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Chapter 3

Waves and Optics

MBBS and BDS entrance past exam questions

Past questions and answers

67 questions set from this chapter. Most repeated first.

  • 2013 · NEET-UG (India) · 4 marks

A wave travelling in the +x+x-direction having displacement along yy-direction as 1 m, wavelength 2π2\pi m and frequency of 1π\frac1\pi Hz is represented by:
(a) y=sin⁡(x−2t)y=\sin(x-2t) (b) y=sin⁡(2πx−2πt)y=\sin(2\pi x-2\pi t) (c) y=sin⁡(10πx−20πt)y=\sin(10\pi x-20\pi t) (d) y=sin⁡(2πx+2πt)y=\sin(2\pi x+2\pi t)

Answer

(a) y=sin⁡(x−2t)y=\sin(x-2t)

Amplitude is 1 m. k=2πλ=1k=\frac{2\pi}{\lambda}=1 and ω=2πf=2\omega=2\pi f=2 rad/s. A wave in the +x+x direction has the form y=Asin⁡(kx−ωt)=sin⁡(x−2t)y=A\sin(kx-\omega t)=\sin(x-2t). Option (d) has +ωt+\omega t, so it travels in −x-x.

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  • 2013 · NEET-UG (India) · 4 marks

If we study the vibration of a pipe open at both ends, then the following statement is not true:
(a) Open end will be antinode (b) Odd harmonics of the fundamental frequency will be generated (c) All harmonics of the fundamental frequency will be generated (d) Pressure change will be maximum at both ends

Answer

(b) Odd harmonics of the fundamental frequency will be generated

A pipe open at both ends has antinodes (maximum pressure variation) at both ends, and produces all harmonics: f=nv2Lf=\frac{nv}{2L}, n=1,2,3,…n=1,2,3,\dots Only odd harmonics occur in a pipe closed at one end, so the statement in (b) is the false one.

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  • 2013 · NEET-UG (India) · 4 marks

A source of unknown frequency gives 4 beats/s, when sounded with a source of known frequency 250 Hz. The second harmonic of the source of unknown frequency gives five beats per second, when sounded with a source of frequency 513 Hz. The unknown frequency is:
(a) 254 Hz (b) 246 Hz (c) 240 Hz (d) 260 Hz

Answer

(a) 254 Hz

The unknown frequency is 250±4250\pm4, i.e. 246 or 254 Hz. Its second harmonic is 492 or 508 Hz. Beats with 513 Hz would be 21 or 5 per second; only 508 gives 5, so n=254n=254 Hz.

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  • 2013 · NEET-UG (India) · 4 marks

A plano convex lens fits exactly into a plano concave lens. Their plane surfaces are parallel to each other. If lenses are made of different materials of refractive indices μ1\mu_1 and μ2\mu_2 and RR is the radius of curvature of the curved surface of the lenses, then the focal length of the combination is:
(a) R2(μ1+μ2)\frac{R}{2(\mu_1+\mu_2)} (b) R2(μ1−μ2)\frac{R}{2(\mu_1-\mu_2)} (c) R(μ1−μ2)\frac{R}{(\mu_1-\mu_2)} (d) 2R(μ2−μ1)\frac{2R}{(\mu_2-\mu_1)}

Answer

(c) R(μ1−μ2)\frac{R}{(\mu_1-\mu_2)}

Plano-convex lens: 1f1=μ1−1R\frac1{f_1}=\frac{\mu_1-1}{R}. Plano-concave lens (the curved face has the same radius): 1f2=−μ2−1R\frac1{f_2}=-\frac{\mu_2-1}{R}. Combined: 1f=μ1−μ2R\frac1f=\frac{\mu_1-\mu_2}{R}, so f=Rμ1−μ2f=\frac{R}{\mu_1-\mu_2}.

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  • 2013 · NEET-UG (India) · 4 marks

For a normal eye, the cornea of eye provides a converging power of 40 D and the least converging power of the eye lens behind the cornea is 20 D. Using this information, the distance between the retina and the cornea-eye lens can be estimated to be:
(a) 5 cm (b) 2.5 cm (c) 1.67 cm (d) 1.5 cm

Answer

(c) 1.67 cm

Powers add for lenses in contact: P=40+20=60P=40+20=60 D, so f=160f=\frac1{60} m ≈1.67\approx1.67 cm. For a normal eye viewing distant objects the image forms on the retina, so the retina lies at the focal length, 1.67 cm.

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  • 2013 · NEET-UG (India) · 4 marks

In Young's double slit experiment, the slits are 2 mm apart and are illuminated by photons of two wavelengths λ1=12000\lambda_1=12000 Å and λ2=10000\lambda_2=10000 Å. At what minimum distance from the common central bright fringe on the screen 2 m from the slit will a bright fringe from one interference pattern coincide with a bright fringe from the other?
(a) 8 mm (b) 6 mm (c) 4 mm (d) 3 mm

Answer

(b) 6 mm

Bright fringes coincide when n1λ1=n2λ2n_1\lambda_1=n_2\lambda_2: 12n1=10n212n_1=10n_2, so the smallest integers are n1=5n_1=5, n2=6n_2=6. y=n1λ1Dd=5×1.2×10−6×22×10−3=6×10−3y=\frac{n_1\lambda_1D}{d}=\frac{5\times1.2\times10^{-6}\times2}{2\times10^{-3}}=6\times10^{-3} m =6=6 mm.

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  • 2014 · NEET-UG (India) · 4 marks

If n1n_1, n2n_2 and n3n_3 are the fundamental frequencies of three segments into which a string is divided, then the original fundamental frequency nn of the string is given by:
(a) 1n=1n1+1n2+1n3\frac{1}{\sqrt n}=\frac{1}{\sqrt{n_1}}+\frac{1}{\sqrt{n_2}}+\frac{1}{\sqrt{n_3}} (b) n=n1+n2+n3\sqrt n=\sqrt{n_1}+\sqrt{n_2}+\sqrt{n_3} (c) n=n1+n2+n3n=n_1+n_2+n_3 (d) 1n=1n1+1n2+1n3\frac1n=\frac1{n_1}+\frac1{n_2}+\frac1{n_3}

Answer

(d) 1n=1n1+1n2+1n3\frac1n=\frac1{n_1}+\frac1{n_2}+\frac1{n_3}

Fundamental frequency is n=12LTμn=\frac1{2L}\sqrt{\frac T\mu}, so n∝1Ln\propto\frac1L for the same tension and mass per length. Since L=L1+L2+L3L=L_1+L_2+L_3, we get 1n=1n1+1n2+1n3\frac1n=\frac1{n_1}+\frac1{n_2}+\frac1{n_3}.

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  • 2014 · NEET-UG (India) · 4 marks

If focal length of objective lens is increased then magnifying power of:
(a) microscope and telescope both will increase. (b) microscope and telescope both will decrease. (c) microscope will decrease but that of telescope will increase. (d) microscope will increase but that of telescope decrease.

Answer

(c) microscope will decrease but that of telescope will increase.

For a telescope, M=fofeM=\frac{f_o}{f_e}, so a larger fof_o increases MM. For a microscope, M≈Lfo(1+Dfe)M\approx\frac{L}{f_o}\left(1+\frac{D}{f_e}\right), so a larger fof_o decreases MM. The two instruments therefore respond in opposite ways, which rules out (a) and (b).

