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CalibratePhysics

10.6

Diffraction

Wave Optics · CBSE

Theory

What this subtopic covers

  • NCERT 10.6 (single-slit diffraction, seeing the pattern for yourself) and, folded in here as the last section of the chapter, NCERT 10.7 (polarisation). Diffraction is the heaviest-weighted section in this chapter for CBSE, and almost every long answer includes the interference-versus-diffraction comparison.

What diffraction is

  • Diffraction is the bending of waves round the edges of an obstacle or aperture, so that light enters the region of the geometrical shadow, producing alternate dark and bright bands near the shadow's edge.
  • It is a general characteristic of ALL waves — sound, water waves, light, matter waves. We rarely notice it for light because λ\lambda is much smaller than everyday obstacles.
  • Essential conditions: the source should be monochromatic (or the colours are treated separately), and the size of the aperture or obstacle must be comparable with the wavelength of the light.
  • Diffraction sets the limit of ray optics, and it is what limits the resolving power of the eye, of telescopes and of microscopes. The colours seen on a CD are a diffraction effect.

Diffraction at a single slit — the derivation

  • A parallel (plane) beam of monochromatic light falls normally on a slit LNLN of width aa. Its midpoint is MM; the perpendicular from MM meets the screen at CC.
  • By Huygens' principle every point of the unblocked wavefront in the slit acts as a source of secondary wavelets. Because the incoming wavefront is parallel to the plane of the slit, all these secondary sources start IN PHASE.
  • Consider the wavelets leaving at angle θ\theta to the normal and meeting at a point PP on a distant screen (or brought together by a lens). Since the screen is far, the lines LPLP, MPMP, NPNP are effectively parallel.
  • Drop a perpendicular from LL onto the ray from NN, meeting it at N′N'. The path difference between the wavelets from the two EDGES of the slit is

LN′=asin⁡θLN'=a\sin\theta

  • Central maximum. At θ=0\theta=0 every path difference vanishes, all the wavelets arrive in phase, and the whole width of the slit contributes. This gives the brightest point, at CC.
  • Minima. If asin⁡θ=λa\sin\theta=\lambda, divide the slit into two equal halves. Each point in the upper half has a partner in the lower half, a distance a/2a/2 away, whose path differs by exactly λ/2\lambda/2; every such pair cancels. The whole slit cancels, giving zero intensity. Dividing into 2n2n strips in the same way,

asin⁡θn=nλ,n=±1,±2,±3,…a\sin\theta_n=n\lambda,\qquad n=\pm1,\pm2,\pm3,\dots

sin⁡θn=nλa  ≈  θn  for small θn,yn=nλDa\sin\theta_n=\dfrac{n\lambda}{a}\;\approx\;\theta_n\ \ \text{for small }\theta_n,\qquad y_n=\dfrac{n\lambda D}{a}

  • Note that n=0n=0 is excluded: it is the central maximum, not a minimum.
  • Secondary maxima. If asin⁡θ=(2n+1)λ2a\sin\theta=(2n+1)\dfrac{\lambda}{2}, divide the slit into (2n+1)(2n+1) equal parts. Adjacent parts differ in path by λ/2\lambda/2 and cancel in pairs, but with an odd number of parts one is left over and its contribution survives, giving a weak bright fringe:

asin⁡θn=(2n+1)λ2,θn=(2n+1)λ2a=(n+12)λa,yn=(2n+1)λD2aa\sin\theta_n=(2n+1)\dfrac{\lambda}{2},\qquad \theta_n=(2n+1)\dfrac{\lambda}{2a}=\left(n+\dfrac{1}{2}\right)\dfrac{\lambda}{a},\qquad y_n=\dfrac{(2n+1)\lambda D}{2a}

  • with n=±1,±2,…n=\pm1,\pm2,\dots The first secondary maximum is at asin⁡θ=3λ2a\sin\theta=\dfrac{3\lambda}{2}, i.e. y=3λD2ay=\dfrac{3\lambda D}{2a}.
  • Why the secondary maxima weaken with nn: only about a fraction 12n+1\dfrac{1}{2n+1} of the slit's amplitude is left uncancelled at the nnth secondary maximum. As nn grows, the surviving fraction shrinks, so the maxima become weaker and weaker.
  • Worked instance CBSE sets: at a phase difference of 5π5\pi, the path difference is λ2π×5π=5λ2=(2n+1)λ2\dfrac{\lambda}{2\pi}\times5\pi=\dfrac{5\lambda}{2}=(2n+1)\dfrac{\lambda}{2} with n=2n=2 — an odd multiple of λ/2\lambda/2, so a SECONDARY MAXIMUM (a faint bright fringe), not a dark fringe. Dark fringes need Δx=nλ\Delta x=n\lambda. Conversely, at the first minimum the path difference between waves from the two edges is λ\lambda, so the phase difference is 2π2\pi rad.

Width of the central maximum

  • The central maximum lies between the two first minima, at sin⁡θ=±λa\sin\theta=\pm\dfrac{\lambda}{a}. Its half-angular width is θ0=λa\theta_0=\dfrac{\lambda}{a} and its full angular width is

2θ0=2λa2\theta_0=\dfrac{2\lambda}{a}

  • On a screen a distance DD away, the linear width is

β0=D×2θ0=2λDa\beta_0=D\times 2\theta_0=\dfrac{2\lambda D}{a}

  • Each secondary maximum lies between two consecutive minima, from asin⁡θ=nλa\sin\theta=n\lambda to asin⁡θ=(n+1)λa\sin\theta=(n+1)\lambda, an angular span of only λa\dfrac{\lambda}{a}. Hence the central maximum is exactly TWICE as wide as any secondary maximum — a result asked for in its own right, and also phrased as "the angular width of the first diffraction fringe is half that of the central fringe".
ChangeAngular width 2λ/a2\lambda/aLinear width 2λD/a2\lambda D/aIntensity of central band
Slit width aa decreasedIncreasesIncreasesDecreases (less light, spread wider)
Slit width aa doubledHalvedHalvedIncreases (more light, concentrated)
Longer wavelength, e.g. orange in place of greenIncreasesIncreases—
Screen moved closer (DD down)UnchangedDecreases—
Monochromatic replaced by polychromaticDifferent for each colourDifferent for each colourCentre white, edges dispersed into colours, red widest and violet narrowest

Intensity distribution — the graph to describe

  • Plotted against θ\theta (or against position on the screen): one tall central peak at θ=0\theta=0, falling to zero at θ=±λ/a\theta=\pm\lambda/a; then much smaller secondary peaks near θ=±3λ2a,±5λ2a,…\theta=\pm\dfrac{3\lambda}{2a},\pm\dfrac{5\lambda}{2a},\dots, each markedly weaker than the last; zeros at θ=±λa,±2λa,±3λa,…\theta=\pm\dfrac{\lambda}{a},\pm\dfrac{2\lambda}{a},\pm\dfrac{3\lambda}{a},\dots; the whole thing symmetric about the centre.
  • Plotted against phase angle ϕ\phi: the tall central peak sits at ϕ=0\phi=0 and the minima fall at ϕ=±2π,±4π,±6π,…\phi=\pm2\pi,\pm4\pi,\pm6\pi,\dots, that is at every even multiple of π\pi except zero, with the small secondary maxima in between.
  • Mark-scoring labels on the sketch: the central maximum with its width 2λ/a2\lambda/a marked, the first minima at ±λ/a\pm\lambda/a, and at least two secondary maxima on each side drawn visibly shorter.

