Wave Optics

NEET Physics · 95 questions · Page 8 of 10 · Click an option or "Show Solution" to reveal answer

Q71
In a Young's double slit experiment, the ratio of the slit's width is 4 : 1. The ratio of the intensity of maxima to minima, close to the central fringe on the screen, will be :
A 25 : 9
B 4 : 1
C (3+1)4:16{\left( {\sqrt 3 + 1} \right)^4}:16
D 9 : 1
Correct Answer
Option D
Solution
I1=4I0{I_1} = 4{I_0}
I2=I0{I_2} = {I_0}
Imax=(I0+I2)2{I_{\max }} = {\left( {\sqrt {{I_0}} + \sqrt {{I_2}} } \right)^2}
=(2I0+I0)2=9I0= {\left( {2\sqrt {{I_0}} + \sqrt {{I_0}} } \right)^2} = 9{I_0}
Imin=(I1I2)2{I_{\min }} = {\left( {\sqrt {{I_1}} - \sqrt {{I_2}} } \right)^2}
=(2I0I0)2=I0= {\left( {2\sqrt {{I_0}} - \sqrt {{I_0}} } \right)^2} = {I_0}

\therefore

ImaxImin=9I0I0=91{{{{\mathop{\rm I}\nolimits} _{\max }}} \over {{I_{\min }}}} = {{9{I_0}} \over {{I_0}}} = {9 \over 1}
Q72
A beam of plane polarised light of large cross-sectional area and uniform intensity of 3.3 Wm-2 falls normally on a polariser (cross sectional area 3 × \times 10-4 m2) which rotates about its axis with an angular speed of 31.4 rad/s. The energy of light passing through the polariser per revolution, is close to :
A 1.0 × \times 10-5 J
B 1.0 × \times 10-4 J
C 1.5 × \times 10-4 J
D 5.0 × \times 10-4 J
Correct Answer
Option B
Solution

Intensity, I = 3.3 Wm–3 Area, A = 3 × 10–4 m2 Angular speed, ω\omega = 31.4 rad/s

I=I0cos2(ωt)I = {I_0}{\cos ^2}(\omega t)
Iav=I02\Rightarrow {I_{av}} = {{{I_0}} \over 2}

\because

cos2θ\left\langle {{{\cos }^2}\theta } \right\rangle

=

12{1 \over 2}

, in one time period \therefore

E=I02×A×(Δt)E = {{{I_0}} \over 2} \times A \times (\Delta t)

and

Δt=2πω=2×3.1431.4=15s\Delta t = {{2\pi } \over \omega } = {{2 \times 3.14} \over {31.4}} = {1 \over 5}s

\therefore

E=3.32×3×104×15=1×104JE = {{3.3} \over 2} \times 3 \times {10^{ - 4}} \times {1 \over 5} = 1 \times {10^{ - 4}}\,J
Q73
Two light waves having the same wavelength λ\lambda in vacuum are in phase initially. Then the first wave travels a path L1 through a medium of refractive index n1 while the second wave travels a path of length L2 through a medium of refractive index n2 . After this the phase difference between the two waves is :
A 2πλ(n1L1n2L2){{2\pi } \over \lambda }\left( {{n_1}{L_1} - {n_2}{L_2}} \right)
B 2πλ(n2L1n1L2){{2\pi } \over \lambda }\left( {{n_2}{L_1} - {n_1}{L_2}} \right)
C 2πλ(L1n1L2n2){{2\pi } \over \lambda }\left( {{{{L_1}} \over {{n_1}}} - {{{L_2}} \over {{n_2}}}} \right)
D 2πλ(L2n1L1n2){{2\pi } \over \lambda }\left( {{{{L_2}} \over {{n_1}}} - {{{L_1}} \over {{n_2}}}} \right)
Correct Answer
Option A
Solution

Phase difference =

2πλ{{2\pi } \over \lambda }

×\times optical path difference =

2πλ(n1L1n2L2){{2\pi } \over \lambda }\left( {{n_1}{L_1} - {n_2}{L_2}} \right)
Q74
Interference fringes are observed on a screen by illuminating two thin slits 1 mm apart with a light source (λ\lambda = 632.8 nm). The distance between the screen and the slits is 100 cm. If a bright fringe is observed on a screen at a distance of 1.27 mm from the central bright fringe, then the path difference between the waves, which are reaching this point from the slits is close is
A 1.27 μ\mu m
B 2.05 μ\mu m
C 2.87 nm
D 2 nm
Correct Answer
Option A
Solution

y =

nDλd{{nD\lambda } \over d}

\Rightarrow n =

ydDλ{{yd} \over {D\lambda }}

=

1.27×103×1031×632.8×109{{1.27 \times {{10}^{ - 3}} \times {{10}^{ - 3}}} \over {1 \times 632.8 \times {{10}^{ - 9}}}}