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  • 2014 · NEET-UG (India) · 4 marks

The angle of a prism is AA. One of its refracting surfaces is silvered. Light rays falling at an angle of incidence 2A2A on the first surface returns back through the same path after suffering reflection at the silvered surface. The refractive index μ\mu, of the prism is:
(a) 2cos⁡A2\cos A (b) 12cos⁡A\frac12\cos A (c) tan⁡A\tan A (d) 2sin⁡A2\sin A

Answer

(a) 2cos⁡A2\cos A

The ray retraces its path only if it strikes the silvered face normally, so the angle of refraction at the first face is r=Ar=A (the prism angle). Snell's law: μ=sin⁡2Asin⁡A=2sin⁡Acos⁡Asin⁡A=2cos⁡A\mu=\frac{\sin 2A}{\sin A}=\frac{2\sin A\cos A}{\sin A}=2\cos A. Option (d) comes from wrongly swapping the roles of sin⁡\sin and cos⁡\cos.

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  • 2014 · NEET-UG (India) · 4 marks

The number of possible natural oscillations of air column in a pipe closed at one end of length 85 cm whose frequencies lie below 1250 Hz are: (velocity of sound =340 m s−1=340\ \mathrm{m\,s^{-1}})
(a) 5 (b) 7 (c) 6 (d) 4

Answer

(c) 6

A closed pipe has only odd harmonics: fn=(2n−1)v4Lf_n=\frac{(2n-1)v}{4L}. Fundamental =3404×0.85=100=\frac{340}{4\times0.85}=100 Hz. Possible frequencies are 100,300,500,700,900,1100100, 300, 500, 700, 900, 1100 Hz, and the next one, 13001300 Hz, exceeds 12501250 Hz. So there are 66 natural oscillations; counting even multiples (as for an open pipe) would give a wrong count.

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  • 2014 · NEET-UG (India) · 4 marks

A beam of light of λ=600\lambda=600 nm from a distant source falls on a single slit 1 mm wide and the resulting diffraction pattern is observed on a screen 2 m away. The distance between first dark fringes on either side of the central bright fringe is:
(a) 1.2 mm (b) 2.4 cm (c) 2.4 mm (d) 1.2 cm

Answer

(c) 2.4 mm

The first minima lie at y=±λDay=\pm\frac{\lambda D}{a} from the centre, so the distance between them is the width of the central maximum 2λDa\frac{2\lambda D}{a}. 2×600×10−9×210−3=2.4×10−3\frac{2\times600\times10^{-9}\times2}{10^{-3}}=2.4\times10^{-3} m =2.4=2.4 mm. Option (a) gives only half this width, the distance from the centre to one first minimum.

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  • 2014 · NEET-UG (India) · 4 marks

A speeding motorcyclist sees a traffic jam ahead of him. He slows down to 36 km/hour. He finds that traffic has eased and a car moving ahead of him at 18 km/hour is honking at a frequency of 1392 Hz. If the speed of sound is 343 m/s, the frequency of the honk as heard by him will be:
(a) 1372 Hz (b) 1412 Hz (c) 1454 Hz (d) 1332 Hz

Answer

(a) 1372 Hz

Both move in the same direction (towards the right), the motorcyclist behind at 1010 m/s and the car ahead at 55 m/s. The source moves away from the observer, who is chasing it. f′=f v−vov−vs=1392×343−10343−5=1392×333338≈1372f'=f\,\frac{v-v_o}{v-v_s}=1392\times\frac{343-10}{343-5}=1392\times\frac{333}{338}\approx1372 Hz. Option (b), which is larger than ff, would need the source and observer approaching each other, which is not the case.

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  • 2014 · NEET-UG (India) · 4 marks

In the Young's double-slit experiment, the intensity of light at a point on the screen where the path difference is λ\lambda is KK (λ\lambda being the wave length of light used). The intensity at a point where the path difference is λ/4\lambda/4 will be:
(a) K/4K/4 (b) K/2K/2 (c) Zero (d) KK

Answer

(b) K/2K/2

Intensity is I=4I0cos⁡2ϕ2I=4I_0\cos^2\frac{\phi}{2} with phase difference ϕ=2πλΔx\phi=\frac{2\pi}{\lambda}\Delta x. For Δx=λ\Delta x=\lambda, ϕ=2π\phi=2\pi and I=4I0=KI=4I_0=K. For Δx=λ/4\Delta x=\lambda/4, ϕ=π/2\phi=\pi/2 and I=4I0cos⁡2π4=2I0=K2I=4I_0\cos^2\frac{\pi}{4}=2I_0=\frac{K}{2}. Option (a) wrongly scales the intensity linearly with path difference.

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  • 2015 · NEET-UG (India) · 4 marks

A string is stretched between fixed points separated by 75.0 cm. It is observed to have resonant frequencies of 420 Hz and 315 Hz. There are no other resonant frequencies between these two. The lowest resonant frequency for this string is:
(a) 10.5 Hz (b) 105 Hz (c) 155 Hz (d) 205 Hz

Answer

(b) 105 Hz

For a string fixed at both ends the resonant frequencies are fn=nf1f_n = nf_1, so consecutive harmonics differ by f1f_1. With no resonance between 315 Hz and 420 Hz, they are adjacent harmonics (3rd and 4th), so f1=420−315=105f_1 = 420-315 = 105 Hz.

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  • 2015 · NEET-UG (India) · 4 marks

In an astronomical telescope in normal adjustment a straight black line of length LL is drawn on inside part of objective lens. The eye-piece forms a real image of this line. The length of this image is ll. The magnification of the telescope is:
(a) L+lL−l\frac{L+l}{L-l} (b) Ll\frac{L}{l} (c) Ll+1\frac{L}{l}+1 (d) Ll−1\frac{L}{l}-1

Answer

(b) Ll\dfrac{L}{l}

The eyepiece forms a real image of the line drawn on the objective, whose linear magnification is l/L=v/ul/L = v/u. In normal adjustment the lens separation is fo+fef_o+f_e, so the object distance is u=fo+feu=f_o+f_e and the image distance is v=fe(fo+fe)fov=\dfrac{f_e(f_o+f_e)}{f_o}, giving lL=fefo\dfrac lL=\dfrac{f_e}{f_o}. The telescope magnification is m=fofe=Llm=\dfrac{f_o}{f_e}=\dfrac{L}{l}.

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  • 2015 · NEET-UG (India) · 4 marks

Two slits in Young's experiment have widths in the ratio 1 : 25. The ratio of intensity at the maxima and minima in the interference pattern, ImaxImin\frac{I_{max}}{I_{min}} is:
(a) 49121\frac{49}{121} (b) 49\frac{4}{9} (c) 94\frac{9}{4} (d) 12149\frac{121}{49}

Answer

(c) 94\dfrac{9}{4}

Slit widths are proportional to intensities, so I1:I2=1:25I_1:I_2=1:25 and the amplitudes are in the ratio a1:a2=1:5a_1:a_2=1:5. Then ImaxImin=(a1+a2a1−a2)2=(64)2=94\dfrac{I_{max}}{I_{min}}=\left(\dfrac{a_1+a_2}{a_1-a_2}\right)^2=\left(\dfrac{6}{4}\right)^2=\dfrac94. A common slip is to use the intensity ratio 1:251:25 in place of the amplitude ratio, which gives (26/24)2(26/24)^2 rather than the correct value.