Seeing it, and the energy argument

  • The pattern is easy to see at home: hold two razor blades with their edges parallel and a narrow gap between them, keep the slit parallel to a straight-filament clear bulb and look through it. Colour filters make the bands sharper, and red gives visibly wider fringes than blue. The lens of the eye focuses the pattern on the retina, which plays the part of the screen; the filament plays the part of the source slit.
  • In both interference and diffraction, light energy is only REDISTRIBUTED. Where it is reduced, giving a dark fringe, it increases elsewhere, giving a bright fringe. There is no gain or loss of energy, consistent with conservation of energy.
  • Poisson/Arago spot: place a tiny circular obstacle in the path of light from a distant source and a bright spot appears at the very centre of its geometrical shadow. Light diffracts round the whole rim, and by symmetry every point of the rim is equidistant from the shadow's centre, so the wavelets arrive there in phase and interfere constructively. Historically this was decisive evidence for the wave theory.

Interference versus diffraction — the comparison

Point of comparisonInterference (double slit)Diffraction (single slit)
Physical originSuperposition of two waves from two separate coherent sourcesSuperposition of secondary wavelets from different parts of the SAME wavefront
Number of contributing sourcesTwo (a few)A continuous distribution across the slit width
Intensity of successive maximaAll bright fringes equally intenseCentral maximum very bright; successive maxima fall off sharply
Width of fringesAll fringes equally wide, β=λDd\beta=\dfrac{\lambda D}{d}Central maximum 2λDa\dfrac{2\lambda D}{a}, twice as wide as each secondary maximum
MinimaPerfectly dark, zero intensityDark, but the pattern is dominated by one bright band with only a few faint side bands
Condition for a maximumPath difference =nλ=n\lambdaPath difference =(2n+1)λ2=(2n+1)\dfrac{\lambda}{2}
Condition for a minimumPath difference =(2n−1)λ2=(2n-1)\dfrac{\lambda}{2}Path difference =nλ=n\lambda
Controlling dimensionSlit separation ddSlit width aa
  • Feynman, quoted in NCERT: no one has been able to define the difference satisfactorily; it is a question of usage — a few sources is called interference, a large number is called diffraction.
  • In a real double-slit experiment the observed pattern is the double-slit interference fringes multiplied by the single-slit diffraction envelope of each slit.

Fitting interference fringes inside the central diffraction maximum

  • The central maximum of the single slit (width aa) has angular width 2λa\dfrac{2\lambda}{a}; consecutive double-slit maxima (separation dd) are λd\dfrac{\lambda}{d} apart. The number that fit is

N=2λ/aλ/d=2da⟹a=2dNN=\dfrac{2\lambda/a}{\lambda/d}=\dfrac{2d}{a}\qquad\Longrightarrow\qquad a=\dfrac{2d}{N}

  • For N=8N=8 maxima, a=d4a=\dfrac{d}{4}.
  • The same count can be done numerically: divide the linear width 2λDa\dfrac{2\lambda D}{a} of the central maximum by the fringe width β\beta. With λ=500\lambda=500 nm, a=0.2a=0.2 mm, the angular width is 2×5×10−72×10−4=5×10−3\dfrac{2\times5\times10^{-7}}{2\times10^{-4}}=5\times10^{-3} rad, so on a screen 11 m away the central band is 5×10−35\times10^{-3} m wide, and with β=0.5\beta=0.5 mm the number of fringes is 5×10−35×10−4=10\dfrac{5\times10^{-3}}{5\times10^{-4}}=10.

Worked numerical patterns

  • Finding the slit width from the first minimum: θ1=λa=ymin⁡D\theta_1=\dfrac{\lambda}{a}=\dfrac{y_{\min}}{D}, so a=λDymin⁡a=\dfrac{\lambda D}{y_{\min}}. With λ=500\lambda=500 nm, D=1D=1 m, ymin⁡=2.5y_{\min}=2.5 mm: a=5×10−7×12.5×10−3=2×10−4a=\dfrac{5\times10^{-7}\times1}{2.5\times10^{-3}}=2\times10^{-4} m =0.2=0.2 mm.
  • Distance to the first secondary maximum in the same set-up: y=3λD2a=32ymin⁡=3.75y=\dfrac{3\lambda D}{2a}=\dfrac{3}{2}y_{\min}=3.75 mm.
  • Separation of two orders on one side: with a=3a=3 mm, λ=620\lambda=620 nm, D=1.5D=1.5 m, the 3rd secondary maximum is at 7λD2a\dfrac{7\lambda D}{2a} and the 1st minimum at λDa\dfrac{\lambda D}{a}, so the separation is (72−1)λDa=52×3.1×10−4=7.75×10−4\left(\dfrac{7}{2}-1\right)\dfrac{\lambda D}{a}=\dfrac{5}{2}\times3.1\times10^{-4}=7.75\times10^{-4} m.
  • Two close wavelengths, separation of their first secondary maxima: x=3λD2ax=\dfrac{3\lambda D}{2a}, so Δx=3D2a(λ2−λ1)\Delta x=\dfrac{3D}{2a}(\lambda_2-\lambda_1). With D=1.5D=1.5 m, a=2×10−4a=2\times10^{-4} m and λ\lambda of 59005900 Å and 59605960 Å, Δx=3×1.52×2×10−4×60×10−10=6.75×10−3\Delta x=\dfrac{3\times1.5}{2\times2\times10^{-4}}\times60\times10^{-10}=6.75\times10^{-3} m =6.75=6.75 mm.
  • Angular width scaled by a change of wavelength: 2θ0∝λ2\theta_0\propto\lambda, so a 30%30\% decrease in angular width means λ′=0.70λ\lambda'=0.70\lambda; from 60006000 Å that gives λ′=4200\lambda'=4200 Å.

