Narrow Slit
After a narrow slit, light spreads into the geometrical-shadow region.
Wave Optics · Chapter 04
Understand single-slit spreading, minima, secondary maxima, central width and resolution through exam-ready derivations and textbook-style diagrams.
Diffraction is the bending and spreading of light when it passes through a narrow aperture or around an obstacle. It becomes clearly observable when the aperture size is comparable with the wavelength.
a ≈ λ → significant diffractionAfter a narrow slit, light spreads into the geometrical-shadow region.
Sound wavelengths are comparable with doors and walls, so sound bends readily.
Visible wavelengths are tiny compared with everyday openings, so spreading is normally small.
Diffraction shows the limitation of straight-line ray optics and directly supports the wave nature of light.
Every point within the open slit emits a secondary wavelet. At a distant point, these wavelets arrive with different phases; their interference produces the observed maxima and minima.
| Feature | Fresnel Diffraction | Fraunhofer Diffraction |
|---|---|---|
| Source and screen | Finite distances | Effectively infinite distances or focal planes |
| Wavefront | Spherical/curved | Plane incident wavefront |
| Lenses | Not essential | Usually used for collimation and focusing |
| Pattern | Changes with distance | Stable angular pattern |
| Application | Near-field edge patterns | Single slit, gratings, spectroscopy |
Consider a slit AB of width a illuminated by a plane monochromatic wave.
For rays leaving A and B at angle θ, the extreme path difference is Δ = a sinθ.
The resultant amplitude is the vector sum of contributions from all elemental strips.
At θ = 0 all contributions are in phase, giving the principal maximum.
First minimum: a sinθ = λ. Divide the slit into two halves; corresponding points differ by λ/2 and cancel pairwise.
Second minimum: a sinθ = 2λ. Divide the slit into four equal parts; adjacent paired contributions again differ by λ/2.
In general, complete cancellation occurs for a sinθ = nλ, n = 1,2,3,...
For the first secondary maximum, a sinθ ≈ 3λ/2.
Divide the aperture into three parts. Two parts cancel approximately and one part remains.
Similarly the next weak maximum occurs near a sinθ ≈ 5λ/2.
The simple exam-level approximate condition is a sinθ = (2n+1)λ/2.
This odd-half-wave condition is an approximation. Exact secondary maxima satisfy tanα = α, where α = πa sinθ/λ.
The first minima lie at a sinθ = ±λ.
For small angles, θ ≈ λ/a.
The central maximum extends from −θ to +θ, so angular width = 2θ = 2λ/a.
At screen distance D, half-width y₁ = Dλ/a.
Therefore linear width β₀ = 2y₁ = 2Dλ/a.
| Change | Effect |
|---|---|
| Increase λ | Central maximum widens |
| Increase D | Linear width increases |
| Decrease a | Central maximum widens |
Example: If D doubles while λ and a remain fixed, β₀ doubles.
Minimum angular separation θmin = 1.22λ/d for a circular aperture. Larger objective diameter improves resolution.
Limit of resolution is approximately 0.61λ/(μ sinα). Shorter wavelength and larger numerical aperture improve detail.
The finite pupil causes diffraction; a typical angular resolution is of order one arcminute under good conditions.
Resolving power is the ability to distinguish nearby objects or spectral features as separate.
Two sources are just resolved when the central maximum of either diffraction image falls at the first minimum of the other. Smaller separation gives strongly overlapping images; larger separation gives clearly distinct peaks.
Closely spaced tracks act like a diffraction grating and separate colors.
Aperture diffraction fixes the ultimate image sharpness.
Gratings separate wavelengths for precise spectral analysis.
Crystal planes diffract X-rays and reveal atomic structure.
Diffraction limits angular resolution of stars and planets.
Aperture size and wavelength set the smallest resolvable detail.
For slit width a = 0.2 mm and λ = 400 nm, find the small angle of first minimum.
Answer: 2.000e-3 rad
Solution: a sinθ = λ. For small θ, θ = λ/a = 2.000e-3 rad.
