Study Guide

Interference and Diffraction

AP Physics 2· AP Physics 2 CED — Geometric and Physical Optics· 14 min read

1. Fundamentals of Interference and Diffraction★★☆☆☆⏱ 3 min

Interference occurs when two or more coherent light waves (with constant phase difference) superpose, producing a resultant wave with amplitude dependent on the phase difference of the incoming waves. Diffraction is the bending of light as it passes through a narrow aperture or around an obstacle, an effect that only exists because light acts as a wave. Diffracted waves from different parts of the aperture naturally superpose, producing interference patterns.

📘 Definition

Coherent Light

Light waves that maintain a constant phase difference with each other, required to produce a stable, visible interference pattern.

This topic makes up approximately 10-15% of the total AP Physics 2 exam score, appearing in both multiple-choice (MCQ) and free-response (FRQ) sections, and provides foundational evidence for the wave nature of light.

2. Double-Slit Interference★★☆☆☆⏱ 4 min

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Young's double-slit experiment was the first definitive proof that light acts as a wave. In this setup, coherent monochromatic light passes through two narrow slits separated by distance , and projects onto a screen a distance away from the slits. For any point on the screen, the path difference between light from the two slits is .

Constructive interference (bright fringe) occurs when the path difference is an integer multiple of the wavelength:

dsinθ=mλ(m=0,±1,±2,...)d\sin\theta = m\lambda \quad (m = 0, \pm 1, \pm 2, ...)

Destructive interference (dark fringe) occurs when the path difference is a half-integer multiple of the wavelength:

dsinθ=(m+12)λ(m=0,±1,±2,...)d\sin\theta = \left(m + \frac{1}{2}\right)\lambda \quad (m = 0, \pm 1, \pm 2, ...)

For small angles (), , where is the vertical distance from the central maximum to the fringe. This simplifies to the fringe spacing formula (distance between adjacent bright fringes):

Δx=λLd\Delta x = \frac{\lambda L}{d}
📐 Worked Example

A student performs a double-slit experiment with 500 nm green light, a slit separation of 0.25 mm, and a screen placed 2.0 m from the slits. Calculate the spacing between adjacent bright fringes, and the total distance from the 0th order central maximum to the 3rd order bright fringe.

  1. 1

    Convert all units to meters for consistency:

    λ=500×109 m,d=0.25×103 m,L=2.0 m\lambda = 500 \times 10^{-9}\ \text{m}, d = 0.25 \times 10^{-3}\ \text{m}, L = 2.0\ \text{m}
  2. 2

    Apply the small-angle fringe spacing formula:

    Δx=λLd\Delta x = \frac{\lambda L}{d}
  3. 3

    Calculate the fringe spacing:

    Δx=(500×109)(2.0)0.25×103=4.0×103 m=4.0 mm\Delta x = \frac{(500 \times 10^{-9})(2.0)}{0.25 \times 10^{-3}} = 4.0 \times 10^{-3}\ \text{m} = 4.0\ \text{mm}
  4. 4

    The distance from 0th to 3rd order is 3 times the fringe spacing:

    3Δx=3(4.0 mm)=12 mm=0.012 m3\Delta x = 3(4.0\ \text{mm}) = 12\ \text{mm} = 0.012\ \text{m}

Exam tip:

Always convert all length units to the same base unit (usually meters) before plugging values into formulas; unit mismatches are the most common avoidable mistake on this topic.

3. Single-Slit Diffraction★★★☆☆⏱ 4 min

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When light passes through a single narrow slit of width , each point within the slit acts as a secondary wave source, and these secondary waves interfere to produce a diffraction pattern. The pattern features a wide, very bright central maximum, followed by much dimmer, narrower maxima on either side, with dark minima between each maximum. Unlike double-slit interference, single-slit maxima are not equally spaced.

The condition for dark minima (zero intensity) in single-slit diffraction is:

asinθ=mλ(m=±1,±2,...)a\sin\theta = m\lambda \quad (m = \pm 1, \pm 2, ...)