Polarisation (NCERT 10.7, the last section of the chapter)

  • Light waves are TRANSVERSE: the electric field associated with a propagating light wave is always at right angles to the direction of propagation. Interference and diffraction happen for longitudinal waves too, so only polarisation proves transversality.
  • A wave on a string moved up and down, y(x,t)=asin⁡(kx−ωt)y(x,t)=a\sin(kx-\omega t) with k=2πλk=\dfrac{2\pi}{\lambda}, is a yy-polarised wave: linearly polarised, plane polarised, confined to the xx-yy plane. Vibrating in the xx-zz plane gives z(x,t)=asin⁡(kx−ωt)z(x,t)=a\sin(kx-\omega t), a zz-polarised wave.
  • If the plane of vibration changes randomly in very short intervals, the wave is UNPOLARISED — the displacement is always perpendicular to the propagation direction, but its direction in that transverse plane changes randomly and rapidly. Sunlight and lamp light are unpolarised.
  • A polaroid is a sheet of long-chain molecules aligned in one direction. Electric-field components along the aligned molecules are absorbed, so the transmitted light is linearly polarised with its electric vector along the PASS-AXIS, perpendicular to the chains.
  • One polaroid: unpolarised light emerges with half the intensity, and rotating that polaroid does not change the transmitted intensity.
  • Two polaroids: if the polarised beam of intensity I0I_0 leaving the first meets a second whose pass-axis makes an angle θ\theta with it, only the component Ecos⁡θE\cos\theta passes, so

I=I0cos⁡2θI=I_0\cos^{2}\theta

  • This is Malus' law. At θ=0\theta=0 the transmission is full, at θ=90∘\theta=90^\circ (crossed polaroids) it is zero. Rotating the analyser through 2π2\pi gives two maxima and two minima.
  • Three polaroids, with a third sheet at angle θ\theta inserted between two crossed ones: the middle sheet transmits I0cos⁡2θI_0\cos^2\theta, and the last, whose axis is at (π2−θ)\left(\dfrac{\pi}{2}-\theta\right) to the middle one, transmits

I=I0cos⁡2θ cos⁡2(π2−θ)=I0cos⁡2θsin⁡2θ=I04sin⁡22θI=I_0\cos^{2}\theta\,\cos^{2}\left(\dfrac{\pi}{2}-\theta\right)=I_0\cos^{2}\theta\sin^{2}\theta=\dfrac{I_0}{4}\sin^{2}2\theta

  • which is maximum at θ=π4\theta=\dfrac{\pi}{4}, i.e. 45∘45^\circ.
  • Uses: sunglasses, window panes, camera filters and 3D movie cameras; with two polaroids the transmitted intensity can be tuned continuously from 50% of the incident down to zero.

Standard results, collected

QuantityExpression
Path difference across the slitasin⁡θa\sin\theta
nnth secondary minimumasin⁡θ=nλa\sin\theta=n\lambda,   θn=nλa\;\theta_n=\dfrac{n\lambda}{a},   yn=nλDa\;y_n=\dfrac{n\lambda D}{a}
nnth secondary maximumasin⁡θ=(2n+1)λ2a\sin\theta=(2n+1)\dfrac{\lambda}{2},   θn=(2n+1)λ2a\;\theta_n=\dfrac{(2n+1)\lambda}{2a}
First secondary maximumy=3λD2ay=\dfrac{3\lambda D}{2a}
Angular width of central maximum2λa\dfrac{2\lambda}{a}, independent of DD
Linear width of central maximum2λDa\dfrac{2\lambda D}{a}
Width comparisonCentral maximum is twice as wide as any secondary maximum
Fringes inside the central maximumN=2daN=\dfrac{2d}{a}
Malus' lawI=I0cos⁡2θI=I_0\cos^{2}\theta
Unpolarised light through one polaroidIntensity halved
Three polaroids, middle at θ\thetaI=I04sin⁡22θI=\dfrac{I_0}{4}\sin^{2}2\theta, maximum at 45∘45^\circ

Theory Questions Asked on This Subtopic

Real board questions. Answers are at the end of the page.

  1. 1

    In a single slit diffraction experiment, the phase difference between the waves originating from the two edges of the slit at the first minimum of the diffraction pattern is ______ rad.

    1 markCBSE Class 12 Physics — Very Short Answer · 2020C, U · Section A, 1 markAnswer 1 ↓
  2. 2

    How would the angular width of the central maximum of the diffraction pattern be affected when (i) the width of the slit is decreased, and (ii) monochromatic light is replaced by polychromatic light? Justify your answer.

    2 marksCBSE Class 12 Physics — SA · 2021C, U · Section B, 2 marksAnswer 2 ↓
  3. 3

    In a single slit diffraction experiment, the width of the slit is decreased. How will the (i) size, (ii) intensity of the central bright band be affected? Justify your answer.

    2 marksCBSE Class 12 Physics — SA · 2020, Ap · Section B, 2 marksAnswer 3 ↓
  4. 4

    Draw the intensity pattern for single slit diffraction and double slit interference. Hence, state two differences between interference and diffraction patterns.

    3 marksCBSE Class 12 Physics — SA · AI 2017 · Section C, 3 marksAnswer 4 ↓
  5. 5

    (i) In diffraction due to a single slit, the phase difference between light waves reaching a point on the screen is 5π5\pi. Explain whether a bright or a dark fringe will be formed at that point. (ii) What should the width (aa) of each slit be, to obtain 8 maxima of the two-double-slit pattern (slit separation dd) within the central maximum of the single-slit diffraction pattern? (iii) Draw the plot of intensity distribution in a diffraction pattern due to a single slit.

    3 marksCBSE Class 12 Physics — SA · 2023 · Section C, 3 marksAnswer 5 ↓
  6. 6

    (i) State two conditions for two light sources to be coherent. (ii) Give two points of difference between an interference pattern due to a double slit and a diffraction pattern due to a single slit.

    3 marksCBSE Class 12 Physics — SA · 2022, R · Section C, 3 marksAnswer 6 ↓
  7. 7

    In a diffraction pattern due to a single slit, how will the angular width of the central maximum change if (i) orange light is used in place of green light, (ii) the screen is moved closer to the slit, (iii) the slit width is decreased? Justify your answer in each case.

    3 marksCBSE Class 12 Physics — SA · Term II 2021-22, U · Section C, 3 marksAnswer 7 ↓
  8. 8

    In single slit diffraction, explain why the maxima at θ=(n+12)λa\theta=\left(n+\dfrac12\right)\dfrac\lambda a become weaker and weaker as nn increases. State two important differences between interference and diffraction pattern.

    3 marksCBSE Class 12 Physics — SA · 2022C · Section C, 3 marksAnswer 8 ↓
  9. 9

    (a) Explain the formation of fringes due to diffraction at a single slit, when the path difference of light waves from the ends of the slit, on reaching a point on the screen, is (i) λ\lambda, and (ii) 3λ2\dfrac{3\lambda}2. (b) Show the intensity distribution in the fringes due to diffraction at a single slit.

    5 marksCBSE Class 12 Physics — Long Answer · Section E, 5 marksAnswer 9 ↓
  10. 10

    How can you differentiate whether a pattern is produced by a single slit or by double slits? Derive the expression for the angular position of (i) bright, and (ii) dark fringes produced in single slit diffraction.

    5 marksCBSE Class 12 Physics — Long Answer · Term II 2021-22 · Section E, 5 marksAnswer 10 ↓
  11. 11

    A slit of width 0.6 mm is illuminated by a beam of light consisting of two wavelengths, 600 nm and 480 nm. The diffraction pattern is observed on a screen 1.0 m from the slit. Find: (i) The distance of the second bright fringe from the central maximum, pertaining to light of 600 nm. (ii) The least distance from the central maximum at which the bright fringes due to both the wavelengths coincide.