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  • 2015 · NEET-UG (India) · 4 marks

A source of sound S emitting waves of frequency 100 Hz and an observer O are located at some distance from each other. The source is moving with a speed of 19.4 m s−119.4\ \mathrm{m\,s^{-1}} at an angle of 60∘60^\circ with the source-observer line (the velocity of the source makes 60∘60^\circ with the line, pointing partly towards the observer). The observer is at rest. The apparent frequency observed by the observer (velocity of sound in air 330 m s−1330\ \mathrm{m\,s^{-1}}) is:
(a) 106 Hz (b) 97 Hz (c) 100 Hz (d) 103 Hz

Answer

(d) 103 Hz

Only the component of the source velocity along the line to the observer matters: vscos⁡60∘=19.4×0.5=9.7 m s−1v_s\cos60^\circ = 19.4\times0.5=9.7\ \mathrm{m\,s^{-1}}, directed toward the observer. Then f′=fvv−vscos⁡60∘=100×330330−9.7≈103f'=f\dfrac{v}{v-v_s\cos60^\circ}=100\times\dfrac{330}{330-9.7}\approx103 Hz. It is higher than 100 Hz because the source is approaching.

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  • 2016 · NEET-UG (India) · 4 marks

A siren emitting a sound of frequency 800 Hz moves away from an observer towards a cliff at a speed of 15 m s−115\ \mathrm{m\,s^{-1}}. Then, the frequency of sound that the observer hears in the echo reflected from the cliff is: (Take velocity of sound in air =330 m s−1=330\ \mathrm{m\,s^{-1}})
(a) 885 Hz (b) 765 Hz (c) 800 Hz (d) 838 Hz

Answer

(d) 838 Hz

The cliff acts as a stationary observer, then a stationary re-emitter. The siren moves toward the cliff, so the cliff receives f′=800×330330−15≈838f'=800\times\dfrac{330}{330-15}\approx838 Hz. The reflected sound travels back to the observer from the stationary cliff, so no further change occurs and the observer hears 838 Hz. The siren moving away from the observer does not matter, since the observer hears only the echo.

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  • 2016 · NEET-UG (India) · 4 marks

In a diffraction pattern due to a single slit of width aa, the first minimum is observed at an angle 30∘30^\circ when light of wavelength 5000 Å is incident on the slit. The first secondary maximum is observed at an angle of:
(a) sin⁡−1(34)\sin^{-1}\left(\frac{3}{4}\right) (b) sin⁡−1(14)\sin^{-1}\left(\frac{1}{4}\right) (c) sin⁡−1(23)\sin^{-1}\left(\frac{2}{3}\right) (d) sin⁡−1(12)\sin^{-1}\left(\frac{1}{2}\right)

Answer

(a) sin⁡−1(34)\sin^{-1}\left(\dfrac{3}{4}\right)

First minimum: asin⁡30∘=λa\sin30^\circ=\lambda, so a=2λa=2\lambda. The first secondary maximum is approximately at asin⁡θ=3λ2a\sin\theta=\dfrac{3\lambda}{2}, giving sin⁡θ=3λ2×2λ=34\sin\theta=\dfrac{3\lambda}{2\times2\lambda}=\dfrac34, so θ=sin⁡−1(34)\theta=\sin^{-1}\left(\frac34\right).

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  • 2016 · NEET-UG (India) · 4 marks

Match the corresponding entries of column 1 with column 2. [Where mm is the magnification produced by the mirror]
Column 1: (A) m=−2m=-2; (B) m=−12m=-\frac12; (C) m=+2m=+2; (D) m=+12m=+\frac12 Column 2: (a) Convex mirror; (b) Concave mirror; (c) Real image; (d) Virtual image
(a) A→c and d; B→b and d; C→b and c; D→a and d (b) A→b and c; B→b and c; C→b and d; D→a and d (c) A→a and c; B→a and d; C→a and b; D→c and d (d) A→a and d; B→b and c; C→b and d; D→b and c

Answer

(b) A→b and c; B→b and c; C→b and d; D→a and d

A convex mirror always gives a virtual, erect, diminished image, so m=+12m=+\frac12 (D) is convex with a virtual image. A real image is inverted (m<0m<0) and only a concave mirror forms it, so m=−2m=-2 and m=−12m=-\frac12 (A, B) are concave and real. A magnified erect image (m=+2m=+2, C) is virtual and needs a concave mirror with the object inside the focus.

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  • 2016 · NEET-UG (India) · 4 marks

An astronomical telescope has objective and eyepiece of focal lengths 40 cm and 4 cm respectively. To view an object 200 cm away from the objective, the lenses must be separated by a distance:
(a) 54.0 cm (b) 37.3 cm (c) 46.0 cm (d) 50.0 cm

Answer

(a) 54.0 cm

For the objective, u=−200u=-200 cm and fo=40f_o=40 cm: 1v=140−1200=150\frac1v=\frac1{40}-\frac1{200}=\frac1{50}, so v=50v=50 cm. For normal viewing (final image at infinity) the eyepiece is placed at its focal length from this image. So the separation is 50+4=5450+4=54 cm.

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  • 2016 · NEET-UG (India) · 4 marks

The angle of incidence for a ray of light at a refracting surface of a prism is 45∘45^\circ. The angle of prism is 60∘60^\circ. If the ray suffers minimum deviation through the prism, the angle of minimum deviation and refractive index of the material of the prism respectively, are:
(a) 30∘; 1230^\circ;\ \frac{1}{\sqrt2} (b) 45∘; 1245^\circ;\ \frac{1}{\sqrt2} (c) 30∘; 230^\circ;\ \sqrt2 (d) 45∘; 245^\circ;\ \sqrt2

Answer

(c) 30∘; 230^\circ;\ \sqrt2

At minimum deviation r1=r2=A/2=30∘r_1=r_2=A/2=30^\circ and i=45∘i=45^\circ. Then δmin=2i−A=90−60=30∘\delta_{min}=2i-A=90-60=30^\circ. The refractive index is μ=sin⁡45∘sin⁡30∘=1/21/2=2\mu=\dfrac{\sin45^\circ}{\sin30^\circ}=\dfrac{1/\sqrt2}{1/2}=\sqrt2. A value μ<1\mu<1 (options a, b) is impossible for glass in air.

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  • 2016 · NEET-UG (India) · 4 marks

An air column, closed at one end and open at the other, resonates with a tuning fork when the smallest length of the column is 50 cm. The next larger length of the column resonating with the same tuning fork is:
(a) 200 cm (b) 66.7 cm (c) 100 cm (d) 150 cm

Answer

(d) 150 cm

In a closed pipe the resonant lengths are odd multiples of λ/4\lambda/4. The smallest length is λ/4=50\lambda/4=50 cm, so λ=200\lambda=200 cm. The next resonance is at 3λ/4=1503\lambda/4=150 cm.

