How unit 2 is examined
This unit covers interference (superposition, Young, Newton's rings, Michelson, Mach-Zehnder) and diffraction (single slit, Rayleigh criterion, grating); Newton's rings and superposition carry the most marks.
Huygens' principle
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Definition. <mark>Every point on a wavefront acts as a source of secondary wavelets, and the new wavefront after time $t$ is the forward envelope of these wavelets.</mark>
Key points.
- A wavefront is the locus of points vibrating in the same phase.
- Each secondary wavelet spreads with the speed of the wave, so its radius after time $t$ is $vt$.
- The tangent drawn to the wavelets in the forward direction gives the new wavefront.
- The principle explains reflection, refraction, interference and diffraction, and it ignores the backward wave.
Superposition of waves and interference by wavefront and amplitude splitting
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Definition. ==Superposition principle: when two or more waves overlap in a medium, the resultant displacement is the algebraic sum of the individual displacements, $y = y_1 + y_2 + \dots + y_n$.== It holds for linear media. Interference is the redistribution of light energy when two coherent waves superpose, giving maxima and minima of intensity.
Formula. For $y_1 = a_1\sin\omega t$ and $y_2 = a_2\sin(\omega t + \phi)$:
$$y = R\sin(\omega t + \theta),\quad R^2 = a_1^2 + a_2^2 + 2a_1a_2\cos\phi,\quad I \propto R^2$$
Key points.
- Constructive interference occurs when $\phi = 2n\pi$, i.e. path difference $\Delta = n\lambda$, giving $R_{max} = a_1 + a_2$ and $I_{max} \propto (a_1+a_2)^2$.
- Destructive interference occurs when $\phi = (2n+1)\pi$, i.e. $\Delta = (2n+1)\lambda/2$, giving $R_{min} = |a_1 - a_2|$ and $I_{min} \propto (a_1-a_2)^2$.
- Sustained fringes need coherent sources: the same frequency and a constant phase difference, so they are obtained from one source.
- In wavefront splitting, a point source or slit is divided into two parts of the same wavefront, as in Young's slits and the Fresnel biprism.
- In amplitude splitting, one beam is divided by partial reflection and transmission into two beams of lower amplitude, as in thin films, Newton's rings and the Michelson interferometer.
- Energy is conserved in interference: it is redistributed from minima to maxima, not destroyed.
- Superposition also underlies diffraction, beats and standing waves.
| Wavefront splitting | Amplitude splitting |
|---|---|
| Wavefront is divided into two parts | Amplitude of one beam is divided |
| Needs a point or narrow slit source | Extended source can be used |
| Fringes are faint because the source is small | Fringes are bright |
| Coherence comes from the same wavefront | Coherence comes from partial reflection |
| Fringes are usually straight, equally spaced | Fringes are circular or localised |
| Examples: Young, biprism | Examples: Newton's rings, Michelson |
Answer frame. Open with the superposition principle and $y=y_1+y_2$; draw two waves and the resultant; derive $R$ then the two conditions in phase and path difference; for the difference question give the 6-row table with examples; close with "energy is redistributed, not lost".
Asked: [7 marks] (Jun 2022) What is superposition of waves? Explain constructive and destructive interference. Asked: [5 marks] (Dec 2023) Differentiate between division of amplitude and division of wavefront. Asked: [5 marks] (Dec 2023) Define superposition of waves. Asked: [7 marks] (Jun 2025) What is superposition of wave and interference of light by amplitude splitting?
Young's double slit experiment
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Definition. <mark>Light from a narrow slit $S$ falls on two close slits $S_1, S_2$ (separation $d$), which act as coherent sources and give alternate bright and dark fringes on a screen at distance $D$.</mark>
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Formula. Path difference at $P$: $\Delta = S_2P - S_1P = \dfrac{yd}{D}$.
$$\text{Bright: } y_n = \frac{n\lambda D}{d},\qquad \text{Dark: } y_n = \frac{(2n-1)\lambda D}{2d},\qquad \beta = \frac{\lambda D}{d}$$
Key points.