Find β₀ for D = 1.5 m, λ = 550 nm and a = 0.5 mm.
Answer: 3.300 mm
Solution: β₀ = 2Dλ/a = 3.300 mm.
Write the path condition for the 3rd minimum.
Answer: a sinθ = 3λ
Solution: The general minimum condition is a sinθ = nλ; substituting n = 3 gives the result.
State the approximate condition for secondary maximum number 1.
Answer: a sinθ = 3λ/2
Solution: Using the conceptual odd-half-wave condition a sinθ = (2n+1)λ/2 gives 3λ/2.
For D = 1.5 m, λ = 600 nm and a = 0.3 mm, find the distance of first minimum from center.
Answer: 3.000 mm
Solution: y₁ = Dλ/a = 3.000 mm; central width is twice this value.
If wavelength is multiplied by 1.25, what happens to central width?
Answer: It becomes 1.25 times
Solution: β₀ = 2Dλ/a, so central width changes in direct proportion to λ.
For slit width a = 0.3 mm and λ = 400 nm, find the small angle of first minimum.
Answer: 1.333e-3 rad
Solution: a sinθ = λ. For small θ, θ = λ/a = 1.333e-3 rad.
Find β₀ for D = 2.5 m, λ = 650 nm and a = 0.5 mm.
Answer: 6.500 mm
Solution: β₀ = 2Dλ/a = 6.500 mm.
Write the path condition for the 1st minimum.
Answer: a sinθ = 1λ
Solution: The general minimum condition is a sinθ = nλ; substituting n = 1 gives the result.
State the approximate condition for secondary maximum number 1.
Answer: a sinθ = 3λ/2
Solution: Using the conceptual odd-half-wave condition a sinθ = (2n+1)λ/2 gives 3λ/2.
For D = 1.5 m, λ = 600 nm and a = 0.3 mm, find the distance of first minimum from center.
Answer: 3.000 mm
Solution: y₁ = Dλ/a = 3.000 mm; central width is twice this value.
If wavelength is multiplied by 1.75, what happens to central width?
Answer: It becomes 1.75 times
Solution: β₀ = 2Dλ/a, so central width changes in direct proportion to λ.
For slit width a = 0.4 mm and λ = 400 nm, find the small angle of first minimum.
Answer: 1.000e-3 rad
Solution: a sinθ = λ. For small θ, θ = λ/a = 1.000e-3 rad.
Find β₀ for D = 1.5 m, λ = 550 nm and a = 0.5 mm.
Answer: 3.300 mm
Solution: β₀ = 2Dλ/a = 3.300 mm.
Write the path condition for the 3rd minimum.
Answer: a sinθ = 3λ
Solution: The general minimum condition is a sinθ = nλ; substituting n = 3 gives the result.
State the approximate condition for secondary maximum number 1.
Answer: a sinθ = 3λ/2
Solution: Using the conceptual odd-half-wave condition a sinθ = (2n+1)λ/2 gives 3λ/2.
For D = 1.5 m, λ = 600 nm and a = 0.3 mm, find the distance of first minimum from center.
Answer: 3.000 mm
Solution: y₁ = Dλ/a = 3.000 mm; central width is twice this value.
If wavelength is multiplied by 1.25, what happens to central width?
Answer: It becomes 1.25 times
Solution: β₀ = 2Dλ/a, so central width changes in direct proportion to λ.
For slit width a = 0.5 mm and λ = 400 nm, find the small angle of first minimum.
Answer: 8.000e-4 rad
Solution: a sinθ = λ. For small θ, θ = λ/a = 8.000e-4 rad.
Find β₀ for D = 2.5 m, λ = 650 nm and a = 0.5 mm.
Answer: 6.500 mm
Solution: β₀ = 2Dλ/a = 6.500 mm.
Write the path condition for the 1st minimum.
Answer: a sinθ = 1λ
Solution: The general minimum condition is a sinθ = nλ; substituting n = 1 gives the result.
State the approximate condition for secondary maximum number 1.