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  • 2016 · NEET-UG (India) · 4 marks

A uniform rope of length LL and mass m1m_1 hangs vertically from a rigid support. A block of mass m2m_2 is attached to the free end of the rope. A transverse pulse of wavelength λ1\lambda_1 is produced at the lower end of the rope. The wavelength of the pulse when it reaches the top of the rope is λ2\lambda_2. The ratio λ2/λ1\lambda_2/\lambda_1 is:
(a) m1+m2m1\sqrt{\frac{m_1+m_2}{m_1}} (b) m1m2\sqrt{\frac{m_1}{m_2}} (c) m1+m2m2\sqrt{\frac{m_1+m_2}{m_2}} (d) m2m1\sqrt{\frac{m_2}{m_1}}

Answer

(c) m1+m2m2\sqrt{\dfrac{m_1+m_2}{m_2}}

The frequency of the pulse stays the same, so λ∝v=T/μ\lambda\propto v=\sqrt{T/\mu}. At the bottom the tension is m2gm_2g; at the top it is (m1+m2)g(m_1+m_2)g, and μ\mu is the same. So λ2λ1=(m1+m2)gm2g=m1+m2m2\dfrac{\lambda_2}{\lambda_1}=\sqrt{\dfrac{(m_1+m_2)g}{m_2g}}=\sqrt{\dfrac{m_1+m_2}{m_2}}.

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  • 2017 · NEET-UG (India) · 4 marks

Young's double slit experiment is first performed in air and then in a medium other than air. It is found that the 8th bright fringe in the medium lies where the 5th dark fringe lies in air. The refractive index of the medium is nearly
(a) 1.59 (b) 1.69 (c) 1.78 (d) 1.25

Answer

(c) 1.78

Position of the nnth bright fringe is nλD/dn\lambda D/d and of the nnth dark fringe is (n−12)λD/d(n-\tfrac12)\lambda D/d. In the medium the wavelength is λ/μ\lambda/\mu, so 8λ/μ=4.5λ8\lambda/\mu = 4.5\lambda (5th dark in air).

Hence μ=8/4.5≈1.78\mu = 8/4.5 \approx 1.78.

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  • 2017 · NEET-UG (India) · 4 marks

Two cars moving in opposite directions approach each other with speed of 22 m/s and 16.5 m/s respectively. The driver of the first car blows a horn having a frequency 400 Hz. The frequency heard by the driver of the second car is [velocity of sound 340 m/s]
(a) 361 Hz (b) 411 Hz (c) 448 Hz (d) 350 Hz

Answer

(c) 448 Hz

Source and observer approach each other, so f′=f v+vov−vs=400×340+16.5340−22=400×356.5318≈448f'=f\,\dfrac{v+v_o}{v-v_s}=400\times\dfrac{340+16.5}{340-22}=400\times\dfrac{356.5}{318}\approx448 Hz.

Using a minus in the numerator or a plus in the denominator would give the receding-case values (such as 361 Hz), which is wrong here.

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  • 2017 · NEET-UG (India) · 4 marks

The ratio of resolving powers of an optical microscope for two wavelengths λ1=4000\lambda_1=4000 Å and λ2=6000\lambda_2=6000 Å is
(a) 9:49:4 (b) 3:23:2 (c) 16:8116:81 (d) 8:278:27

Answer

(b) 3:23:2

Resolving power of a microscope is R=2μsin⁡θ1.22λ∝1λR=\dfrac{2\mu\sin\theta}{1.22\lambda}\propto\dfrac1\lambda.

So R1:R2=λ2:λ1=6000:4000=3:2R_1:R_2=\lambda_2:\lambda_1=6000:4000=3:2. The squared ratio 9:49:4 is wrong because the dependence is linear.

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  • 2017 · NEET-UG (India) · 4 marks

A thin prism having refracting angle 10∘10^\circ is made of glass of refractive index 1.42. This prism is combined with another thin prism of glass of refractive index 1.7. This combination produces dispersion without deviation. The refracting angle of second prism should be
(a) 6∘6^\circ (b) 8∘8^\circ (c) 10∘10^\circ (d) 4∘4^\circ

Answer

(a) 6∘6^\circ

For dispersion without deviation the net deviation is zero: (μ−1)A+(μ′−1)A′=0(\mu-1)A+(\mu'-1)A'=0 in magnitude.

(1.42−1)(10∘)=(1.7−1)A′(1.42-1)(10^\circ)=(1.7-1)A', so A′=4.2/0.7=6∘A'=4.2/0.7=6^\circ.

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  • 2017 · NEET-UG (India) · 4 marks

The two nearest harmonics of a tube closed at one end and open at the other end are 220 Hz and 260 Hz. What is the fundamental frequency of the system?
(a) 20 Hz (b) 30 Hz (c) 40 Hz (d) 10 Hz

Answer

(a) 20 Hz

A closed pipe has only odd harmonics fn=(2k+1)f0f_n=(2k+1)f_0, so adjacent harmonics differ by 2f02f_0.

2f0=260−220=402f_0=260-220=40 Hz, so f0=20f_0=20 Hz (220 and 260 are the 11th and 13th harmonics).

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  • 2017 · NEET-UG (India) · 4 marks

A beam of light from a source LL is incident normally on a plane mirror fixed at a certain distance xx from the source. The beam is reflected back as a spot on a scale placed just above the source LL. When the mirror is rotated through a small angle θ\theta, the spot of the light is found to move through a distance yy on the scale. The angle θ\theta is given by
(a) yx\dfrac{y}{x} (b) x2y\dfrac{x}{2y} (c) xy\dfrac{x}{y} (d) y2x\dfrac{y}{2x}

Answer

(d) y2x\dfrac{y}{2x}

Rotating the mirror by θ\theta turns the reflected ray by 2θ2\theta. The spot moves y=xtan⁡2θ≈2θxy=x\tan2\theta\approx2\theta x for small angles.

So θ=y2x\theta=\dfrac{y}{2x}. Option (a) forgets the doubling.

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  • 2017 · NEET-UG (India) · 4 marks

Two polaroids P1P_1 and P2P_2 are placed with their axes perpendicular to each other. Unpolarised light I0I_0 is incident on P1P_1. A third polaroid P3P_3 is kept in between P1P_1 and P2P_2 such that its axis makes an angle 45∘45^\circ with that of P1P_1. The intensity of transmitted light through P2P_2 is
(a) I04\dfrac{I_0}{4} (b) I08\dfrac{I_0}{8} (c) I016\dfrac{I_0}{16} (d) I02\dfrac{I_0}{2}

Answer

(b) I08\dfrac{I_0}{8}

P1P_1 transmits half of the unpolarised light: I1=I0/2I_1=I_0/2. Then by Malus's law through P3P_3 at 45∘45^\circ: I2=I02cos⁡245∘=I0/4I_2=\tfrac{I_0}{2}\cos^245^\circ=I_0/4.

P2P_2 is 45∘45^\circ from P3P_3 too, so I3=I04cos⁡245∘=I0/8I_3=\tfrac{I_0}{4}\cos^245^\circ=I_0/8.

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  • 2018 · NEET-UG (India) · 4 marks

An object is placed at a distance of 40 cm from a concave mirror of focal length 15 cm. If the object is displaced through a distance of 20 cm towards the mirror, the displacement of the image will be
(a) 36 cm towards the mirror (b) 30 cm away from the mirror (c) 30 cm towards the mirror (d) 36 cm away from the mirror

Answer

(d) 36 cm away from the mirror

Mirror formula with f=−15f=-15 cm. For u=−40u=-40: 1v=−115+140\tfrac1v=-\tfrac1{15}+\tfrac1{40}, so v=−24v=-24 cm. After moving 20 cm closer, u=−20u=-20: 1v=−115+120\tfrac1v=-\tfrac1{15}+\tfrac1{20}, so v=−60v=-60 cm.