- Bright fringes need $\Delta = n\lambda$ and dark fringes need $\Delta = (2n-1)\lambda/2$.
- All fringes have the same width $\beta = \lambda D/d$, so they are equally spaced, straight and parallel to the slits.
- Fringe width grows with $\lambda$ and $D$ and falls with $d$; white light gives a white centre with coloured edges.
- The experiment proved the wave nature of light and gave a way to measure $\lambda$.
Answer frame. Open with the definition of interference and the need for coherent sources; draw the labelled figure; derive $\Delta = yd/D$ using $S_1P^2$ and $S_2P^2$ (so $S_2P^2 - S_1P^2 = 2yd$ and $S_1P + S_2P \approx 2D$); write maxima, minima, then $\beta$; close with significance.
Asked: [7 marks] (Dec 2023, Jun 2023) Discuss Young's double slit experiment on the basis of labelled diagram, formula used and significance; What is interference of light? Describe Young's experiment and derive the expression of fringe width.
Newton's rings
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Definition. <mark>Newton's rings are concentric circular interference fringes formed in the wedge-shaped air film between a plano-convex lens of large radius of curvature $R$ and a plane glass plate, seen in reflected light.</mark>
<figure class="ds-fig" style="margin:1.4rem 0;overflow-x:auto"><svg xmlns="http://www.w3.org/2000/svg" id="dsfig-u2-02" viewBox="0 0 424 252" width="424" height="252" role="img" aria-label="Newton's rings setup: Src monochromatic source, M glass plate at 45 degrees, L plano-convex lens on plane plate Gp, Mic microscope"><style>#dsfig-u2-02 .e{stroke:#454C5A;stroke-width:1.4;fill:none}#dsfig-u2-02 .e.hi{stroke:#2340B8;stroke-width:2.6}#dsfig-u2-02 .n{fill:#FFFFFF;stroke:#16181D;stroke-width:1.4}#dsfig-u2-02 .n.hi{fill:#E3E9FC;stroke:#2340B8;stroke-width:2.2}#dsfig-u2-02 .n.rb-b{fill:#16181D;stroke:#16181D}#dsfig-u2-02 .n.rb-r{fill:#BD3227;stroke:#BD3227}#dsfig-u2-02 text{font-family:"JetBrains Mono",ui-monospace,Menlo,Consolas,monospace;font-size:13px}#dsfig-u2-02 .t{fill:#16181D;font-weight:500}#dsfig-u2-02 .t.inv{fill:#FFFFFF;font-weight:700}#dsfig-u2-02 .kd{stroke:#16181D;stroke-width:1.2}#dsfig-u2-02 .dot{fill:#16181D}#dsfig-u2-02 .ann{fill:#2340B8;font-size:11px;font-weight:700}#dsfig-u2-02 .lbl{fill:#6F7787;font-family:system-ui,-apple-system,sans-serif;font-size:12px;font-weight:700}#dsfig-u2-02 .ptr{fill:#2340B8;font-size:12px;font-weight:700}#dsfig-u2-02 .ah{fill:#454C5A}#dsfig-u2-02 .ah.hi{fill:#2340B8}#dsfig-u2-02 .wl rect{fill:#FFFFFF;stroke:#DCE0E7}#dsfig-u2-02 .wl .t{font-size:12px;font-weight:700}#dsfig-u2-02 .wl.hi rect{fill:#2340B8;stroke:#2340B8}#dsfig-u2-02 .wl.hi .t{fill:#FFFFFF}html.dark #dsfig-u2-02 .e{stroke:#B1B7C3}html.dark #dsfig-u2-02 .e.hi{stroke:#8FA3FF}html.dark #dsfig-u2-02 .n{fill:#161920;stroke:#E6E8ED}html.dark #dsfig-u2-02 .n.hi{fill:#1E2748;stroke:#8FA3FF}html.dark #dsfig-u2-02 .n.rb-b{fill:#E6E8ED;stroke:#E6E8ED}html.dark #dsfig-u2-02 .n.rb-r{fill:#FF7E71;stroke:#FF7E71}html.dark #dsfig-u2-02 .t{fill:#E6E8ED}html.dark #dsfig-u2-02 .t.inv{fill:#0F1115}html.dark #dsfig-u2-02 .kd{stroke:#E6E8ED}html.dark #dsfig-u2-02 .dot{fill:#E6E8ED}html.dark #dsfig-u2-02 .ann{fill:#8FA3FF}html.dark #dsfig-u2-02 .lbl{fill:#858D9C}html.dark #dsfig-u2-02 .ptr{fill:#8FA3FF}html.dark #dsfig-u2-02 .ah{fill:#B1B7C3}html.dark #dsfig-u2-02 .ah.hi{fill:#8FA3FF}html.dark #dsfig-u2-02 .wl rect{fill:#161920;stroke:#2A2E37}html.dark #dsfig-u2-02 .wl.hi rect{fill:#8FA3FF;stroke:#8FA3FF}html.dark #dsfig-u2-02 .wl.hi .t{fill:#0F1115}</style><defs><marker id="ah2" viewBox="0 0 10 10" refX="9" refY="5" markerWidth="7" markerHeight="7" orient="auto-start-reverse"><path class="ah" d="M0,1 L9,5 L0,9 z"/></marker><marker id="ahh2" viewBox="0 0 10 10" refX="9" refY="5" markerWidth="7" markerHeight="7" orient="auto-start-reverse"><path class="ah hi" d="M0,1 L9,5 L0,9 z"/></marker></defs><path class="e" d="M40,59 L40,107"/><path class="e" d="M365.6,44.6 L232.4,77.9" marker-end="url(#ah2)"/><path class="e" d="M193.6,87.6 L60.4,120.9" marker-end="url(#ah2)"/><path class="e" d="M40,145 L40,191" marker-end="url(#ah2)"/><g class="wl"><rect x="-11.9" y="74" width="103.8" height="18" rx="9"/><text class="t" x="40" y="83" dy=".35em" text-anchor="middle">lens_on_plate</text></g><circle class="n" cx="40" cy="40" r="18"/><text class="t" x="40" y="40" dy=".35em" text-anchor="middle">L</text><circle class="n" cx="40" cy="126" r="18"/><text class="t" x="40" y="126" dy=".35em" text-anchor="middle">Gp</text><circle class="n" cx="212" cy="83" r="18"/><text class="t" x="212" y="83" dy=".35em" text-anchor="middle">M</text><circle class="n" cx="384" cy="40" r="18"/><text class="t" x="384" y="40" dy=".35em" text-anchor="middle">Src</text><circle class="n" cx="40" cy="212" r="18"/><text class="t" x="40" y="212" dy=".35em" text-anchor="middle">Mic</text></svg><figcaption style="font-size:.82em;opacity:.72;margin-top:.45rem">Newton's rings setup: Src monochromatic source, M glass plate at 45 degrees, L plano-convex lens on plane plate Gp, Mic microscope</figcaption></figure>
Formation. Light from the source is reflected by the plate at $45^\circ$ down onto the lens. Rays reflected from the top and bottom surfaces of the air film interfere. The film thickness is constant on a circle about the contact point, so the fringes are circles; the centre is dark because of the $\pi$ phase change on reflection at the plate.
Derivation. For a ring of radius $r$ at film thickness $t$: $r^2 = 2Rt - t^2 \approx 2Rt$, so $t = r^2/2R$. In reflected light (normal incidence) the condition is $2t = n\lambda$ for dark and $2t = (2n-1)\lambda/2$ for bright. Hence $r_n^2 = n\lambda R$, so for dark rings $D_n^2 = 4n\lambda R$, and for bright rings $D_n^2 = 2(2n-1)\lambda R$. Between ring $n$ and $n+p$:
$$\lambda = \frac{D_{n+p}^2 - D_n^2}{4pR}$$
Key points.
- Dark ring diameter is proportional to $\sqrt n$, so the rings crowd together outward.
- The centre is dark because of the $\pi$ phase change at the glass surface.
- Using $D_{n+p}^2 - D_n^2$ removes the error in locating the centre.
- The refractive index of a liquid is found from $\mu = (D_n^2)_{air}/(D_n^2)_{liquid}$.
