Wave Optics

NEET Physics · 95 questions · Page 9 of 10 · Click an option or "Show Solution" to reveal answer

Q81
Unpolarized light of intensity I passes through an ideal polarizer A. Another identical polarizer B is placed behind A. The intensity of light beyond B is found to be I/2. Now another identical polarizer C is placed between A and B. The intensity beyond B is now found to be I/8. The angle between polarizer A and C is :
A 60o
B 30o
C 45o
D 0o
Correct Answer
Option C
Solution

As after B intensity of light does not drops, it means both A and B are alligned in single line means their plane of polarization is same.

Let C makes an angle θ\theta with A then C will make θ\theta with B also, as both A and B are alligned in a single line.

So, after C intensity is =

I2{{\rm I} \over 2}

cos2θ\theta , and , intensity after B =

I2{{\rm I} \over 2}

cos2θ\theta ×\times cos2θ\theta According to question,

I2{{\rm I} \over 2}

cos4θ\theta =

I8{{\rm I} \over 8}

\Rightarrow\,\,\, CO4θ\theta =

I4{{\rm I} \over 4}

\Rightarrow

\,\,\,

cosθ\theta =

=12= {1 \over {\sqrt 2 }}

= cos45o

\therefore\,\,\,

θ\theta = 45o

Q82
In a Young’s double slit experiment, light of 500 nm is used to produce an interference pattern. When the distance between the slits is 0.05 mm, the angular width (in degree) of the fringes formed on the distance screen is close to
A 0.17o
B 1.7o
C 0.57o
D 0.07o
Correct Answer
Option C
Solution

β\beta =

λDd{{\lambda D} \over d}

and θ\theta =

βD{\beta \over D}

\Rightarrow θ\theta =

λd{\lambda \over d}

=

500×1090.05×103{{500 \times {{10}^{ - 9}}} \over {0.05 \times {{10}^{ - 3}}}}

= 0.01 rad = 0.57o

Q83
A single slit of width b is illuminated by a coherent monochromatic light of wavelength λ\lambda . If the second and fourthminima in the diffraction pattern at a distance 1 m from the slit are at 3 cm and 6 cm respectively from the central maximum, what is the width of the central maximum ? (i.e. distance between first minimum on either side of the central maximum)
A 1.5 cm
B 3.0 cm
C 4.5 cm
D 6.0 cm
Correct Answer
Option B
Solution

For single slit diffraction, sinθ\theta =

nλb{{n\lambda } \over b}

From central maxima the position of nth minima =

nλDb{{n\lambda D} \over b}

Now when, n = 2, then x2 =

2λDb{{2\lambda D} \over b}

= 0.03 . . . .(1) n = 4, then x4 =

4λDb{{4\lambda D} \over b}

= 0.06 . . . .(2) Performing (2) - (1) we get, x4 - x2 =

2λDb{{2\lambda D} \over b}

= 0.03

\therefore\,\,\,
λDb{{\lambda D} \over b}

=

0.032{{0.03} \over 2}

As, width of crntral maximum =

2λDb{{2\lambda D} \over b}

= 2 ×\times

0.032{{0.03} \over 2}

= 0.03 m = 3 cm

Q84
Two coherent sources produce waves of different intensities which interfere. After interference, the ratio of the maximum intensity to the minimum intensity is 16. The intensity of the waves are in the ratio :
A 16 : 9
B 25 : 9
C 4 : 1
D 5 : 3
Correct Answer
Option B
Solution

Given that,

ImaxImin=161{{{{\rm I}_{\max }}} \over {{{\mathop{\rm I}\nolimits} _{min}}}} = {{16} \over 1}

We know, Imax ==

(I1+I2)2{\left( {\sqrt {{{\rm I}_1}} + \sqrt {{{\rm I}_2}} } \right)^2}

and Imin

=(I1I2)2= {\left( {\sqrt {{{\rm I}_1}} - \sqrt {{{\rm I}_2}} } \right)^2}

\therefore

(I1+I2)2(I1I2)2=161{{{{\left( {\sqrt {{{\rm I}_1}} + \sqrt {{{\rm I}_2}} } \right)}^2}} \over {{{\left( {\sqrt {{{\rm I}_1}} - \sqrt {{{\rm I}_2}} } \right)}^2}}} = {{16} \over 1}

\Rightarrow

I1+I2I1I2=41{{\sqrt {{{\rm I}_1}} + \sqrt {{{\rm I}_2}} } \over {\sqrt {{{\rm I}_1}} - \sqrt {{{\rm I}_2}} }} = {4 \over 1}

\Rightarrow

4I14I2=I1+I24\sqrt {{{\rm I}_1}} - 4\sqrt {{{\rm I}_2}} = \sqrt {{{\rm I}_1}} + \sqrt {{{\rm I}_2}}

\Rightarrow

3I1=5I23\sqrt {{{\rm I}_1}} = 5\sqrt {{{\rm I}_2}}

\Rightarrow

I1I2=53{{\sqrt {{{\rm I}_1}} } \over {\sqrt {{{\rm I}_2}} }} = {5 \over 3}

\Rightarrow

I1I2=259{{{{\rm I}_1}} \over {{{\rm I}_2}}} = {{25} \over 9}
Q85
To demonstrate the phenomenon of interference, we require two sources which emit radiation
A of nearly the same frequency
B of the same frequency
C of different wavelengths
D of the same frequency and having a definite phase relationship
Correct Answer
Option D
Solution

To observe the phenomenon of interference, you need two sources that emit radiation of the same frequency and have a definite phase relationship.