Answer: a sinθ = 3λ/2
Solution: Using the conceptual odd-half-wave condition a sinθ = (2n+1)λ/2 gives 3λ/2.
For D = 1.5 m, λ = 600 nm and a = 0.3 mm, find the distance of first minimum from center.
Answer: 3.000 mm
Solution: y₁ = Dλ/a = 3.000 mm; central width is twice this value.
If wavelength is multiplied by 1.75, what happens to central width?
Answer: It becomes 1.75 times
Solution: β₀ = 2Dλ/a, so central width changes in direct proportion to λ.
For slit width a = 0.6 mm and λ = 400 nm, find the small angle of first minimum.
Answer: 6.667e-4 rad
Solution: a sinθ = λ. For small θ, θ = λ/a = 6.667e-4 rad.
Find β₀ for D = 1.5 m, λ = 550 nm and a = 0.5 mm.
Answer: 3.300 mm
Solution: β₀ = 2Dλ/a = 3.300 mm.
Write the path condition for the 3rd minimum.
Answer: a sinθ = 3λ
Solution: The general minimum condition is a sinθ = nλ; substituting n = 3 gives the result.
State the approximate condition for secondary maximum number 1.
Answer: a sinθ = 3λ/2
Solution: Using the conceptual odd-half-wave condition a sinθ = (2n+1)λ/2 gives 3λ/2.
For D = 1.5 m, λ = 600 nm and a = 0.3 mm, find the distance of first minimum from center.
Answer: 3.000 mm
Solution: y₁ = Dλ/a = 3.000 mm; central width is twice this value.
If wavelength is multiplied by 1.25, what happens to central width?
Answer: It becomes 1.25 times
Solution: β₀ = 2Dλ/a, so central width changes in direct proportion to λ.
Academic note: These are original CBSE, NEET, JEE, IB, IGCSE and A-Level exam-style questions, not verbatim copyrighted papers.
A. a ≈ λ
B. frequency changes
C. central maximum is narrowest
D. diffraction requires a ≫ λ
A. frequency changes
B. central maximum is narrowest
C. diffraction requires a ≫ λ
D. Δ = a sinθ
A. central maximum is narrowest
B. diffraction requires a ≫ λ
C. a sinθ = nλ
D. frequency changes
A. diffraction requires a ≫ λ
B. a sinθ = (2n+1)λ/2
C. frequency changes
D. central maximum is narrowest
A. 2λ/a
B. frequency changes
C. central maximum is narrowest
D. diffraction requires a ≫ λ
A. frequency changes
B. central maximum is narrowest
C. diffraction requires a ≫ λ
D. 2Dλ/a
A. central maximum is narrowest
B. diffraction requires a ≫ λ
C. sinθ = λ/a
D. frequency changes
A. diffraction requires a ≫ λ
B. brightest and widest
C. frequency changes
D. central maximum is narrowest
A. parallel
B. frequency changes
C. central maximum is narrowest
D. diffraction requires a ≫ λ
A. frequency changes
B. central maximum is narrowest
C. diffraction requires a ≫ λ
D. central maximum coincides with first minimum
A. central maximum is narrowest
B. diffraction requires a ≫ λ
C. a ≈ λ
D. frequency changes
A. diffraction requires a ≫ λ
B. Δ = a sinθ
C. frequency changes
D. central maximum is narrowest
A. a sinθ = nλ
B. frequency changes
C. central maximum is narrowest
D. diffraction requires a ≫ λ
A. frequency changes
B. central maximum is narrowest
C. diffraction requires a ≫ λ
D. a sinθ = (2n+1)λ/2
A. central maximum is narrowest
B. diffraction requires a ≫ λ
C. 2λ/a
D. frequency changes
A. diffraction requires a ≫ λ
B. 2Dλ/a
C. frequency changes
D. central maximum is narrowest
A. sinθ = λ/a
B. frequency changes
C. central maximum is narrowest
D. diffraction requires a ≫ λ
A. frequency changes
B. central maximum is narrowest
C. diffraction requires a ≫ λ
D. brightest and widest
A. central maximum is narrowest
B. diffraction requires a ≫ λ
C. parallel