= 2 Path difference

Δ\Delta

x = nλ\lambda = 2 ×\times 632.8 nm = 1265.6 nm = 1.27 μ\mum

Q75
When a polaroid sheet is rotated between two crossed polaroids then the transmitted light intensity will be maximum for a rotation of :
A 9090^\circ
B 3030^\circ
C 4545^\circ
D 6060^\circ
Correct Answer
Option C
Solution

Let

I0\mathrm{I}_0

be intensity of unpolarised light incident on first polaroid.

I1=\mathrm{I}_1=

Intensity of light transmitted from

1st 1^{\text{st }}

polaroid

=I02=\frac{\mathrm{I}_0}{2}

θ\theta be the angle between

1st1^{\mathrm{st}}

and

2nd 2^{\text{nd }}

polaroid ϕ\phi be the angle between

2nd 2^{\text{nd }}

and

3rd 3^{\text{rd }}

polaroid

θ+ϕ=90\theta+\phi=90^{\circ}

(as

1st 1^{\text{st }}

and

3rd 3^{\text{rd }}

polaroid are crossed)

ϕ=90θ\phi=90^{\circ}-\theta
I2=\mathrm{I}_2=

Intensity from

2nd 2^{\text{nd }}

polaroid

I2=I1cos2θ=I02cos2θ\mathrm{I}_2=\mathrm{I}_1 \cos ^2 \theta=\frac{\mathrm{I}_0}{2} \cos ^2 \theta
I3=\mathrm{I}_3=

Intensity from

3rd 3^{\text{rd }}

polaroid

I3=I2cos2ϕ\mathrm{I}_3=\mathrm{I}_2 \cos ^2 \phi
I3=I1cos2θcos2ϕ\mathrm{I}_3=\mathrm{I}_1 \cos ^2 \theta \cos ^2 \phi
I3=I02cos2θcos2ϕ\mathrm{I}_3=\frac{\mathrm{I}_0}{2} \cos ^2 \theta \cos ^2 \phi
ϕ=90θ\phi=90-\theta
I3=I02cos2θsin2θI3=I02[2sinθcosθ2]2I3=I08sin22θ\begin{aligned} & I_3=\frac{I_0}{2} \cos ^2 \theta \sin ^2 \theta \\ & I_3=\frac{I_0}{2}\left[\frac{2 \sin \theta \cos \theta}{2}\right]^2 \\ & I_3=\frac{I_0}{8} \sin ^2 2 \theta \end{aligned}
I3\mathrm{I}_3

will be maximum when

sin2θ=1\sin 2 \theta=1
2θ=90θ=45\begin{aligned} & 2 \theta=90^{\circ} \\ & \theta=45^{\circ} \end{aligned}
Q76
A polarizer - analyser set is adjusted such that the intensity of light coming out of the analyser is just 10% of the original intensity. Assuming that the polarizer - analyser set does not absorb any light, the angle by which the analyser need to be rotated further to reduce the output intensity to be zero, is :
A 71.6o
B 90o
C 18.4o
D 45o
Correct Answer
Option C
Solution

I = I0 cos2 θ\theta \Rightarrow

I010{{{I_0}} \over {10}}

= I0 cos2 θ\theta \Rightarrow cos θ\theta =

110{1 \over {\sqrt {10} }}

\Rightarrow θ\theta = 71.6o \therefore ϕ\phi = 90 - 71.6 = 18.4o

Q77
The Young's double slit interference experiment is performed using light consisting of 480 nm and 600 nm wavelengths to form interference patterns. The least number of the bright fringes of 480 nm light that are required for the first coincidence with the bright fringes formed by 600 nm light is
A 8
B 4
C 5
D 6
Correct Answer
Option C
Solution
dsinθ=mλd \sin \theta = m \lambda

For two wavelengths,

λ1=600nm\lambda_1 = 600\,\text{nm}

and

λ2=480nm\lambda_2 = 480\,\text{nm}

, the bright fringes coincide when the conditions

mλ2=nλ1m \lambda_2 = n \lambda_1

are simultaneously satisfied for integers

mm

and

nn

, representing the bright fringe order for each wavelength. Rearranging the equation gives:

mn=λ1λ2=600480=54\frac{m}{n} = \frac{\lambda_1}{\lambda_2} = \frac{600}{480} = \frac{5}{4}

Thus, the smallest positive integers that satisfy this ratio are:

m=5andn=4.m = 5 \quad \text{and} \quad n = 4.