The image moves from 24 cm to 60 cm in front of the mirror, a shift of 36 cm away from the mirror.

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  • 2018 · NEET-UG (India) · 4 marks

The refractive index of the material of a prism is 2\sqrt{2} and the angle of the prism is 30∘30^\circ. One of the two refracting surfaces of the prism is made a mirror inwards, by silver coating. A beam of monochromatic light entering the prism from the other face will retrace its path (after reflection from the silvered surface) if its angle of incidence on the prism is
(a) Zero (b) 60∘60^\circ (c) 30∘30^\circ (d) 45∘45^\circ

Answer

(d) 45∘45^\circ

The ray retraces its path only if it strikes the silvered face normally. With prism angle A=30∘A=30^\circ, r1+r2=Ar_1+r_2=A and r2=0r_2=0, so r1=30∘r_1=30^\circ.

Snell's law: sin⁡i=2sin⁡30∘=12\sin i=\sqrt2\sin30^\circ=\tfrac{1}{\sqrt2}, so i=45∘i=45^\circ.

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  • 2018 · NEET-UG (India) · 4 marks

A tuning fork is used to produce resonance in a glass tube. The length of the air column in the tube can be adjusted by a variable piston. At room temperature of 27∘27^\circC two successive resonances are produced at 20 cm and 73 cm column length. If the frequency of the tuning fork is 320 Hz, the velocity of sound in air at 27∘27^\circC is
(a) 300 m/s (b) 330 m/s (c) 350 m/s (d) 339 m/s

Answer

(d) 339 m/s

Successive resonances in a closed tube differ by λ/2\lambda/2: λ/2=73−20=53\lambda/2 = 73 - 20 = 53 cm, so λ=106\lambda = 106 cm. v=fλ=320×1.06=339.2v = f\lambda = 320 \times 1.06 = 339.2 m/s. Using λ/4=20\lambda/4 = 20 cm would ignore the end correction and give the wrong value.

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  • 2018 · NEET-UG (India) · 4 marks

The fundamental frequency in an open organ pipe is equal to the third harmonic of a closed organ pipe. If the length of the closed organ pipe is 20 cm, the length of the open organ pipe is
(a) 16 cm (b) 13.2 cm (c) 12.5 cm (d) 8 cm

Answer

(b) 13.2 cm

Third harmonic of a closed pipe: f=3v4Lc=3v0.8f = \dfrac{3v}{4L_c} = \dfrac{3v}{0.8}. Fundamental of an open pipe: f=v2Lof = \dfrac{v}{2L_o}. Equating, Lo=0.86=0.1333L_o = \dfrac{0.8}{6} = 0.1333 m ≈13.2\approx 13.2 cm.

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  • 2018 · NEET-UG (India) · 4 marks

Unpolarised light is incident from air on a plane surface of a material of refractive index μ\mu. At a particular angle of incidence ii, it is found that the reflected and refracted rays are perpendicular to each other. Which of the following options is correct for this situation?
(a) i=tan⁡−1(1μ)i=\tan^{-1}\left(\dfrac{1}{\mu}\right) (b) Reflected light is polarised with its electric vector parallel to the plane of incidence (c) i=sin⁡−1(1μ)i=\sin^{-1}\left(\dfrac{1}{\mu}\right) (d) Reflected light is polarised with its electric vector perpendicular to the plane of incidence

Answer

(d) Reflected light is polarised with its electric vector perpendicular to the plane of incidence

Reflected and refracted rays at 90∘90^\circ is Brewster's condition, so tan⁡i=μ\tan i = \mu (not 1/μ1/\mu or sin⁡i=1/μ\sin i = 1/\mu). Only the component perpendicular to the plane of incidence is reflected, so the reflected light is plane polarised with E perpendicular to that plane.

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  • 2018 · NEET-UG (India) · 4 marks

In Young's double slit experiment the separation dd between the slits is 2 mm, the wavelength λ\lambda of the light used is 5896 Å and the distance DD between the screen and slits is 100 cm. It is found that the angular width of the fringes is 0.20∘0.20^\circ. To increase the fringe angular width to 0.21∘0.21^\circ (with same λ\lambda and DD) the separation between the slits needs to be changed to
(a) 1.7 mm (b) 1.8 mm (c) 2.1 mm (d) 1.9 mm

Answer

(d) 1.9 mm

Angular fringe width θ=λ/d\theta = \lambda/d, so d∝1/θd \propto 1/\theta for fixed λ\lambda. d2=2 mm×0.200.21≈1.9d_2 = 2\ \text{mm} \times \dfrac{0.20}{0.21} \approx 1.9 mm. A wider angle needs closer slits.

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  • 2018 · NEET-UG (India) · 4 marks

An astronomical refracting telescope will have large angular magnification and high angular resolution, when it has an objective lens of
(a) small focal length and small diameter (b) small focal length and large diameter (c) large focal length and large diameter (d) large focal length and small diameter

Answer

(c) large focal length and large diameter

Angular magnification of a telescope is m=fo/fem = f_o/f_e, so a large fof_o is needed. Resolving power is proportional to the aperture DD (limit 1.22λ/D1.22\lambda/D), so a large diameter is needed too.

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  • 2019 · NEET-UG (India) · 4 marks

In a double slit experiment, when light of wavelength 400 nm was used, the angular width of the first minima formed on a screen placed 1 m away was found to be 0.2∘0.2^\circ. What will be the angular width of the first minima if the entire experimental apparatus is immersed in water? (μwater=4/3\mu_{water}=4/3)
(a) 0.266∘0.266^\circ (b) 0.15∘0.15^\circ (c) 0.05∘0.05^\circ (d) 0.1∘0.1^\circ

Answer

(b) 0.15∘0.15^\circ

Angular width θ∝λ\theta \propto \lambda, and in a medium λ′=λ/μ\lambda' = \lambda/\mu. θ′=0.2∘×34=0.15∘\theta' = 0.2^\circ \times \dfrac34 = 0.15^\circ.

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  • 2019 · NEET-UG (India) · 4 marks

Which colour of light has the longest wavelength?
(a) Red (b) Blue (c) Green (d) Violet

Answer

(a) Red

In the visible spectrum red has the longest wavelength (about 700 nm) and violet the shortest (about 400 nm). So the order of wavelength is red > green > blue > violet.

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  • 2019 · NEET-UG (India) · 4 marks

Two similar thin equi-convex lenses, of focal length ff each, are kept coaxially in contact with each other such that the focal length of the combination is F1F_1. When the space between the two lenses is filled with glycerin (which has the same refractive index (μ=1.5\mu=1.5) as that of glass) then the equivalent focal length is F2F_2. The ratio F1:F2F_1:F_2 will be
(a) 2:12:1 (b) 1:21:2 (c) 2:32:3 (d) 3:43:4

Answer

(b) 1:21:2

In contact, 1/F1=2/f1/F_1 = 2/f, so F1=f/2F_1 = f/2. Glycerin has the same index as glass, so the filled combination acts as a single equi-convex lens with the same two curved surfaces: 1/F2=(1.5−1)(2/R)=1/f1/F_2 = (1.5-1)(2/R) = 1/f, so F2=fF_2 = f. Hence F1:F2=1:2F_1:F_2 = 1:2.

