Edexcel A Level (IAL) Physics-2.18 - 2.19 Diffraction and Diffraction Grating Equation- Study Notes- New Syllabus
Edexcel A Level (IAL) Physics -2.18 – 2.19 Diffraction and Diffraction Grating Equation- Study Notes- New syllabus
Edexcel A Level (IAL) Physics -2.18 – 2.19 Diffraction and Diffraction Grating Equation- Study Notes -Edexcel A level Physics – per latest Syllabus.
Key Concepts:
Diffraction and Huygens’ Construction
Diffraction is the spreading of waves when they pass through a gap or move around an obstacle. It is a fundamental wave phenomenon that occurs with all types of waves — water waves, sound waves, light waves, and even matter waves.
What Is Diffraction?
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- When a wave passes through a slit or past the edge of an object, it spreads out.
- Diffraction is most noticeable when the size of the slit or obstacle is comparable to the wavelength.
- Light diffracts very little through large slits because its wavelength is extremely small.
Key idea: Greater spreading occurs when slit width ≈ wavelength.
Huygens’ Construction (Huygens’ Principle)
Huygens’ principle states:
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- Every point on a wavefront acts as a source of secondary spherical wavelets.
- The new wavefront is the surface tangent to all these secondary wavelets.
This helps explain how waves change direction when encountering a boundary.
Using Huygens’ Principle to Explain Diffraction
(a) Wave Meets a Slit
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- Each point across the slit acts as a source of secondary wavelets.
- These wavelets spread out in all forward directions.
- The overlapping of these wavelets forms a curved wavefront after the slit.
- For a narrow slit (width ≈ wavelength), the wavefront becomes almost circular → strong diffraction.
(b) Wave Meets an Obstacle
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- The wavefront hits the obstacle and is blocked except at the edges.
- Edges behave like point sources of new wavelets.
- These edge-originating wavelets spread into the shadow region.
Conclusion: Diffraction occurs because edge points behave as new sources of waves.
Factors Affecting Diffraction
- Wavelength:
- Longer wavelength → more diffraction.
- Sound (large wavelength) diffracts well; light (small wavelength) diffracts poorly.
- Slit Width:
- Wide slit ≫ wavelength → very little diffraction.
- Narrow slit ≈ wavelength → strong spreading.
- Obstacle Size:
- Large obstacle → small edge diffraction.
- Obstacle size ≈ wavelength → noticeable bending.
Importance of Diffraction
- Essential for understanding interference patterns.
- Used in diffraction gratings and spectroscopy.
- Explains why sound can be heard around corners.
- Explains resolution limits of microscopes and telescopes.
Example (Easy)
Why does sound bend around corners but light does not?
▶️ Answer / Explanation
- Sound has a very large wavelength (≈ 1 m).
- Building doorways and corners have size ≈ wavelength → strong diffraction.
- Light has a very small wavelength (≈ \( 5 \times 10^{-7} \) m) → barely diffracts.
Example (Medium)
A slit has width equal to the wavelength of a wave. Describe what happens as the wave passes through the slit using Huygens’ principle.
▶️ Answer / Explanation
Each point on the slit behaves as a source of secondary wavelets. These wavelets spread in all forward directions, overlapping to produce a nearly circular wavefront. This results in strong diffraction.
Example (Hard)
Explain why diffraction decreases when slit width becomes much larger than wavelength.
▶️ Answer / Explanation
- A wider slit contains many secondary sources (according to Huygens).
- Most of these are in the interior → their wavelets interfere and reinforce a forward-moving plane wave.
- Only the edge sources produce spreading, but their effect becomes small compared to interior contributions.
- Thus, the outgoing wave remains almost straight → little diffraction.
Diffraction Grating: Using the Equation \( n\lambda = d\sin\theta \)
A diffraction grating consists of many equally spaced slits that diffract light and produce sharp interference maxima. The condition for maxima is given by the diffraction grating equation.
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Diffraction Grating Formula
The angles at which bright fringes (maxima) occur are found using:
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\( n\lambda = d\sin\theta \)
- \( n \) = order of maximum (0, 1, 2, 3 …)
- \( \lambda \) = wavelength of light (m)
- \( d \) = grating spacing (m)
- \( \theta \) = angle of diffraction (from normal)
Meaning: Constructive interference occurs when the path difference between adjacent slits equals an integer multiple of wavelength.
Grating Spacing \( d \)
If the grating has \( N \) lines per metre, then:
\( d = \dfrac{1}{N} \)
Example: 600 lines per mm → \( N = 600 \times 10^3 = 6.0\times10^5\ \mathrm{m^{-1}} \) → \( d = \dfrac{1}{6.0\times10^5} \)
Features of Diffraction Gratings
- Produce very sharp, bright maxima (better than double slits)
- Widely used in spectroscopy
- Higher orders give larger angles
- Maximum order when \( \sin\theta = 1 \), so:
\( n_{\text{max}} = \dfrac{d}{\lambda} \)
How to Use the Formula
- Find \( d \) from number of lines per metre.
- Choose the order \( n \) (e.g., 1st, 2nd, 3rd).
- Substitute wavelength \( \lambda \).
- Solve for the angle \( \theta \) or wavelength depending on the question.
Example (Easy)
A grating has 500 lines per mm. Find the slit spacing \( d \).
▶️ Answer / Explanation
500 lines/mm = \( 500 \times 10^3 = 5.0\times10^5\ \mathrm{m^{-1}} \)
\( d = \dfrac{1}{5.0\times10^5} = 2.0\times10^{-6}\ \mathrm{m} \)
Example (Medium)
White light of wavelength \( \lambda = 600\ \mathrm{nm} \) falls on a grating with spacing \( d = 2.0\times10^{-6}\ \mathrm{m} \). Find the first-order diffraction angle.
▶️ Answer / Explanation
Using \( n\lambda = d\sin\theta \):
\( 1 \times 600\times10^{-9} = 2.0\times10^{-6}\sin\theta \)
\( \sin\theta = \dfrac{600\times10^{-9}}{2.0\times10^{-6}} = 0.300 \)
\( \theta = \sin^{-1}(0.300) \approx 17.5^\circ \)
Example (Hard)
Light of wavelength \( 520\ \mathrm{nm} \) is used with a diffraction grating of spacing \( 1.80\times10^{-6}\ \mathrm{m} \). What is the highest possible order visible?
▶️ Answer / Explanation
Condition for maximum order:
\( n_{\text{max}} = \dfrac{d}{\lambda} \)
\( n_{\text{max}} = \dfrac{1.80\times10^{-6}}{520\times10^{-9}} = 3.46 \)
The highest whole number ≤ 3.46 is:
n = 3
Maximum observable order = 3