Example. Given $D_n = 0.42$ cm, $D_{n+14} = 0.70$ cm, $R = 100$ cm, $p = 14$.
| Step | Working |
|---|---|
| $D_{n+p}^2 - D_n^2$ | $0.49 - 0.1764 = 0.3136\ \text{cm}^2$ |
| $4pR$ | $4 \times 14 \times 100 = 5600$ cm |
| $\lambda$ | $0.3136/5600 = 5.6\times10^{-5}$ cm |
$\lambda = 5600\ \text{\AA}$.
Answer frame. Open with the definition and draw the setup; explain formation by the air film; derive $t = r^2/2R$, then $D_n^2 = 4n\lambda R$, then $\lambda$ using $n$ and $n+p$; close with the dark centre and $\sqrt n$ spacing. For the numerical, write formula, substitute, box the answer.
Asked: [7 marks] (Jun 2022, Nov 2022, Dec 2024) Explain the formation of Newton's rings. Obtain the expression for the wavelength of light; How are Newton's rings formed? Deduce the expression for diameter of dark and bright fringes. Asked: [5 marks] (Dec 2023) In Newton's ring method the diameters of the $n^{th}$ and $(n+14)^{th}$ rings are 0.42 cm and 0.70 cm. If $R$ = 100 cm, calculate the wavelength of light.
Michelson interferometer
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Definition. <mark>Michelson interferometer is an amplitude-splitting instrument in which a beam is divided by a beam splitter into two perpendicular beams that are reflected back by two mirrors and recombined to give interference fringes.</mark>
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Key points.
- Light from an extended source falls on $G_1$, a half-silvered glass plate at $45^\circ$, which splits it into a reflected beam going to $M_2$ and a transmitted beam going to $M_1$.
- Both beams return, recombine at $G_1$ and enter the telescope, where they interfere because they come from the same source.
- $G_2$ has the same thickness as $G_1$ and is placed in the path of the transmitted beam so that both beams pass through equal glass thickness, which makes the path difference independent of wavelength.
- $M_1$ moves on a micrometer screw, so the path difference $2d$ can be varied, where $d$ is the distance between $M_1$ and the image of $M_2$.
- If $M_1$ and $M_2$ are exactly perpendicular the fringes are circular (equal inclination); if slightly tilted the fringes are straight (equal thickness); with white light a few coloured fringes appear at $d = 0$.
- When $M_1$ moves by $\lambda/2$, one fringe crosses the field, so $\lambda = 2x/N$ for a displacement $x$ giving $N$ fringes.
Answer frame. Open with the definition; draw the labelled figure; describe construction, then working, then fringe types; close with the formula $\lambda = 2x/N$.
Asked: [7 marks] (Jun 2022, Dec 2023, Jun 2025) Discuss the construction and working of Michelson interferometer; explain it on the basis of labelled diagram and types of fringes.
Mach-Zehnder interferometer
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Definition. <mark>Mach-Zehnder interferometer is an amplitude-splitting device in which a collimated beam is split by a first beam splitter into two separate paths that are recombined by a second beam splitter.</mark>
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Key points.
- The set-up has a collimated source, two beam splitters $BS_1$ and $BS_2$, two fully reflecting mirrors $M_1$ and $M_2$, and detectors or a screen.
- $BS_1$ divides the beam into a reference arm and a test arm, each of which reflects only once from its mirror.
- The two beams recombine at $BS_2$, and the phase difference between the arms decides whether the output is bright or dark.
- A sample of refractive index $n$ and thickness $t$ placed in one arm adds a path difference $(n-1)t$.
- The two beams travel separate paths, so a sample can be placed in one arm without disturbing the other; this is the main advantage over the Michelson.
- It gives two complementary outputs and is used to measure refractive index changes, in flow visualisation in aerodynamics and in optical modulators.
Answer frame. Open with the definition; draw the schematic with labelled arms; describe construction, then working, then path difference; close with applications.
Asked: [7 marks] (Nov 2022, Jun 2023, Jun 2025) Describe the construction and working of Mach-Zehnder interferometer; explain its working principle with suitable ray diagram.