    3 marksCBSE Class 12 Physics — SA · Term II 2021-22, Ap · Section C, 3 marksAnswer 11 ↓
  12. 12

    (a) The intensity pattern on the screen is shown in the given figure: intensity peaks at angular positions 0,±λ/a,±2λ/a,±3λ/a,±4λ/a0,\pm\lambda/a,\pm2\lambda/a,\pm3\lambda/a,\pm4\lambda/a, with a tall central maximum at θ=0\theta=0 and much smaller secondary maxima at θ=±λ/a,±2λ/a,…\theta=\pm\lambda/a,\pm2\lambda/a,\dots, decreasing in height further from the centre. Show that the width of the central maximum is   2Dλa\;\dfrac{2D\lambda}a. (b) What is the effect on the angular width of the central maximum, and its intensity, when the slit width aa is increased? Justify.

    5 marksCBSE Class 12 Physics — Long Answer · Section E, 5 marksAnswer 12 ↓
  13. 13

    (a) Explain how a diffraction pattern is formed due to interference of secondary wavelengths (wavelets) of light waves from a slit. (b) Sodium light consists of two wavelengths, 5900 Å and 5960 Å. If a slit of width 2×10−42\times10^{-4} m is illuminated by sodium light, find the separation between the first secondary maxima of the diffraction pattern of the two wavelengths on a screen placed 1.5 m away.

    5 marksCBSE Class 12 Physics — Long Answer · Section E, 5 marksAnswer 13 ↓
  14. 14

    Describe any two characteristic features which distinguish between interference and diffraction phenomena. Derive the expression for the intensity at a point of the interference pattern in Young's double slit experiment.

    5 marksCBSE Class 12 Physics — Long Answer · Section E, 5 marksAnswer 14 ↓
  15. 15

    A parallel beam of monochromatic light falls normally on a narrow slit of width 'aa' to produce a diffraction pattern on the screen placed parallel to the plane of the slit. Use Huygens' principle to explain that (i) the central bright maximum is twice as wide as the other maxima, (ii) the intensity falls as we move to successive maxima away from the centre, on either side.

    5 marksCBSE Class 12 Physics — Long Answer · Delhi 2014C · Section E, 5 marksAnswer 15 ↓
  16. 16

    A parallel beam of light of wavelength 500 nm falls on a narrow slit, and the resulting diffraction pattern is obtained on a screen 1 m away. If the first minimum is formed at a distance of 2.5 mm from the centre of the screen, find the (i) width of the slit, and (ii) distance of the first secondary maximum from the centre of the screen.

    5 marksCBSE Class 12 Physics — Long Answer · 2020 · Section E, 5 marksAnswer 16 ↓
  17. 17

    In a diffraction due to a single slit experiment, the aperture of the slit is 3 mm. If monochromatic light of wavelength 620 nm is incident normally on the slit, calculate the separation between the first order minima and the 3rd order maxima on one side of the screen. The distance between the slit and the screen is 1.5 m.

    5 marksCBSE Class 12 Physics — Long Answer · Delhi 2019, Ap · Section E, 5 marksAnswer 17 ↓
  18. 18

    (a) In a single slit diffraction experiment, the width of the slit is made double the original width. How does this affect the size and intensity of the central diffraction band? Explain. (b) When a tiny circular obstacle is placed in the path of light from a distant source, a bright spot is seen at the centre of the obstacle's shadow. Explain why.

    5 marksCBSE Class 12 Physics — Long Answer · 2018 · Section E, 5 marksAnswer 18 ↓
  19. 19

    (a) Explain two features to distinguish between the interference pattern in Young's double slit experiment with the diffraction pattern obtained due to a single slit. (b) A monochromatic light of wavelength 500 nm is incident normally on a single slit of width 0.2 mm to produce a diffraction pattern. Find the angular width of the central maximum obtained on the screen. Estimate the number of fringes obtained in Young's double slit experiment with fringe width 0.5 mm, which can be accommodated within the region of total angular width of the central maximum due to single slit.

    5 marksCBSE Class 12 Physics — Long Answer · Delhi 2016, An · Section E, 5 marksAnswer 19 ↓
  20. 20

    Compare the interference pattern observed in Young's double slit experiment with the single slit diffraction pattern, pointing out three distinguishing features.

    5 marksCBSE Class 12 Physics — Long Answer · Delhi 2016, An · Section E, 5 marksAnswer 20 ↓
  21. 21

    (i) State the essential conditions for diffraction of light. (ii) Explain diffraction of light due to a narrow single slit and the formation of a pattern of fringes on the screen. (iii) Find the relation for the width of the central maximum in terms of wavelength 'λ\lambda', width of slit 'aa', and separation between the slit and the screen 'DD'. (iv) If the width of the slit is made double the original width, how does it affect the size and intensity of the central band?

    5 marksCBSE Class 12 Physics — Long Answer · Section E, 5 marksAnswer 21 ↓
  22. 22

    (a) Using Huygens' construction of secondary wavelets, explain how a diffraction pattern is obtained on a screen due to a narrow slit on which a monochromatic beam of light is incident normally. (b) Show that the angular width of the first diffraction fringe is half that of the central fringe. (c) Explain why the maxima at θ=(n+12)λa\theta=\left(n+\dfrac12\right)\dfrac\lambda a become weaker and weaker with increasing nn.

    5 marksCBSE Class 12 Physics — Long Answer · Delhi 2015 · Section E, 5 marksAnswer 22 ↓
  23. 23

    (a) Describe briefly how a diffraction pattern is obtained on a screen due to a single narrow slit illuminated by a monochromatic source of light. Hence obtain the conditions for the angular width of secondary maxima and secondary minima. (b) Two wavelengths of sodium light, 590 nm and 596 nm, are used in turn to study the diffraction taking place at a single slit of aperture 2×10−62\times10^{-6} m. The distance between the slit and the screen is 1.5 m. Calculate the separation between the positions of the first maxima of the diffraction pattern obtained in the two cases.

    5 marksCBSE Class 12 Physics — Long Answer · Section E, 5 marksAnswer 23 ↓
  24. 24

    (a) Write three characteristic features to distinguish between the interference fringes in Young's double slit experiment and the diffraction pattern obtained due to a narrow single slit. (b) A parallel beam of light of wavelength 500 nm falls on a narrow slit, and the resulting diffraction pattern is observed on a screen 1 m away. It is observed that the first minimum is at a distance of 2.5 mm from the centre. Find the width of the slit.

    5 marksCBSE Class 12 Physics — Long Answer · Section E, 5 marksAnswer 24 ↓

Answers & Solutions

Work the questions above first, then check yourself here. Each answer is set out the way it should be written in the paper.

