r = {90^ \circ }. So, cosr=cos90=1\cos r = \cos {90^ \circ } = 1.

To find: The wavelength in the visible spectrum that will be intensified.

Step 1
First rewrite the eq.(1) to find an expression of λ\lambda :
2dn2n1cosr=(m12)λ λ=2dn2cosrn1(m12)  2d\dfrac{{{n_2}}}{{{n_1}}}\cos r = \left( {m - \dfrac{1}{2}} \right)\lambda \\\ \therefore \lambda = \dfrac{{2d{n_2}\cos r}}{{{n_1}\left( {m - \tfrac{1}{2}} \right)}} \\\ (2)

Step 2
Now, substitute the values of d, n2{n_2}and cosr\cos rinto eq.(2) to get the set of solutions for λ\lambda :
λ=2×4×107×1.5×11×(m12)meter=1.2×106(m12)meter=12000(m12)Ao\therefore \lambda = \dfrac{{2 \times 4 \times {{10}^{ - 7}} \times 1.5 \times 1}}{{1 \times \left( {m - \tfrac{1}{2}} \right)}}meter = \dfrac{{1.2 \times {{10}^{ - 6}}}}{{\left( {m - \tfrac{1}{2}} \right)}}meter = \dfrac{{12000}}{{\left( {m - \tfrac{1}{2}} \right)}}\mathop A\limits^o
As the wavelength of visible light is within 3800Ao\mathop A\limits^o to 7000Ao\mathop A\limits^o , so to get the wavelength within visible light range, the value of m must be 3. Then the intensified visible wavelength will be:
λ=12000(312)Ao=12000×25Ao=4800Ao\lambda = \dfrac{{12000}}{{\left( {3 - \tfrac{1}{2}} \right)}}\mathop A\limits^o = 12000 \times \dfrac{2}{5}\mathop A\limits^o = 4800\mathop A\limits^o

Correct answer:
The wavelength within the visible spectrum that will be intensified in the reflected beam is (a) 4800Ao4800\mathop A\limits^o .

Note: While using the constructive interference condition a student might get confused noticing the fraction 12\dfrac{1}{2} subtracted from m-th order. This phase subtraction is necessary to nullify an extra π\pi phase difference that happens when light reflects back while travelling from rarer to denser medium.