Note that is not a minimum, as all waves interfere constructively at the central maximum. For small angles, the distance from the central maximum to the first minimum on one side is . The full width of the central maximum (distance between the two first minima on opposite sides of center) is:

W=2λLaW = \frac{2\lambda L}{a}

A key relationship: decreasing the slit width increases the width of the central maximum, meaning more diffraction occurs for smaller apertures.

📐 Worked Example

A 633 nm red laser passes through a single slit of width 0.10 mm, producing a diffraction pattern on a screen 1.5 m away. What is the full width of the central bright maximum?

  1. 1

    Convert all units to meters:

    a=0.10×103 m,λ=633×109 m,L=1.5 ma = 0.10 \times 10^{-3}\ \text{m}, \lambda = 633 \times 10^{-9}\ \text{m}, L = 1.5\ \text{m}
  2. 2

    Use the full central maximum width formula for small angles:

    W=2λLaW = \frac{2\lambda L}{a}
  3. 3

    Substitute and calculate:

    W=2(633×109)(1.5)0.10×103=1.9×102 m=1.9 cmW = \frac{2(633 \times 10^{-9})(1.5)}{0.10 \times 10^{-3}} = 1.9 \times 10^{-2}\ \text{m} = 1.9\ \text{cm}
  4. 4

    Verify the trend: a narrow 0.10 mm slit produces a reasonably large 1.9 cm central width, which matches expected diffraction behavior.

Exam tip:

Never mix up (single slit width) and (slit separation for double-slit/grating); swapping these gives an answer off by multiple orders of magnitude.

4. Diffraction Gratings★★★☆☆⏱ 4 min

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A diffraction grating is an optical device with hundreds or thousands of equally spaced parallel slits etched into a glass or metal surface. It produces much sharper, brighter, and better-separated principal maxima than a double-slit, making it ideal for measuring the wavelength of unknown light or splitting white light into its component wavelengths to produce a spectrum.

For a grating with lines per unit length, the separation between adjacent slits is . The condition for principal (bright) maxima is identical to the double-slit constructive interference condition:

dsinθ=mλ(m=0,±1,±2,...)d\sin\theta = m\lambda \quad (m = 0, \pm 1, \pm 2, ...)

Since can never be greater than 1, the maximum possible order is the largest integer less than . Any order with does not exist, as it would require a diffraction angle larger than 90°.

📐 Worked Example

A diffraction grating has 300 lines per mm. It is illuminated with white light, which has a wavelength range of 400 nm (violet) to 700 nm (red). What is the highest order complete full spectrum produced by this grating?

  1. 1

    Calculate in meters: 300 lines per mm = 300,000 lines per meter, so:

    d=13000003.33×106 md = \frac{1}{300000} \approx 3.33 \times 10^{-6}\ \text{m}
  2. 2

    The longest wavelength (red) diffracts the most, so if red for order is still visible (i.e., ), all shorter wavelengths in the spectrum will also be visible for that order.

  3. 3

    Calculate the maximum possible for red light:

    m<dλred=3.33×106700×1094.76m < \frac{d}{\lambda_{\text{red}}} = \frac{3.33 \times 10^{-6}}{700 \times 10^{-9}} \approx 4.76
  4. 4

    Since must be an integer, the highest order complete spectrum is . For , , which is impossible.

Exam tip:

Always check if your calculated is greater than 1; if it is, that order does not exist, and you need to pick the next smaller integer order.

5. AP-Style Problem Solving Practice★★★★☆⏱ 5 min

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📐 Worked Example

A double-slit experiment is set up in air with 700 nm red light, producing a fringe spacing of 5.0 mm. If the entire apparatus is fully immersed in pure water (refractive index ), what is the new fringe spacing?

A) 6.65 mm B) 3.76 mm C) 5.0 mm D) 2.83 mm

  1. 1

    The wavelength of light in a medium with refractive index is , where is the wavelength in air.

  2. 2

    Fringe spacing is proportional to wavelength: , so the new fringe spacing is the original spacing divided by :

  3. 3

    . The correct answer is B.

📐 Worked Example

A student uses a diffraction grating to measure the wavelength of an unknown laser. The grating has 500 lines per mm, and the two first-order bright spots are 1.28 m apart on a screen 2.00 m from the grating. (a) Calculate the wavelength of the laser. (b) The student claims a second-order maximum for this laser exists. Justify whether the student is correct. (c) If the laser is replaced with one of shorter wavelength, what happens to the distance between the first-order maxima? Explain your reasoning.