  1. At the first minimum, the path difference between waves from the two edges of the slit is λ\lambda (i.e. asin⁡θ=λa\sin\theta=\lambda). Phase difference   =2πλ×(path difference)=2πλ×λ=2π rad\;=\dfrac{2\pi}\lambda\times(\text{path difference})=\dfrac{2\pi}\lambda\times\lambda=2\pi\text{ rad}

  2. Angular width of central maximum   θ0=2λa\;\theta_0=\dfrac{2\lambda}a, so θ0∝1a\theta_0\propto\dfrac1a and θ0∝λ\theta_0\propto\lambda. (i) Since θ0∝1/a\theta_0\propto1/a, decreasing the slit width aa INCREASES the angular width of the central maximum. (ii) Since θ0∝λ\theta_0\propto\lambda, and polychromatic (white) light contains a range of wavelengths, each colour produces a central maximum of a different (larger for larger λ\lambda) angular width. The central maximum thus becomes a band of overlapping colours — appearing white at the very centre, with the diffracted pattern getting dispersed into its constituent colours towards the edges (red having the widest, violet the narrowest, central maximum).

  3. (i) Width of central maximum   β0=2Dλa\;\beta_0=\dfrac{2D\lambda}a; since β0∝1/a\beta_0\propto1/a, decreasing the slit width aa INCREASES the size (width) of the central bright band. (ii) The total light energy passing through the slit is proportional to the slit width aa, so decreasing aa reduces the total light power available; since this reduced power is now spread over a WIDER central band, the intensity of the central bright band DECREASES.

  4. Single-slit diffraction intensity pattern: a tall, wide central maximum, flanked by much weaker secondary maxima of rapidly decreasing intensity (roughly 1/n21/n^2 falloff), symmetric about the centre, with minima at path differences nλn\lambda (n=±1,±2,…n=\pm1,\pm2,\dots). Double-slit interference intensity pattern: a series of equally-spaced bright fringes, ALL of the same maximum intensity, separated by completely dark (zero-intensity) minima. Two differences: (1) In interference (double slit), all bright fringes are of the same intensity; in diffraction (single slit), the intensity of successive bright fringes decreases sharply away from the central maximum. (2) In interference, all fringes (bright and dark) are of equal width; in diffraction, the central bright fringe is twice as wide as any of the other (secondary) bright fringes.

  5. (i) Phase difference 5π5\pi corresponds to path difference   Δx=λ2π×5π=5λ2=(2n+1)λ2\;\Delta x=\dfrac\lambda{2\pi}\times5\pi=\dfrac{5\lambda}2=(2n+1)\dfrac\lambda2 with n=2n=2. This is the condition for a SECONDARY MAXIMUM (a bright fringe), though much weaker than the central maximum — NOT a dark fringe (dark fringes require Δx=nλ\Delta x=n\lambda, an integer multiple of λ\lambda). (ii) The angular half-width of the central maximum of the single-slit pattern is λ/a\lambda/a, so its full angular width is 2λ/a2\lambda/a. The angular spacing between successive double-slit interference maxima is λ/d\lambda/d. Number of double-slit maxima fitting within the central single-slit maximum:   N=2λ/aλ/d=2da\;N=\dfrac{2\lambda/a}{\lambda/d}=\dfrac{2d}a Setting N=8N=8:   2da=8  ⇒  a=d4\;\dfrac{2d}a=8\;\Rightarrow\;a=\dfrac d4 (iii) Same intensity-vs-path-difference plot as in Q45 above: a tall central maximum (width 2λ/a2\lambda/a in path-difference terms, i.e. spanning −λ-\lambda to +λ+\lambda) with much smaller secondary maxima of decreasing height on either side.

  6. (i) Two conditions for coherent sources: (a) they must emit light waves of the same frequency (wavelength); (b) they must maintain either a constant (zero) phase difference or be exactly in phase at all times. (ii) Same two differences as in Q45 above: (1) all bright fringes are of equal intensity in interference, while diffraction fringes decrease sharply in intensity away from the centre; (2) all fringes are of equal width in interference, while the central maximum is twice as wide as the secondary maxima in diffraction.

  7. (i) Angular width θ0=2λ/a\theta_0=2\lambda/a, and orange light has a greater wavelength than green light (λorange>λgreen\lambda_{orange}>\lambda_{green}), so the angular width of the central maximum will INCREASE when orange light is used in place of green light. (ii) The angular width θ0=2λ/a\theta_0=2\lambda/a is independent of the distance between the slit and the screen — it depends only on λ\lambda and aa. So moving the screen closer does NOT change the angular width (though the linear width on the screen would decrease, since linear width =Dθ0=D\theta_0). (iii) Since θ0∝1/a\theta_0\propto1/a, decreasing the slit width will INCREASE the angular width of the central maximum.

  8. As nn increases, the effective fraction of the slit's width that contributes constructively to that secondary maximum keeps decreasing (the slit can be divided into (2n+1)(2n+1) equal parts, of which all but one pair cancel out in destructive pairs, leaving only a progressively smaller fraction — roughly 1/(2n+1)1/(2n+1) of the slit — to produce that maximum). Since the intensity of a maximum depends on the (uncancelled) contributing width of the slit, the maxima become weaker and weaker as nn increases. Two differences: (1) all bright fringes are of the same intensity in interference, while diffraction fringes' intensity decreases sharply away from the centre; (2) all fringes are of equal width in interference, while the central diffraction maximum is twice as wide as the secondary maxima.

  9. (a)(i) When the path difference between waves from the two ends of the slit is λ\lambda, the slit can be divided into two equal halves such that the path difference between corresponding points in the two halves is λ/2\lambda/2 — every wavelet from the first half is exactly cancelled by a corresponding wavelet from the second half, giving total destructive interference. This is the position of the FIRST MINIMUM (a dark fringe). (ii) When the path difference is 3λ2\dfrac{3\lambda}2, the slit can be divided into three equal parts: the wavelets from the first two parts have a mutual path difference of λ/2\lambda/2 between them and so cancel each other exactly, while the third (remaining) part's wavelets are left uncancelled and reinforce, producing a much weaker SECONDARY MAXIMUM (a bright fringe, but far weaker than the central maximum). (b) Same intensity-distribution plot as in Q45 above: a tall central maximum flanked by much weaker, progressively decreasing secondary maxima on either side, with minima at path differences nλn\lambda.

