2.5.11 · D3Optics

Worked examples — Young's double slit — fringe width derivation

3,309 words15 min readBack to topic

This page is the exhaustive problem-drill child of the fringe-width derivation. The parent gave you the two master tools:

Here we hit every kind of number these formulas can throw at you: the point above centre, the point below centre, the exact centre, the tiny-input and huge-input limits, a change of medium, a real-world word problem, and an exam twist. Each example says which cell of the matrix it fills, and — crucially — makes you forecast the answer before I show it.


The apparatus — every symbol, in words and a picture

Before any formula, meet the physical setup. The figure below is the schematic every example silently assumes; look at it once and the letters , , , , , , stop being mysterious.

Figure — Young's double slit — fringe width derivation

Notation we will lean on — defined once, in words

Two more symbols do the counting work, so let us pin them down before we ever use them in a sum.

We will also need the dark-fringe positions. A dark band sits exactly halfway between two bright ones, so its order is a half-integer:


The scenario matrix

Before working examples, let us list every case-class a YDSE problem can be. If a cell is not covered you would meet a scenario you have never seen — that is exactly what we forbid.

# Case class What is weird / what to watch Example that covers it
A Point above centre, Straight Ex 1
B Point below centre, is negative → same fringe by symmetry Ex 2
C Point at centre, → the zeroth (central) bright fringe Ex 2
D Find from a known fringe Rearrange , not Ex 3
E Bright or dark? classify a given Compute , integer vs half-integer Ex 4
F Medium change (water/oil) shrinks Ex 5
G Real-world word problem Reading a lab ruler, count fringes Ex 6
H Exam twist — shift screen distance Careful re-reading of which variable changed Ex 7
I Degenerate / limiting input (, , ) Does the formula stay sane? Ex 8

We now fill every cell.


Example 1 — Cell A (point above centre)

Step 1 — Convert to SI. , , . Why this step? The formula is only true if all lengths use the same ruler; mixing nm and mm gives nonsense.

Step 2 — Fringe width first. Why this step? is the "unit gap"; once we have it, the -th fringe is just of them.

Step 3 — Position of 3rd bright fringe. Why this step? , so counting fringes is literally counting 's.

The figure below turns this arithmetic into a picture: the blue bars are the bright bands at mm; notice each is exactly one green arrow () above the last, and the orange bar is our answer mm — the third rung up the ladder.

Figure — Young's double slit — fringe width derivation

Verify: Directly, ✓. Millimetres, as forecast — sensible for a lab bench.


Example 2 — Cells B & C (below centre, and the centre itself)

Step 1 — Below centre means . For the point below , . Why this step? is a signed height measured from ; below centre is negative. The path difference becomes , meaning now (the distance from slit to the point) is the longer path instead of .

Step 2 — Negative is still a valid bright condition. satisfies with . A whole number of wavelengths — positive or negative — is still constructive. Why this step? The pattern is symmetric about ; the fringe below looks identical to the one above. That is why we allow

The figure makes the mirror symmetry explicit: the blue slits on the left send dashed rays to three screen points. The green dot is (the central bright fringe at ); the orange dot is a point above (, ) and the red dot its mirror image below (, ). The two double-headed arrows are equal in length — that equality is the symmetry.

Figure — Young's double slit — fringe width derivation

Step 3 — The centre. At , . That is : a bright fringe. Why this step? Zero path difference means the two waves arrive perfectly in step — maximum brightness. The centre is always bright in a symmetric YDSE.

Verify: matches by symmetry ✓. Central fringe → constructive → bright ✓ (a common trap: people say the centre is dark).


Example 3 — Cell D (find the wavelength)

Step 1 — Choose the right formula. We know a specific fringe's position, so use , not alone. Why this step? tells you spacing; here we are handed the absolute position of fringe number , so the form is the direct fit.

Step 2 — Rearrange for . Why this step? Solve algebraically for the unknown before plugging numbers — fewer arithmetic slips.

Step 3 — Compute.

Verify: is orange-red visible light ✓ — inside 400–700 nm as forecast. Back-check: ✓.

This uses the small-angle result derived above.