  1. 1

    (a) The distance from the central maximum to one first-order spot is . Grating slit separation: .

    tanθ=0.64/2.00=0.32,sinθ0.304\tan\theta = 0.64/2.00 = 0.32, \quad \sin\theta \approx 0.304
  2. 2

    Rearrange for :

    λ=(2.00×106)(0.304)=608×109 m=608 nm\lambda = (2.00 \times 10^{-6})(0.304) = 608 \times 10^{-9}\ \text{m} = 608\ \text{nm}
  3. 3

    (b) Check the value of for :

    sinθ=2(608×109)2.00×106=0.608\sin\theta = \frac{2(608 \times 10^{-9})}{2.00 \times 10^{-6}} = 0.608
  4. 4

    Since , the angle is valid, so the student is correct: the second-order maximum exists.

  5. 5

    (c) The distance between the first-order maxima will decrease. From , a shorter wavelength gives a smaller , a smaller diffraction angle , and a smaller distance from the central maximum to each first-order spot, so the total distance between the two spots decreases.

6. Common Pitfalls

Wrong move:

Swapping (slit separation) and (slit width), calculating instead of .

Why:

The symbols are both lowercase letters, so students often confuse what each variable measures.

Correct move:

Label every variable on your diagram as you read the problem: write between two slits, write across the single slit width before starting calculations.

Wrong move:

Forgetting that the full width of the central maximum in single-slit diffraction is , using instead.

Why:

Students memorize that the first minimum is at from center, so they stop there instead of doubling for full width between the two minima.

Correct move:

Always confirm: 'full width of central maximum' means distance between the two first minima on either side, so multiply the distance from center to one minimum by two.

Wrong move:

Using the small angle approximation for large angles (e.g., diffraction grating problems where ).

Why:

Students get used to small angles in basic double-slit experiments and automatically use the approximation regardless of angle size.

Correct move:

Only use the small angle fringe spacing formula when ; for larger angles, use the full relation and calculate position from .

Wrong move:

Calculating for a diffraction grating as (lines per meter) instead of .

Why:

Problems usually give lines per mm or lines per cm, so students just plug the given number in without inverting or converting units.

Correct move:

If you have lines per unit length, ; always convert to lines per meter first to get in meters.

Wrong move:

Mixing up constructive and destructive interference conditions, claiming constructive interference occurs at half-integer path differences.

Why:

Students memorize the conditions backwards or confuse them with thin film interference rules.

Correct move:

Start every interference problem by writing: Constructive = integer multiple of , destructive = half-integer multiple of at the top of your work.

7. Quick Reference Cheatsheet

Category

Formula

Notes

Double-slit constructive interference

, bright fringe condition, = slit separation

Double-slit destructive interference

, dark fringe condition

Double-slit small angle fringe spacing

Only valid for , = distance to screen

Single-slit diffraction minima

= slit width, , no minimum

Single-slit full central maximum width

Small angle approximation only

Diffraction grating slit separation

= lines per unit length

Diffraction grating principal maxima

Maxima are sharp and bright, same as double-slit constructive

Wavelength in medium

= vacuum wavelength, = refractive index

Maximum order of maxima

Any order with does not exist, since

When this came up on past exams

AI-estimated based on syllabus patterns — cross-check with official past papers for accuracy. Use only as revision-focus signals.

  • 2023 · MCQ

    Double-slit in water calculation

  • 2022 · FRQ

    Diffraction grating wavelength problem

What's Next

After mastering interference and diffraction, the next key topics in Unit 6 Geometric and Physical Optics are thin film interference and optical resolution, both of which rely directly on the path difference and interference rules you learned here. Without understanding this chapter, you cannot correctly calculate the conditions for constructive/destructive interference in thin films, or apply the Rayleigh criterion for resolving power of optical instruments. This topic also underpins the wave nature of matter, a core concept in modern physics, where electrons and other subatomic particles produce interference patterns identical to light. Interference and diffraction also enable many modern technologies from optical storage to astronomical spectroscopy.