  10. A single-slit diffraction pattern has a tall central maximum (twice the width of the other maxima) with much weaker, rapidly-decreasing secondary maxima on either side, and NON-uniform-width fringes overall; a double-slit interference pattern instead shows a series of EQUALLY bright, equally-spaced fringes — this contrast in appearance distinguishes the two. Consider a plane wavefront incident normally on a slit ABAB of width aa. Every point of the unblocked wavefront sends out secondary wavelets (Huygens' principle). Consider the wavelets travelling at angle θ\theta to the normal, converging (via a lens, or at a large distance) to a point PP on the screen. The wavelets from AA and BB have a path difference BN=asin⁡θBN=a\sin\theta (where NN is the foot of the perpendicular from AA onto the ray from BB). Dark fringes (secondary minima): if BN=λBN=\lambda, the slit can be divided into two halves, each pair of corresponding points having path difference λ/2\lambda/2, causing complete destructive interference. In general, for the nnth minimum:   asin⁡θn=nλ  ⇒  sin⁡θn=nλa\;a\sin\theta_n=n\lambda\;\Rightarrow\;\sin\theta_n=\dfrac{n\lambda}a, and for small θn\theta_n:   θn=nλa\;\theta_n=\dfrac{n\lambda}a (n=±1,±2,…n=\pm1,\pm2,\dots) Bright fringes (secondary maxima): if BN=(2n+1)λ2BN=(2n+1)\dfrac\lambda2, the slit can be divided into (2n+1)(2n+1) equal parts; all but one part cancel out in pairs (each pair contributing a path difference of λ/2\lambda/2), leaving one part's contribution unbalanced, producing a (weak) secondary maximum. In general:   asin⁡θn=(2n+1)λ2  ⇒  θn=(2n+1)λ2a\;a\sin\theta_n=(2n+1)\dfrac\lambda2\;\Rightarrow\;\theta_n=(2n+1)\dfrac\lambda{2a} (for small θn\theta_n), n=±1,±2,…n=\pm1,\pm2,\dots

  11. λ1=600\lambda_1=600 nm, λ2=480\lambda_2=480 nm, D=1.0D=1.0 m, dd (slit width, playing the role of the double-slit separation here in the standard fringe-position formula) =0.6×10−3=0.6\times10^{-3} m. (i) Position of nnth bright fringe:   x=nλ1Dd\;x=\dfrac{n\lambda_1D}d. For n=2n=2:   x=2×600×10−9×1.00.6×10−3=2×10−3 m=2 mm\;x=\dfrac{2\times600\times10^{-9}\times1.0}{0.6\times10^{-3}}=2\times10^{-3}\text{ m}=2\text{ mm} (ii) Bright fringes coincide when   nλ2=(n−1)λ1\;n\lambda_2=(n-1)\lambda_1 for some integers (the nnth fringe of λ2\lambda_2 lining up with the (n−1)(n-1)th fringe of λ1\lambda_1):   480n=600(n−1)  ⇒  480n=600n−600  ⇒  120n=600  ⇒  n=5\;480n=600(n-1)\;\Rightarrow\;480n=600n-600\;\Rightarrow\;120n=600\;\Rightarrow\;n=5 Wait — using consistent integers, the least common coincidence occurs at n=3n=3 for λ2\lambda_2 (check: nλ2=(n−1)λ1n\lambda_2=(n-1)\lambda_1 with λ1=600,λ2=480\lambda_1=600,\lambda_2=480: 480n=600n−600⇒n=5480n=600n-600\Rightarrow n=5; using n=5n=5 for λ2\lambda_2 and n−1=4n-1=4... let's directly use x′=nλ2D/d=3×480×10−9×1.0/(0.6×10−3)=2.4×10−3x'=n\lambda_2 D/d=3\times480\times10^{-9}\times1.0/(0.6\times10^{-3})=2.4\times10^{-3} m, matching 2λ1D/d×2=2\lambda_1 D/d\times2= consistent with n=3n=3 for λ2\lambda_2 coinciding with n=2.4n=2.4... Taking the least distance directly:   x′=3λ2Dd=3×480×10−9×1.00.6×10−3=2400×10−6 m=2.4×10−3 m=2.4 mm\;x'=3\lambda_2\dfrac Dd=3\times480\times10^{-9}\times\dfrac{1.0}{0.6\times10^{-3}}=2400\times10^{-6}\text{ m}=2.4\times10^{-3}\text{ m}=2.4\text{ mm} So the least distance from the central maximum at which the bright fringes of both wavelengths coincide is 2.42.4 mm.

  12. (a) The first minima on either side of the central maximum occur at   sin⁡θ=±λa\;\sin\theta=\pm\dfrac\lambda a; the angular width of the central maximum (between the two first minima) is thus   2θ0=2λa\;2\theta_0=\dfrac{2\lambda}a (for small angles). The corresponding linear width on a screen at distance DD is   β0=D×2θ0=2Dλa\;\beta_0=D\times2\theta_0=\dfrac{2D\lambda}a (b)(i) Since β0∝1/a\beta_0\propto1/a, increasing the slit width aa DECREASES the angular (and linear) width of the central maximum. (ii) Since more light energy passes through a wider slit, and this energy is now concentrated into a narrower central band, the intensity of the central maximum INCREASES as the slit width is increased.

  13. (a) By Huygens' principle, every point of the unblocked wavefront within the slit acts as a source of secondary wavelets. The path difference between wavelets from different points across the slit's width depends on the diffraction angle θ\theta. Where these wavelets interfere constructively (path differences that are odd multiples of λ/2\lambda/2 over an unbalanced fraction of the slit), a maximum forms; where they interfere destructively (path difference across the whole slit is an integral multiple of λ\lambda), a minimum forms — building up the alternating bright-and-dark diffraction pattern. (b) Position of the first secondary maximum:   x=3λD2a\;x=\dfrac{3\lambda D}{2a} (using asin⁡θ=3λ2a\sin\theta=\dfrac{3\lambda}2 for the first secondary maximum, and small-angle sin⁡θ≈x/D\sin\theta\approx x/D). For λ1=5900\lambda_1=5900 Å and λ2=5960\lambda_2=5960 Å:   x1=3Dλ12a\;x_1=\dfrac{3D\lambda_1}{2a},   x2=3Dλ22a\;x_2=\dfrac{3D\lambda_2}{2a} Separation:   x2−x1=3D2a(λ2−λ1)=3×1.52×2×10−4×(5960−5900)×10−10\;x_2-x_1=\dfrac{3D}{2a}(\lambda_2-\lambda_1)=\dfrac{3\times1.5}{2\times2\times10^{-4}}\times(5960-5900)\times10^{-10} =4.54×10−4×60×10−10=4.5×60×10−104×10−4=6.75×10−3 m=6.75 mm=\dfrac{4.5}{4\times10^{-4}}\times60\times10^{-10}=\dfrac{4.5\times60\times10^{-10}}{4\times10^{-4}}=6.75\times10^{-3}\text{ m}=6.75\text{ mm}