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  • 2019 · NEET-UG (India) · 4 marks

Pick the wrong answer in the context of rainbow.
(a) When the light rays undergo two internal reflections in a water drop, a secondary rainbow is formed (b) The order of colours is reversed in the secondary rainbow (c) An observer can see a rainbow when his front is towards the sun (d) Rainbow is a combined effect of dispersion, refraction and reflection of sunlight

Answer

(c) An observer can see a rainbow when his front is towards the sun

A rainbow is seen only when the sun is behind the observer, since light is dispersed and reflected back toward the eye at about 42∘42^\circ from the antisolar point. So (c) is the wrong statement. In the secondary bow, two internal reflections reverse the colour order, and the whole effect is dispersion, refraction and reflection.

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  • 2019 · NEET-UG (India) · 4 marks

In total internal reflection, when the angle of incidence is equal to the critical angle for the pair of media in contact, what will be the angle of refraction?
(a) 180∘180^\circ (b) 0∘0^\circ (c) Equal to angle of incidence (d) 90∘90^\circ

Answer

(d) 90∘90^\circ

At the critical angle, the refracted ray grazes the interface, so the angle of refraction is 90∘90^\circ (from sin⁡C=1μ\sin C=\dfrac{1}{\mu} with sin⁡r=1\sin r=1). Beyond CC there is no refracted ray and total internal reflection occurs.

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  • 2020 · NEET-UG (India) · 4 marks

The Brewster's angle ibi_b for an interface should be
(a) 45∘<ib<90∘45^\circ<i_b<90^\circ (b) ib=90∘i_b=90^\circ (c) 0∘<ib<30∘0^\circ<i_b<30^\circ (d) 30∘<ib<45∘30^\circ<i_b<45^\circ

Answer

(a) 45∘<ib<90∘45^\circ<i_b<90^\circ

Brewster's law: tan⁡ib=μ\tan i_b=\mu. Since μ>1\mu>1 for an interface from air to a denser medium, tan⁡ib>1\tan i_b>1. Hence 45∘<ib<90∘45^\circ<i_b<90^\circ; ib=90∘i_b=90^\circ would need infinite μ\mu.

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  • 2020 · NEET-UG (India) · 4 marks

A ray is incident at an angle of incidence ii on one surface of a small angle prism (with angle of prism AA) and emerges normally from the opposite surface. If the refractive index of the material of the prism is μ\mu, then the angle of incidence is nearly equal to
(a) μA\mu A (b) μA2\dfrac{\mu A}{2} (c) A2μ\dfrac{A}{2\mu} (d) 2Aμ\dfrac{2A}{\mu}

Answer

(a) μA\mu A

Normal emergence means the internal angle at the second face is zero, so the internal angle at the first face is r1=Ar_1=A. Snell's law for small angles: i=μr1=μAi=\mu r_1=\mu A.

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  • 2020 · NEET-UG (India) · 4 marks

Assume that light of wavelength 600 nm is coming from a star. The limit of resolution of a telescope whose objective has a diameter of 2 m is
(a) 7.32×10−77.32\times10^{-7} rad (b) 6.00×10−76.00\times10^{-7} rad (c) 3.66×10−73.66\times10^{-7} rad (d) 1.83×10−71.83\times10^{-7} rad

Answer

(c) 3.66×10−73.66\times10^{-7} rad

Limit of resolution: Δθ=1.22λD=1.22×600×10−92=3.66×10−7\Delta\theta=\dfrac{1.22\lambda}{D}=\dfrac{1.22\times600\times10^{-9}}{2}=3.66\times10^{-7} rad. Omitting the factor 1.22 gives 3.0×10−73.0\times10^{-7}, and forgetting the division by DD gives a much larger value.

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  • 2020 · NEET-UG (India) · 4 marks

In a guitar, two strings AA and BB made of the same material are slightly out of tune and produce beats of frequency 6 Hz. When tension in BB is slightly decreased, the beat frequency increases to 7 Hz. If the frequency of AA is 530 Hz, the original frequency of BB will be
(a) 536 Hz (b) 537 Hz (c) 523 Hz (d) 524 Hz

Answer

(d) 524 Hz

Beat frequency is ∣fA−fB∣=6|f_A - f_B| = 6 Hz, so fB=530±6f_B = 530 \pm 6, i.e. 524 Hz or 536 Hz. Frequency of a string goes as f∝Tf \propto \sqrt{T}, so decreasing the tension of BB lowers fBf_B.

If fBf_B were 536 Hz, lowering it would bring it closer to 530 Hz and the beats would fall below 6 Hz, which contradicts the rise to 7 Hz. With fB=524f_B = 524 Hz, lowering it moves it further from fAf_A, giving 530−523=7530 - 523 = 7 Hz. So the original frequency is 524 Hz (this matches NTA's key).

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  • 2021 · NEET-UG (India) · 4 marks

A lens of large focal length and large aperture is best suited as an objective of an astronomical telescope since:
(a) A large aperture contributes to the quality and visibility of the images (b) A large area of the objective ensures better light gathering power (c) A large aperture provides a better resolution (d) All of the above

Answer

(d) All of the above

A large aperture collects more light (better light gathering and brighter, more visible images) and gives better resolving power (∝D/λ\propto D/\lambda). A large focal length of the objective also gives higher magnification fo/fef_o/f_e. All the stated reasons hold, so (d) is correct.

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  • 2021 · NEET-UG (India) · 4 marks

A convex lens 'A' of focal length 20 cm and a concave lens 'B' of focal length 5 cm are kept along the same axis with a distance 'd' between them. If a parallel beam of light falling on 'A' leaves 'B' as a parallel beam, then the distance 'd' in cm will be:
(a) 50 (b) 30 (c) 25 (d) 15

Answer

(d) 15

For a parallel beam to remain parallel, the lens pair acts as a telescope in normal adjustment: the second focal point of the convex lens must coincide with the focal point of the concave lens. So d=fA−∣fB∣=20−5=15d=f_A-|f_B|=20-5=15 cm. The sum, 25 cm, would apply to two convex lenses.

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  • 2021 · NEET-UG (India) · 4 marks

A point object is placed at a distance of 60 cm from a convex lens of focal length 30 cm. If a plane mirror were put perpendicular to the principal axis of the lens and at a distance of 40 cm from it, the final image would be formed at a distance of:
(a) 30 cm from the plane mirror, it would be a virtual image. (b) 20 cm from the plane mirror, it would be a virtual image. (c) 20 cm from the lens, it would be a real image. (d) 30 cm from the lens, it would be a real image.

Answer

(c) 20 cm from the lens, it would be a real image.

The lens (u=−60u=-60, f=30f=30) forms an image at v=60v=60 cm from the lens, which is 20 cm behind the mirror at 40 cm. The mirror treats this as a virtual object and forms a real image 20 cm in front of the mirror, which is 20 cm from the lens. This matches the answer key's option (c).

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  • 2022 · NEET-UG (India) · 4 marks

In a Young's double slit experiment, a student observes 8 fringes in a certain segment of screen when a monochromatic light of 600 nm wavelength is used. If the wavelength of light is changed to 400 nm, then the number of fringes he would observe in the same region of the screen is:
(a) 6 (b) 8 (c) 9 (d) 12

Answer

(d) 12

Fringe width β=λD/d\beta = \lambda D/d, so the number of fringes in a fixed region is ∝1/λ\propto 1/\lambda. Hence N2=8×600400=12N_2 = 8\times\dfrac{600}{400} = 12.