Fraunhofer diffraction from a single slit and a circular aperture
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Definition. <mark>Fraunhofer diffraction is the bending of light at a slit of width $a$ when the source and screen are at infinite distance, using parallel incident and diffracted beams.</mark>
Key points.
- Wavelets from the two edges have path difference $a\sin\theta$, so the phase difference is $2\beta = \dfrac{2\pi}{\lambda}a\sin\theta$ with $\beta = \dfrac{\pi a\sin\theta}{\lambda}$.
- Adding the wavelet contributions by integration or vector polygon gives amplitude $R = A\dfrac{\sin\beta}{\beta}$, so the intensity is $I = I_0\left(\dfrac{\sin\beta}{\beta}\right)^2$.
- The central maximum is at $\theta = 0$ where $I = I_0$; minima occur at $a\sin\theta = \pm m\lambda$ ($m = 1, 2, \dots$).
- Secondary maxima lie near $\beta = \pm\dfrac{3\pi}{2}, \pm\dfrac{5\pi}{2}$ and have intensities about $4.5\%$ and $1.6\%$ of $I_0$.
- For a circular aperture of diameter $D$ the first minimum is at $\sin\theta = 1.22\lambda/D$.
Asked: [7 marks] (Dec 2024) Explain the Fraunhofer diffraction due to single slit with necessary analysis.
Rayleigh criterion and its application to vision
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Definition. <mark>Rayleigh criterion: two point objects or spectral lines are just resolved when the central maximum of the diffraction pattern of one falls on the first minimum of the pattern of the other.</mark>
| Condition | Position of peaks | Intensity at middle |
|---|---|---|
| Well resolved | Peaks far apart | Deep dip, clear separation |
| Just resolved (Rayleigh) | Peak of one on first minimum of other | About $0.81$ of the peak, a dip of about $19\%$ |
| Unresolved | Peaks closer than Rayleigh limit | No dip, they appear as one |
Key points.
- Every image is a diffraction pattern, so two close objects give overlapping patterns.
- In the just-resolved case the resultant intensity at the mid-point is about $81\%$ of either maximum, and the eye can detect this dip.
- For a circular aperture of diameter $D$, the smallest resolvable angle is $\theta_{min} = 1.22\lambda/D$.
- A larger aperture or a shorter wavelength gives better resolution; this is why telescopes are large and electron microscopes resolve finely.
- For the human eye, with pupil $D \approx 2$ mm and $\lambda = 550$ nm, $\theta_{min} \approx 3.4\times10^{-4}$ rad, about $1'$ of arc.
- For a grating the criterion fixes the resolving power $\lambda/d\lambda$.
Answer frame. Open with the statement of the criterion; draw the three intensity curves (well resolved, just resolved, unresolved) with the dip marked; then the $0.81$ point and $1.22\lambda/D$; close with the application to the eye and instruments.
Asked: [7 marks] (Dec 2023, Jun 2025) Explain the Rayleigh's criteria for resolving power; what is the importance of the Rayleigh criteria; explain the Rayleigh criterion for limit of resolution.
Diffraction gratings and their resolving power
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Definition. <mark>A diffraction grating is an optical component with a large number of equally spaced parallel slits ($a$ transparent, $b$ opaque) that splits light into spectra of different orders.</mark> The grating element is $a + b = 1/N'$, where $N'$ is the number of lines per unit length.
Formula. Grating equation: $(a+b)\sin\theta = n\lambda$ for the $n^{th}$ principal maximum.
Resolving power derivation. Resolving power is $\lambda/d\lambda$, where $\lambda$ and $\lambda + d\lambda$ are two lines just resolved. The $n^{th}$ maximum of $\lambda + d\lambda$ is at angle $\theta$: $(a+b)\sin\theta = n(\lambda + d\lambda)$. By the Rayleigh criterion, this must fall on the first minimum next to the $n^{th}$ maximum of $\lambda$, which for $N$ lines is at $(a+b)\sin\theta = \left(n + \dfrac{1}{N}\right)\lambda$. Equating, $n\,d\lambda = \lambda/N$, so
$$\frac{\lambda}{d\lambda} = nN$$
Key points.