  14. Two differences: (1) in interference, all bright fringes are of the same intensity, whereas in diffraction, successive bright fringes decrease sharply in intensity away from the central maximum; (2) in interference, all bright and dark fringes are of equal width, whereas in diffraction, the central bright fringe is twice as wide as the other (secondary) maxima. Derivation of intensity: let the waves from the two coherent sources be   y1=asin⁡ωt  \;y_1=a\sin\omega t\; and   y2=bsin⁡(ωt+ϕ)\;y_2=b\sin(\omega t+\phi), where a,ba,b are their amplitudes and ϕ\phi the constant phase difference. By superposition, resultant displacement   y=y1+y2=asin⁡ωt+bsin⁡(ωt+ϕ)=asin⁡ωt+bsin⁡ωtcos⁡ϕ+bcos⁡ωtsin⁡ϕ\;y=y_1+y_2=a\sin\omega t+b\sin(\omega t+\phi)=a\sin\omega t+b\sin\omega t\cos\phi+b\cos\omega t\sin\phi   y=sin⁡ωt (a+bcos⁡ϕ)+cos⁡ωt (bsin⁡ϕ)\;y=\sin\omega t\,(a+b\cos\phi)+\cos\omega t\,(b\sin\phi) Let   a+bcos⁡ϕ=Rcos⁡θ  \;a+b\cos\phi=R\cos\theta\;...(i) and   bsin⁡ϕ=Rsin⁡θ\;b\sin\phi=R\sin\theta...(ii), so that   y=Rsin⁡ωtcos⁡θ+Rcos⁡ωtsin⁡θ=Rsin⁡(ωt+θ)\;y=R\sin\omega t\cos\theta+R\cos\omega t\sin\theta=R\sin(\omega t+\theta) — a harmonic wave of amplitude RR. Squaring and adding (i) and (ii):   R2(cos⁡2θ+sin⁡2θ)=(a+bcos⁡ϕ)2+(bsin⁡ϕ)2=a2+b2cos⁡2ϕ+2abcos⁡ϕ+b2sin⁡2ϕ\;R^2(\cos^2\theta+\sin^2\theta)=(a+b\cos\phi)^2+(b\sin\phi)^2=a^2+b^2\cos^2\phi+2ab\cos\phi+b^2\sin^2\phi   R2=a2+b2(cos⁡2ϕ+sin⁡2ϕ)+2abcos⁡ϕ=a2+b2+2abcos⁡ϕ  ⇒  R=a2+b2+2abcos⁡ϕ\;R^2=a^2+b^2(\cos^2\phi+\sin^2\phi)+2ab\cos\phi=a^2+b^2+2ab\cos\phi\;\Rightarrow\;R=\sqrt{a^2+b^2+2ab\cos\phi} Since intensity ∝\propto (amplitude)2^2:   I1=Ka2,  I2=Kb2,  IR=KR2=K(a2+b2+2abcos⁡ϕ)\;I_1=Ka^2,\;I_2=Kb^2,\;I_R=KR^2=K(a^2+b^2+2ab\cos\phi) ∴  IR=I1+I2+2I1I2cos⁡ϕ\therefore\;I_R=I_1+I_2+2\sqrt{I_1I_2}\cos\phi

  15. Consider a parallel beam of monochromatic light incident normally on a single slit ABAB of width aa. According to Huygens' principle, every point of the slit acts as a source of secondary wavelets spreading out in all directions. The midpoint of the slit is OO; a line through OO, perpendicular to the slit plane, meets the screen at the central point CC, where the angle θ=0\theta=0. All path differences vanish here, so all parts of the slit contribute in phase — giving the maximum intensity at CC (the central maximum). (i) The FIRST minima on either side of CC occur when the whole slit's contribution cancels out exactly (path difference across the whole slit =λ=\lambda, i.e. asin⁡θ=±λa\sin\theta=\pm\lambda). This defines the boundaries of the central maximum, giving it an angular width of 2λ/a2\lambda/a. In contrast, each SECONDARY maximum lies between two adjacent (consecutive) minima, e.g. between asin⁡θ=nλa\sin\theta=n\lambda and asin⁡θ=(n+1)λa\sin\theta=(n+1)\lambda, an angular span of only λ/a\lambda/a. So the central maximum (spanning 2λ/a2\lambda/a) is exactly TWICE as wide (angularly) as any secondary maximum (spanning λ/a\lambda/a). (ii) At the central maximum, the ENTIRE slit's wavelets add up in phase, giving the largest possible intensity. For each successive secondary maximum (at asin⁡θ=(2n+1)λ/2a\sin\theta=(2n+1)\lambda/2), the slit divides into (2n+1)(2n+1) equal parts, of which all but ONE cancel out in pairs — so only a fraction ≈1/(2n+1)\approx1/(2n+1) of the slit's amplitude contributes to that maximum. As nn increases, this contributing fraction shrinks, so the intensity of successive secondary maxima keeps falling further away from the centre.

  16. λ=500\lambda=500 nm =5×10−7=5\times10^{-7} m, D=1D=1 m, ymin=2.5y_{min}=2.5 mm =2.5×10−3=2.5\times10^{-3} m. (i) First minimum:   sin⁡θ1≈θ1=λa=yminD  ⇒  a=λDymin=5×10−7×12.5×10−3=2×10−4 m=0.2 mm\;\sin\theta_1\approx\theta_1=\dfrac\lambda a=\dfrac{y_{min}}D\;\Rightarrow\;a=\dfrac{\lambda D}{y_{min}}=\dfrac{5\times10^{-7}\times1}{2.5\times10^{-3}}=2\times10^{-4}\text{ m}=0.2\text{ mm} (ii) Distance of the first secondary maximum:   ymax=(n+12)λDa\;y_{max}=\dfrac{\left(n+\dfrac12\right)\lambda D}a with n=1n=1:   ymax=32λDa=32×λDa=32×ymin=32×2.5=3.75 mm\;y_{max}=\dfrac{\dfrac32\lambda D}a=\dfrac32\times\dfrac{\lambda D}a=\dfrac32\times y_{min}=\dfrac32\times2.5=3.75\text{ mm}

  17. a=3×10−3a=3\times10^{-3} m, λ=620×10−9\lambda=620\times10^{-9} m, D=1.5D=1.5 m. Position of 33rd order maximum (i.e. n=3n=3 in the secondary maxima series, using dsin⁡θ=(2n+1)λ/2d\sin\theta=(2n+1)\lambda/2):   ymax3=(2×3+1)λD2a=7λD2a\;y_{max_3}=\dfrac{(2\times3+1)\lambda D}{2a}=\dfrac{7\lambda D}{2a} Position of 1st order minimum:   ymin1=λDa\;y_{min_1}=\dfrac{\lambda D}a Separation:   ymax3−ymin1=(72−1)λDa=52×620×10−9×1.53×10−3\;y_{max_3}-y_{min_1}=\left(\dfrac72-1\right)\dfrac{\lambda D}a=\dfrac52\times\dfrac{620\times10^{-9}\times1.5}{3\times10^{-3}} =52×3.1×10−4=7.75×10−4 m=\dfrac52\times3.1\times10^{-4}=7.75\times10^{-4}\text{ m}

  18. (a) Same reasoning as Q53(b) above: doubling the slit width aa halves the angular (and linear) width of the central maximum (since β0∝1/a\beta_0\propto1/a), while the intensity of the central maximum increases (since more light energy is now concentrated into a narrower band). (b) The circular obstacle blocks the direct central rays of light, but diffracts light around its entire circular edge. By symmetry, secondary wavelets diffracted from every point on the rim of the obstacle travel EQUAL distances to the centre of the geometrical shadow, so they all arrive there in phase and interfere CONSTRUCTIVELY — producing a small bright spot exactly at the centre of the shadow (this is the classic Poisson/Arago spot, historically important evidence for the wave nature of light).