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  • 2022 · NEET-UG (India) · 4 marks

If the initial tension on a stretched string is doubled, then the ratio of the initial and final speeds of a transverse wave along the string is:
(a) 1 : 1 (b) 2:1\sqrt{2} : 1 (c) 1:21 : \sqrt{2} (d) 1 : 2

Answer

(c) 1:21 : \sqrt{2}

Wave speed on a string is v=T/μv = \sqrt{T/\mu}, so v∝Tv\propto\sqrt{T}. Doubling the tension gives vf=2 viv_f = \sqrt2\,v_i, so vi:vf=1:2v_i : v_f = 1:\sqrt2.

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  • 2022 · NEET-UG (India) · 4 marks

A biconvex lens has radii of curvature, 20 cm each. If the refractive index of the material of the lens is 1.5, the power of the lens is:
(a) +2 D (b) +20 D (c) +5 D (d) Infinity

Answer

(c) +5 D

Lensmaker formula: 1f=(n−1)(1R1−1R2)=0.5(120+120)=120\dfrac1f = (n-1)\left(\dfrac1{R_1}-\dfrac1{R_2}\right) = 0.5\left(\dfrac1{20}+\dfrac1{20}\right) = \dfrac1{20} cm−1^{-1}. So f=20f = 20 cm =0.2= 0.2 m and P=1/f=+5P = 1/f = +5 D.

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  • 2022 · NEET-UG (India) · 4 marks

A light ray falls on a glass surface of refractive index 3\sqrt{3}, at an angle 60∘60^\circ. The angle between the refracted and reflected rays would be:
(a) 30∘30^\circ (b) 60∘60^\circ (c) 90∘90^\circ (d) 120∘120^\circ

Answer

(c) 90∘90^\circ

tan⁡ip=μ=3\tan i_p = \mu = \sqrt3 gives ip=60∘i_p = 60^\circ, so the incidence is at the Brewster angle. Then the reflected and refracted rays are perpendicular. Check: sin⁡60∘/sin⁡r=3\sin60^\circ/\sin r=\sqrt3 gives r=30∘r=30^\circ, and the angle between the rays is 180∘−60∘−30∘=90∘180^\circ-60^\circ-30^\circ=90^\circ.

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  • 2022 · NEET-UG (India) · 4 marks

Two transparent media A and B are separated by a plane boundary. The speed of light in those media are 1.5×1081.5 \times 10^8 m/s and 2.0×1082.0 \times 10^8 m/s, respectively. The critical angle for a ray of light for these two media is:
(a) sin⁡−1(0.500)\sin^{-1}(0.500) (b) sin⁡−1(0.750)\sin^{-1}(0.750) (c) tan⁡−1(0.500)\tan^{-1}(0.500) (d) tan⁡−1(0.750)\tan^{-1}(0.750)

Answer

(b) sin⁡−1(0.750)\sin^{-1}(0.750)

Refractive index is inversely proportional to speed, so A is denser (slower). Total internal reflection occurs going from A to B with sin⁡C=nBnA=vAvB=1.5×1082.0×108=0.75\sin C = \dfrac{n_B}{n_A} = \dfrac{v_A}{v_B} = \dfrac{1.5\times10^8}{2.0\times10^8} = 0.75.

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  • 2023 · NEET-UG (India) · 4 marks

Light travels a distance xx in time t1t_1 in air and 10x10x in time t2t_2 in another denser medium. What is the critical angle for this medium?
(a) sin⁡−1(t2t1)\sin^{-1}\left(\frac{t_2}{t_1}\right) (b) sin⁡−1(10t2t1)\sin^{-1}\left(\frac{10t_2}{t_1}\right) (c) sin⁡−1(t110t2)\sin^{-1}\left(\frac{t_1}{10t_2}\right) (d) sin⁡−1(10t1t2)\sin^{-1}\left(\frac{10t_1}{t_2}\right)

Answer

(d) sin⁡−1(10t1t2)\sin^{-1}\left(\dfrac{10t_1}{t_2}\right)

Speed in air c=x/t1c = x/t_1, speed in the medium v=10x/t2v = 10x/t_2. So n=c/v=t210t1n = c/v = \dfrac{t_2}{10t_1} and sin⁡C=1n=10t1t2\sin C = \dfrac1n = \dfrac{10t_1}{t_2}.

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  • 2023 · NEET-UG (India) · 4 marks

The ratio of frequencies of fundamental harmonic produced by an open pipe to that of closed pipe having the same length is:
(a) 1 : 2 (b) 2 : 1 (c) 1 : 3 (d) 3 : 1

Answer

(b) 2 : 1

An open pipe of length LL has fundamental fo=v2Lf_o = \frac{v}{2L}, while a closed pipe has fc=v4Lf_c=\frac{v}{4L}. Hence fo:fc=2:1f_o : f_c = 2:1.

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  • 2023 · NEET-UG (India) · 4 marks

For Young's double slit experiment, two statements are given below:
Statement I: If screen is moved away from the plane of slits, angular separation of the fringes remains constant. Statement II: If the monochromatic source is replaced by another monochromatic source of larger wavelength, the angular separation of fringes decreases.
In the light of the above statements, choose the correct answer from the options given below:
(a) Both Statement I and Statement II are true. (b) Both Statement I and Statement II are false. (c) Statement I is true but Statement II is false. (d) Statement I is false but Statement II is true.

Answer

(c) Statement I is true but Statement II is false.

Angular fringe separation is θ=λd\theta=\frac{\lambda}{d}, which does not depend on the screen distance DD, so Statement I is true. Increasing λ\lambda increases θ\theta, so Statement II (decreases) is false.

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  • 2023 · NEET-UG (India) · 4 marks

Two thin lenses are of same focal lengths (ff), but one is convex and the other one is concave. When they are placed in contact with each other, the equivalent focal length of the combination will be:
(a) Zero (b) f4\frac{f}{4} (c) f2\frac{f}{2} (d) Infinite

Answer

(d) Infinite

1F=1f+1−f=0\frac1F=\frac1f+\frac{1}{-f}=0, so F=∞F=\infty. The combination acts like a plane glass plate with zero net power.

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  • 2024 · NEET-UG (India) · 4 marks

If the monochromatic source in Young's double slit experiment is replaced by white light, then:
(a) There will be a central dark fringe surrounded by a few coloured fringes (b) There will be a central bright fringe surrounded by a few coloured fringes. (c) All bright fringes will be of equal width (d) Interference pattern will disappear.

Answer

(b) There will be a central bright fringe surrounded by a few coloured fringes.

At the centre the path difference is zero for every colour, so all colours form a bright (white) fringe. Away from it the different fringe widths β=λDd\beta=\frac{\lambda D}{d} separate the colours, giving a few coloured fringes before the pattern washes out. A central dark fringe is wrong, as is equal fringe width.

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  • 2024 · NEET-UG (India) · 4 marks

An unpolarized light beam strikes a glass surface at Brewster's angle. Then:
(a) The refracted light will be completely polarised (b) Both the reflected and refracted light will be completely polarised (c) The reflected light will be completely polarized but the refracted light will be partially polarized (d) The reflected light will be partially polarized.