- The resolving power is proportional to the order $n$ and to the total number of lines $N$ illuminated.
- A wider grating with more lines resolves closer lines, and higher orders resolve better but are fainter.
- Resolving power does not depend directly on the grating element.
Example. $N' = 4250$ lines/cm, $n = 2$, $\theta = 30^\circ$.
| Step | Working |
|---|---|
| $a+b$ | $1/4250\ \text{cm} = 2.353\times10^{-6}$ m |
| $\lambda$ | $(2.353\times10^{-6}\times0.5)/2 = 5.88\times10^{-7}$ m |
$\lambda = 588\ \text{nm}$ ($5882\ \text{\AA}$).
Answer frame. Open with the definition and grating equation; state the Rayleigh criterion; derive $\lambda/d\lambda = nN$ using the $(n+1/N)$ minimum; add the factors (order and lines); for the numerical, write $a+b$ from $N'$, substitute and box.
Asked: [7 marks] (Nov 2022) Explain about the diffraction grating. A parallel beam of sodium light is incident on a plane transmission grating with 4250 lines per cm and a second-order line is seen at $30^\circ$. Find the wavelength. Asked: [7 marks] (Jun 2023) Explain Rayleigh's criterion of resolution. Derive an expression for the resolving power of a grating.
Last-minute revision
- Superposition: $y = y_1 + y_2$; $R^2 = a_1^2 + a_2^2 + 2a_1a_2\cos\phi$.
- Constructive: $\Delta = n\lambda$ ($\phi = 2n\pi$); destructive: $\Delta = (2n+1)\lambda/2$.
- Wavefront splitting: Young, biprism; amplitude splitting: Newton's rings, thin films, Michelson.
- Young: $\Delta = yd/D$, $\beta = \lambda D/d$.
- Newton's rings: $D_n^2 = 4n\lambda R$ (dark), $\lambda = (D_{n+p}^2 - D_n^2)/4pR$; centre dark.
- Newton's numerical answer: $5600$ \AA (0.42, 0.70 cm, $p=14$, $R=100$ cm).
- Michelson: division of amplitude, compensating plate $G_2$, $\lambda = 2x/N$.
- Mach-Zehnder: two beam splitters, two mirrors, separate arms, sample adds $(n-1)t$.
- Single slit: $I = I_0(\sin\beta/\beta)^2$, minima $a\sin\theta = m\lambda$.
- Rayleigh: peak on first minimum, dip $0.81$; $\theta_{min} = 1.22\lambda/D$.
- Grating: $(a+b)\sin\theta = n\lambda$; $\lambda/d\lambda = nN$; sodium answer $588$ nm.
Memory hooks
- Wavefront splitting = Young; Amplitude splitting = Newton and Michelson (thin films, "A for Aggregate of reflections").
- "Dark centre, root-n rings": Newton's rings have a dark centre and diameter $\propto \sqrt n$.
- Michelson has one compensating plate, Mach-Zehnder has two beam splitters and separate arms.
- Rayleigh: "peak on trough", the dip is 81%.
- Grating power: order times lines, $nN$.
Coverage checklist
- Huygens' principle: definition, secondary wavelets, envelope (no past question).
- superposition of waves and interference of light by wave front splitting and amplitude splitting: covers Jun 2022 superposition, Dec 2023 difference, Dec 2023 definition, Jun 2025 amplitude splitting.
- Young's double slit experiment: covers Jun 2023 and Dec 2023.
- Newton's rings: covers Jun 2022, Nov 2022, Dec 2024 derivation and Dec 2023 numerical.
- Michelson interferometer: covers Jun 2022, Dec 2023, Jun 2025.
- Mach-Zehnder interferometer: covers Nov 2022, Jun 2023, Jun 2025.
- Farunhofer diffraction from a single slit and a circular aperture: covers Dec 2024.
- the Rayleigh criterion for limit of resolution and its application to vision: covers Dec 2023 and Jun 2025.
- Diffraction gratings and their resolving power: covers Nov 2022 and Jun 2023.