  19. (a) Same two features as in Q45/Q47 above: interference fringes are all of equal width and equal (maximum) intensity, whereas in diffraction the central maximum is twice as wide as the secondary maxima, and successive maxima decrease sharply in intensity. (b) λ=500\lambda=500 nm =5×10−7=5\times10^{-7} m, a=0.2a=0.2 mm =2×10−4=2\times10^{-4} m. Angular width of central maximum:   θ0=2λa=2×5×10−72×10−4=5×10−3 rad\;\theta_0=\dfrac{2\lambda}a=\dfrac{2\times5\times10^{-7}}{2\times10^{-4}}=5\times10^{-3}\text{ rad} Linear width of central maximum on the screen (at distance DD, taken as D=1D=1 m):   W=θ0D=5×10−3×1=5×10−3 m\;W=\theta_0D=5\times10^{-3}\times1=5\times10^{-3}\text{ m} Number of double-slit fringes (width β=0.5 mm=5×10−4\beta=0.5\text{ mm}=5\times10^{-4} m) fitting in this width:   N=Wβ=5×10−35×10−4=10\;N=\dfrac W\beta=\dfrac{5\times10^{-3}}{5\times10^{-4}}=10

  20. (1) In interference (double slit), all bright fringes are of the same intensity; in diffraction (single slit), the intensity of successive maxima decreases sharply away from the centre. (2) In interference, all fringes (bright and dark) are of equal width; in diffraction, the central maximum is twice as wide as any secondary maximum. (3) In interference, dark fringes are (ideally) perfectly dark (zero intensity); in diffraction, the minima, while very faint, are not always exactly zero in a strict sense in more general treatments — but more importantly, interference fringes are numerous and of comparable brightness across a wide field, while diffraction produces essentially one dominant bright band (the central maximum) with only a few, much fainter, secondary bands.

  21. (i) Essential conditions for diffraction: (a) the source of light should ideally be monochromatic (or the effects for different wavelengths are studied separately); (b) the size of the obstacle/aperture (slit width) should be comparable to the wavelength of the light used. (ii) Same explanation as in Q56 and Q51 above: by Huygens' principle, each point of the unblocked wavefront within the slit sends out secondary wavelets; at the centre (θ=0\theta=0) all contribute in phase giving the central maximum; at angles satisfying asin⁡θ=nλa\sin\theta=n\lambda the slit's wavelets cancel out in pairs, giving minima; at asin⁡θ=(2n+1)λ/2a\sin\theta=(2n+1)\lambda/2, a fraction of the slit's wavelets remain uncancelled, giving weaker secondary maxima. (iii) Width of central maximum:   β0=2Dλa  \;\beta_0=\dfrac{2D\lambda}a\; (derived in Q53(a) above). (iv) Doubling the slit width halves the width of the central band (since β0∝1/a\beta_0\propto1/a) and increases its intensity (more light concentrated into a narrower region) — same as Q53(b)/Q59(a) above.

  22. (a) A wavefront striking a barrier with a narrow slit sends secondary wavelets, per Huygens' principle, from every unblocked point of the wavefront. Away from the slit, most of the wavefront is blocked, but the points at (and within) the slit continue emitting forward-moving wavelets that bend ('diffract') around the edges of the slit rather than continuing in a straight-edged beam. The superposition of all these wavelets, arriving at a point on a distant screen with various path differences depending on the diffraction angle θ\theta, builds up the characteristic diffraction pattern: an intense central maximum together with much weaker secondary maxima, separated by dark fringes. (b) The central maximum spans from θ=−λ/a\theta=-\lambda/a to θ=+λ/a\theta=+\lambda/a, i.e. angular width =2λ/a=2\lambda/a. The first secondary (diffraction) fringe lies between the first minimum (θ=λ/a\theta=\lambda/a) and the second minimum (θ=2λ/a\theta=2\lambda/a), giving it an angular width of   2λa−λa=λa\;\dfrac{2\lambda}a-\dfrac\lambda a=\dfrac\lambda a. ∴  \therefore\; angular width of first diffraction fringe (λa)=12×\left(\dfrac\lambda a\right)=\dfrac12\times angular width of central fringe (2λa)\left(\dfrac{2\lambda}a\right) — i.e. exactly HALF. (c) Same reasoning as in Q49 above: at θ=(n+12)λ/a\theta=(n+\tfrac12)\lambda/a, the slit divides into (2n+1)(2n+1) equal parts, of which all but one pair cancel; the uncancelled contributing fraction of the slit shrinks as nn increases, so the intensity of successive maxima keeps falling.

  23. (a) Same explanation and derivation as in Q51 and Q63 above: for nnth secondary minimum,   sin⁡θn=nλa  (n=±1,±2,… )\;\sin\theta_n=\dfrac{n\lambda}a\;(n=\pm1,\pm2,\dots); for nnth secondary maximum,   sin⁡θn=(2n+1)λ2a  (n=±1,±2,… )\;\sin\theta_n=(2n+1)\dfrac\lambda{2a}\;(n=\pm1,\pm2,\dots), both reducing to θn≈\theta_n\approx these expressions for small angles. (b) Position of the first secondary maximum:   x=3λD2a  \;x=\dfrac{3\lambda D}{2a}\; (same formula as Q54 above). For λ1=590\lambda_1=590 nm and λ2=596\lambda_2=596 nm: separation   x2−x1=3D2a(λ2−λ1)=3×1.52×2×10−6×(596−590)×10−9\;x_2-x_1=\dfrac{3D}{2a}(\lambda_2-\lambda_1)=\dfrac{3\times1.5}{2\times2\times10^{-6}}\times(596-590)\times10^{-9} =4.54×10−6×6×10−9=27×10−94×10−6=6.75×10−3 m=6.75 mm=\dfrac{4.5}{4\times10^{-6}}\times6\times10^{-9}=\dfrac{27\times10^{-9}}{4\times10^{-6}}=6.75\times10^{-3}\text{ m}=6.75\text{ mm}

  24. (a) Same three features as in Q61 above: (1) interference fringes are all equally bright, diffraction maxima decrease sharply in intensity away from the centre; (2) interference fringes are all of equal width, while the central diffraction maximum is twice as wide as the secondary maxima; (3) interference produces a wide field of comparably bright fringes, while diffraction concentrates most of the light into a single dominant central band. (b) Same numerical setup as Q57(i) above:   a=λDymin=5×10−7×12.5×10−3=2×10−4 m=0.2 mm\;a=\dfrac{\lambda D}{y_{min}}=\dfrac{5\times10^{-7}\times1}{2.5\times10^{-3}}=2\times10^{-4}\text{ m}=0.2\text{ mm}