Answer

(c) The reflected light will be completely polarized but the refracted light will be partially polarized

At Brewster's angle the reflected ray is fully plane polarised (perpendicular to the plane of incidence). The refracted ray contains the rest of the perpendicular component and all the parallel component, so it is only partially polarised.

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  • 2024 · NEET-UG (India) · 4 marks

A small telescope has an objective of focal length 140 cm and an eye piece of focal length 5.0 cm. The magnifying power of telescope for viewing a distant object is:
(a) 28 (b) 17 (c) 32 (d) 34

Answer

(a) 28

For a telescope in normal adjustment viewing a distant object, m=fofem=\frac{f_o}{f_e}. m=1405=28m=\frac{140}{5}=28. Option (d) 34 would come from wrongly adding the focal lengths or using the near-point formula.

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  • 2025 · NEET-UG (India) · 4 marks

The intensity of transmitted light when a polaroid sheet, placed between two crossed polaroids at 22.5∘22.5^\circ from the polarization axis of one of the polaroid, is (I0I_0 is the intensity of polarized light after passing through the first polaroid):
(a) I08\frac{I_0}{8} (b) I016\frac{I_0}{16} (c) I02\frac{I_0}{2} (d) I04\frac{I_0}{4}

Answer

(a) I08\frac{I_0}{8}

The middle polaroid is 22.5∘22.5^\circ from the first axis and so 67.5∘67.5^\circ from the crossed one. By Malus' law: I=I0cos⁡222.5∘cos⁡267.5∘=I0cos⁡222.5∘sin⁡222.5∘I=I_0\cos^2 22.5^\circ\cos^2 67.5^\circ=I_0\cos^2 22.5^\circ\sin^2 22.5^\circ. This equals I0(sin⁡45∘2)2=I08I_0\left(\frac{\sin45^\circ}{2}\right)^2=\frac{I_0}{8}. Option (d) I04\frac{I_0}{4} is not reached at this angle: even the best angle, 45∘45^\circ, gives only I04\frac{I_0}{4}.

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  • 2025 · NEET-UG (India) · 4 marks

A microscope has an objective of focal length 2 cm, eyepiece of focal length 4 cm and the tube length of 40 cm. If the distance of distinct vision of eye is 25 cm, the magnification in the microscope is:
(a) 150 (b) 250 (c) 100 (d) 125

Answer

(d) 125

Using the standard approximation for a compound microscope with the tube length LL taken as the separation of the lenses and the final image at the near point: m≈Lfo⋅Dfem\approx\frac{L}{f_o}\cdot\frac{D}{f_e}. m=402×254=20×6.25=125m=\frac{40}{2}\times\frac{25}{4}=20\times6.25=125.

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  • 2025 · NEET-UG (India) · 4 marks

A pipe open at both ends has a fundamental frequency ff in air. The pipe is now dipped vertically in a water drum to half of its length. The fundamental frequency of the air column is now equal to:
(a) 3f2\frac{3f}{2} (b) 2f2f (c) f2\frac{f}{2} (d) ff

Answer

(d) ff

The open pipe of length LL has f=v2Lf=\frac{v}{2L}. Dipped to half its length, it becomes a closed pipe of length L2\frac L2, with fundamental fnew=v4(L/2)=v2L=ff_{new}=\frac{v}{4(L/2)}=\frac{v}{2L}=f. The frequency is unchanged.

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  • 2025 · NEET-UG (India) · 4 marks

In a certain camera, a combination of four similar thin convex lenses are arranged axially in contact. Then the power of the combination and the total magnification in comparison to the power (pp) and magnification (mm) for each lens will be, respectively:
(a) 4p4p and m4m^4 (b) p4p^4 and m4m^4 (c) 4p4p and 4m4m (d) p4p^4 and 4m4m

Answer

(a) 4p4p and m4m^4

Powers of thin lenses in contact add, so P=p+p+p+p=4pP=p+p+p+p=4p. For lenses in series the image of one is the object of the next, so the magnifications multiply: mtot=m⋅m⋅m⋅m=m4m_{tot}=m\cdot m\cdot m\cdot m=m^4. Options (c) and (d) wrongly add magnifications.

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  • 2025 · NEET-UG (India) · 4 marks

An unpolarized light beam travelling in air is incident on a medium of refractive index 1.73 at Brewster's angle. Then:
(a) Both reflected and transmitted light are perfectly polarized with angles of reflection and refraction close to 60∘60^\circ and 30∘30^\circ, respectively (b) Transmitted light is completely polarized with angle of refraction close to 30∘30^\circ (c) Reflected light is completely polarized and the angle of reflection is close to 60∘60^\circ (d) Reflected light is partially polarized and the angle of reflection is close to 30∘30^\circ

Answer

(c) Reflected light is completely polarized and the angle of reflection is close to 60∘60^\circ

At Brewster's angle tan⁡θB=μ=1.73≈3\tan\theta_B=\mu=1.73\approx\sqrt3, so θB≈60∘\theta_B\approx60^\circ. The reflected ray is then completely plane polarized, perpendicular to the refracted ray. The refracted ray is at 30∘30^\circ but is only partially polarized, which rules out (a) and (b). Option (d) is wrong because the reflected light is fully, not partially, polarized.

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Questions from NEET-UG 2013 (India), Code W (NTA NEET-UG 2013 question paper; only questions on topics in Nepal's MBBS entrance syllabus), AIPMT 2014 (India), main paper (NTA NEET-UG 2014 question paper; only questions on topics in Nepal's MBBS entrance syllabus), NEET-UG 2015 (India), Code C (re-exam) (NTA NEET-UG 2015 question paper; only questions on topics in Nepal's MBBS entrance syllabus), NEET-UG 2016 (India), Phase 1 Code C/R/Y (NTA NEET-UG 2016 question paper; only questions on topics in Nepal's MBBS entrance syllabus), NEET-UG 2017 (India), Code B (NTA NEET-UG 2017 question paper; only questions on topics in Nepal's MBBS entrance syllabus), NEET-UG 2018 (India), Code NN (NTA NEET-UG 2018 question paper; only questions on topics in Nepal's MBBS entrance syllabus), NEET-UG 2019 (India), Code P1 (NTA NEET-UG 2019 question paper; only questions on topics in Nepal's MBBS entrance syllabus), NEET-UG 2020 (India), Code F1 (13 September 2020) (NTA NEET-UG 2020 question paper; only questions on topics in Nepal's MBBS entrance syllabus), NEET-UG 2021 (India), Paper Code O1 (12 September 2021) (NTA NEET-UG 2021 question paper; only questions on topics in Nepal's MBBS entrance syllabus), NEET-UG 2022 (India), Paper Code Q6 (17 July 2022) (NTA NEET-UG 2022 question paper; only questions on topics in Nepal's MBBS entrance syllabus), NEET-UG 2023 (India), 7 May 2023 (NTA NEET-UG 2023 question paper; only questions on topics in Nepal's MBBS entrance syllabus), NEET-UG 2024 (India), Paper Code R3 (5 May 2024) (NTA NEET-UG 2024 question paper; only questions on topics in Nepal's MBBS entrance syllabus) and NEET-UG 2025 (India), Paper Code Narmada 48 (4 May 2025) (NTA NEET-UG 2025 question paper; only questions on topics in Nepal's MBBS entrance syllabus). Answers are written for this site; check them against your class notes.