This is because interference is a result of the superposition of waves, which requires the waves to be coherent.

Coherence is achieved when the waves have a constant phase difference, which implies that they are of the same frequency and have a definite phase relationship (a phase relationship that does not change with time).

So, the correct answer is : Option D : of the same frequency and having a definite phase relationship.

Q86
Given below are two statements : Statement I : If the Brewster's angle for the light propagating from air to glass is θB\mathrm{\theta_B}, then the Brewster's angle for the light propagating from glass to air is π2θB\dfrac{\pi}{2}-\theta_B Statement II : The Brewster's angle for the light propagating from glass to air is tan1(μg){\tan ^{ - 1}}({\mu _\mathrm{g}}) where μg\mathrm{\mu_g} is the refractive index of glass. In the light of the above statements, choose the correct answer from the options given below :
A Both Statement I and Statement II are false
B Both Statement I and Statement II are true
C Statement I is false but Statement II is true
D Statement I is true but Statement II is false
Correct Answer
Option D
Solution

Case I : Transmitted is \perp to reflected.

i+r=90i+r=90^{\circ} Snell's law μasini=μgsinr\mu_{a} \sin i=\mu_{g} \sin r tani=μgμa\tan i=\dfrac{\mu_{g}}{\mu_{a}} i=tan1(μgμa)=θBi=\tan ^{-1}\left(\dfrac{\mu_{g}}{\mu_{a}}\right)=\theta_{B} Case II : i+r=90i+r=90^{\circ} as transmitted is \perp to reflected.

tani=μaμgi=tan1μaμg=π2θB\tan i=\dfrac{\mu_{a}}{\mu_{g}} \Rightarrow i=\tan ^{-1} \dfrac{\mu_{a}}{\mu_{g}}=\dfrac{\pi}{2}-\theta_{B}

Q87
A single slit of width 0.1 mm is illuminated by a parallel beam of light of wavelength 6000 A\mathop A\limits^ \circ and diffraction bands are observed on a screen 0.5 m from the slit. The distance of the third dark band from the central bright band is :
A 3 mm
B 9 mm
C 4.5 mm
D 1.5 mm
Correct Answer
Option B
Solution

The slit width is a = 0.1 mm = 10-4 m.

The wavelength of the light is λ\lambda = 6000 ×\times 10-10 = 6 ×\times 10-7.

The distance from the slit to diffraction bands is D = 0.5 m.

We calculate the third dark band from the central band as follows:

Asinθ=3λsinθ=3λa=xDA\sin \theta = 3\lambda \Rightarrow \sin \theta = {{3\lambda } \over a} = {x \over D}
x=3λDa=3×6×107×0.5104=9\Rightarrow x = {{3\lambda D} \over a} = {{3 \times 6 \times {{10}^{ - 7}} \times 0.5} \over {{{10}^{ - 4}}}} = 9

mm

Q88
Visible light of wavelength 6000 × \times 10-8 cm falls normally on a single slit and produces a diffraction pattern. It is found that the second diffraction minimum is at 60o from the central maximum. If the first minimum is produced at θ\theta 1, then θ\theta 1, is close to :
A 45o
B 30o
C 25o
D 20o
Correct Answer
Option C
Solution

For 2nd minima

sinθ=2λd\sin \theta = {{2\lambda } \over d }

\Rightarrow

sin60=2λd\sin 60^\circ = {{2\lambda } \over d}

\Rightarrow

λd=34{\lambda \over d} = {{\sqrt 3 } \over 4}

For 1st minima

sinθ1=λd\sin {\theta _1} = {\lambda \over d}

=

34{{\sqrt 3 } \over 4}

\Rightarrow

θ1={\theta _1} =

25o

Q89
In a Young’s double slit experiment with slit separation 0.1 mm, one observes a bright fringe at angle 140{1 \over {40}} by using light of wavelength λ\lambda 1. When the light of wavelength λ\lambda 2 is used a bright fringe is seen at the same angle in the same set up. Given that λ\lambda 1 and λ\lambda 2 are in visible range (380 nm to 740 nm), their values are -
A 400 nm, 500 nm
B 625 nm, 500 nm
C 380 nm, 500 nm
D 380 nm, 525 nm
Correct Answer
Option B
Solution

Path difference = d sinθ\theta \approx dθ\theta = 0.1 ×\times

140{1 \over {40}}

mm = 2500nm or bright fringe, path difference must be integral multiple of λ\lambda. \therefore 2500 = nλ\lambda1 = mλ\lambda2 \therefore λ\lambda1 = 625 (from n = 4), λ\lambda2 = 500 (from m = 5)

Q90
Diameter of the objective lens of a telescope is 250 cm. For light of wavelength 600nm. coming from a distant object, the limit of resolution of the telescope is close to :-
A 3.0 × 10–7 rad
B 4.5 × 10–7 rad
C 1.5 × 10–7 rad
D 2.0 × 10–7 rad
Correct Answer
Option A
Solution

Limit of resolution =

1.22λd{{1.22\lambda } \over d}

=

1.22×600×109250×102{{1.22 \times 600 \times {{10}^{ - 9}}} \over {250 \times {{10}^{ - 2}}}}

= 2.9 × 10–7 rad.

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