This means the first coincidence of the bright fringes occurs at the 5th bright fringe for the 480 nm light.

Q78
A system of three polarizers P1, P2, P3 is set up such that the pass axis of P3 is crossed with respect to that of P1. The pass axis of P2 is inclined at 60o to the pass axis of P3. When a beam of unpolarized light of intensity I0 is incident on P1, the intensity of light transmitted by the three polarizers is I. The ratio (I0I{{{I_0}} \over I}) equals (nearly) :
A 10.67
B 5.33
C 16.00
D 1.80
Correct Answer
Option A
Solution

When unpolarized light of intensity I0 passes through P1, then intensity I1 =

I02{{{I_0}} \over 2}

as we know, I = I0 cos2θ\theta Given that angle between P2 & P3 = 60o and P1 and P3 are crossed that means angle between P1 and P3 is 90o so angle between P1 and P2 = 90° – 60° = 30° I2 =

I02cos230{{{I_0}} \over 2}{\cos ^2}30^\circ

=

3I08{{3{I_0}} \over 8}

I3 =

3I08cos260{{3{I_0}} \over 8}{\cos ^2}60^\circ

=

3I032{{3{I_0}} \over {32}}

= I \therefore

I0I{{{I_0}} \over I}

=

I03I032{{{I_0}} \over {{{3{I_0}} \over {32}}}}

=

323{{32} \over 3}

= 10.67

Q79
In a Young's double slit experiment, the path difference, at a certain point on the screen, between two interfering waves is 18{1 \over 8} th of wavelength. The ratio of the intensity at this point to that at the centre of a bright fringe is close to :
A 0.94
B 0.85
C 0.74
D 0.80
Correct Answer
Option B
Solution
Δ\Delta

x ==

λ8{\lambda \over 8}
Δ\Delta

ϕ\phi ==

(2π)λλ8=π4{{\left( {2\pi } \right)} \over \lambda }{\lambda \over 8} = {\pi \over 4}

I == I0cos2

(π8)\left( {{\pi \over 8}} \right)
II0={{\rm I} \over {{{\rm I}_0}}} =

cos2

(π8)\left( {{\pi \over 8}} \right)
Q80
The box of a pin hole camera, of length L,L, has a hole of radius a. It is assumed that when the hole is illuminated by a parallel beam of light of wavelength λ\lambda the spread of the spot (obtained on the opposite wall of the camera) is the sum of its geometrical spread and the spread due to diffraction. The spot would then have its minimum size (say bmin{b_{\min }}) when :
A a=λLa = \sqrt {\lambda L} \, and bmin=4λL{b_{\min }} = \sqrt {4\lambda L}
B a=λ2La = {{{\lambda ^2}} \over L} and bmin=4λL{b_{\min }} = \sqrt {4\lambda L}
C a=λ2La = {{{\lambda ^2}} \over L} and bmin=(2λ2L){b_{\min }} = \left( {{{2{\lambda ^2}} \over L}} \right)
D a=λLa = \sqrt {\lambda L} and bmin=(2λ2L){b_{\min }} = \left( {{{2{\lambda ^2}} \over L}} \right)
Correct Answer
Option A
Solution

Given geometrical spread

=a=a

Diffraction spread

=λa×L=λLa= {\lambda \over a} \times L = {{\lambda L} \over a}

The sum

b=a+λLab = a + {{\lambda L} \over a}

For

bb

to be minimum

dbda=0{{db} \over {da}} = 0
dda(a+λLa)=0{d \over {da}}\left( {a + {{\lambda L} \over a}} \right) = 0
a=λLa = \sqrt {\lambda L}
bmin=λL+λL=2λL=4λLb_{min} = \sqrt {\lambda L} + \sqrt {\lambda L} = 2\sqrt {\lambda L} = \sqrt {4\lambda L}
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