D. frequency changes
A. diffraction requires a ≫ λ
B. central maximum coincides with first minimum
C. frequency changes
D. central maximum is narrowest
A. a ≈ λ
B. frequency changes
C. central maximum is narrowest
D. diffraction requires a ≫ λ
A. frequency changes
B. central maximum is narrowest
C. diffraction requires a ≫ λ
D. Δ = a sinθ
A. central maximum is narrowest
B. diffraction requires a ≫ λ
C. a sinθ = nλ
D. frequency changes
A. diffraction requires a ≫ λ
B. a sinθ = (2n+1)λ/2
C. frequency changes
D. central maximum is narrowest
A. 2λ/a
B. frequency changes
C. central maximum is narrowest
D. diffraction requires a ≫ λ
A. frequency changes
B. central maximum is narrowest
C. diffraction requires a ≫ λ
D. 2Dλ/a
A. central maximum is narrowest
B. diffraction requires a ≫ λ
C. sinθ = λ/a
D. frequency changes
A. diffraction requires a ≫ λ
B. brightest and widest
C. frequency changes
D. central maximum is narrowest
A. parallel
B. frequency changes
C. central maximum is narrowest
D. diffraction requires a ≫ λ
A. frequency changes
B. central maximum is narrowest
C. diffraction requires a ≫ λ
D. central maximum coincides with first minimum
A. central maximum is narrowest
B. diffraction requires a ≫ λ
C. a ≈ λ
D. frequency changes
A. diffraction requires a ≫ λ
B. Δ = a sinθ
C. frequency changes
D. central maximum is narrowest
A. a sinθ = nλ
B. frequency changes
C. central maximum is narrowest
D. diffraction requires a ≫ λ
A. frequency changes
B. central maximum is narrowest
C. diffraction requires a ≫ λ
D. a sinθ = (2n+1)λ/2
A. central maximum is narrowest
B. diffraction requires a ≫ λ
C. 2λ/a
D. frequency changes
A. diffraction requires a ≫ λ
B. 2Dλ/a
C. frequency changes
D. central maximum is narrowest
A. sinθ = λ/a
B. frequency changes
C. central maximum is narrowest
D. diffraction requires a ≫ λ
A. frequency changes
B. central maximum is narrowest
C. diffraction requires a ≫ λ
D. brightest and widest
A. central maximum is narrowest
B. diffraction requires a ≫ λ
C. parallel
D. frequency changes
A. diffraction requires a ≫ λ
B. central maximum coincides with first minimum
C. frequency changes
D. central maximum is narrowest
A. a ≈ λ
B. frequency changes
C. central maximum is narrowest
D. diffraction requires a ≫ λ
A. frequency changes
B. central maximum is narrowest
C. diffraction requires a ≫ λ
D. Δ = a sinθ
A. central maximum is narrowest
B. diffraction requires a ≫ λ
C. a sinθ = nλ
D. frequency changes
A. diffraction requires a ≫ λ
B. a sinθ = (2n+1)λ/2
C. frequency changes
D. central maximum is narrowest
A. 2λ/a
B. frequency changes
C. central maximum is narrowest
D. diffraction requires a ≫ λ
A. frequency changes
B. central maximum is narrowest
C. diffraction requires a ≫ λ
D. 2Dλ/a
A. central maximum is narrowest
B. diffraction requires a ≫ λ
C. sinθ = λ/a
D. frequency changes
A. diffraction requires a ≫ λ
B. brightest and widest
C. frequency changes
D. central maximum is narrowest
A. parallel
B. frequency changes
C. central maximum is narrowest
D. diffraction requires a ≫ λ
A. frequency changes
B. central maximum is narrowest
C. diffraction requires a ≫ λ
D. central maximum coincides with first minimum
a ≈ λ → diffraction is prominent
It is both widest and brightest.
a sinθ = nλ
β₀ = 2Dλ/a
Diffraction cannot be explained by ray optics alone.
Minima and central-width numericals are frequent in NEET/JEE.