Example 4 — Cell E (bright or dark? classify a point)

Step 1 — Compute the path difference. Why this step? is the master quantity — everything (bright/dark) is decided by comparing to . See Path difference and phase difference.

Step 2 — Divide by to count wavelengths. Why this step? Compare against the two exact conditions written as equations:

Step 3 — Classify. is neither an integer nor a half-integer. It lies between (dark) and (bright), so the point is partially lit — brighter than a minimum, dimmer than a maximum. Why this step? Real detectors read intensity smoothly; only the exact integer/half-integer points are pure max/min.

Verify: ✓; not in nor , so "neither" is correct ✓.


Example 5 — Cell F (immerse in a medium)

Step 1 — What changes in water? Frequency is fixed (set by the source); light slows by factor , so . Why this step? depends on the in-medium wavelength, and only changes — and are physical distances that do not care about the medium.

Step 2 — Scale the fringe width. Why this step? , so dividing by divides by the same .

Step 3 — Compute.

Verify: ✓ — narrower, as forecast (higher index squeezes the pattern).


Example 6 — Cell G (real-world word problem)

Step 1 — Count the gaps, not the fringes. From fringe number 1 to fringe number 10 there are gaps (each gap is one ). Picture nine fence-panels between ten fence-posts: ten posts, but only nine panels. So Why this step? This is the single most common lab error. The distance between fringe and fringe is , because from . Counting fringes (ten) instead of gaps (nine) inflates the spacing.

Step 2 — Solve for . Why this step? Everything else is measured; only is unknown, so isolate it.

Step 3 — Compute.

Verify: ✓ arithmetic — but this is ultraviolet, invisible to the eye. In a real lab that flags something: either the light truly is UV (detected on film, not by eye), or the student mis-counted and used 10 gaps instead of 9. Had they wrongly used mm they would get mm and — still UV, and further from any visible value. Lesson: count gaps = (last − first), then sanity-check the colour band.


Example 7 — Cell H (exam twist)

Step 1 — Compute . Why this step? Anchor the "before" value.

Step 2 — Use proportionality, don't recompute from scratch. , so . Why this step? Recognising is faster and exam-safe: only changed (the slits and their spacing are untouched), so scale.

Step 3 — The shift. Why this step? Exams often ask for the change, testing whether you know the linear dependence.

Verify: ✓ ; doubling doubled ✓ as forecast.


Example 8 — Cell I (degenerate & limiting inputs)

Step 1 — (slits merge). . Why this step? As the two slits merge into one, fringes spread infinitely far apart — meaning the whole screen becomes a single bright blur (no distinguishable pattern). This is the two-source pattern collapsing back to one source. Physically: you cannot have interference from a single opening (that is single-slit diffraction instead).

Step 2 — (screen very far). too, but the angular width stays fixed and finite. Why this step? The linear spacing grows without bound, yet the angle between fringes is independent of — that is why the parent note prized the angular form .

Step 3 — (imagine light with no wavelength). : fringes crowd infinitely close, washing into uniform brightness — no visible pattern. Why this step? Interference is a wave effect; a zero-wavelength wave behaves like a straight ray (geometric optics), and rays do not interfere. This is why we never see interference with, say, a cricket ball.

The figure plots against for fixed : watch the blue curve rocket toward the sky as shrinks to the left (the blow-up, red dashed line), and flatten toward small as grows to the right (fringes crowding, green arrow). It is the shape of made visible.

Figure — Young's double slit — fringe width derivation

Verify: All three limits are consistent with : numerator gives ; denominator gives ; gives while stays finite ✓.


Recap of the matrix

Recall Which example filled each cell?

A→Ex1, B→Ex2, C→Ex2, D→Ex3, E→Ex4, F→Ex5, G→Ex6, H→Ex7, I→Ex8. Every cell covered.

Recall The single question behind every problem

Compute , divide by : integer = bright, half-integer = dark, else in-between. ::: Yes — that one comparison drives all nine cells.

Recall How do you convert "distance across N fringes" into

? Count gaps = (last fringe number − first fringe number), then divide the measured distance by that number of gaps. ::: From fringe 1 to fringe 10 there are 9 gaps, so .


Connections

  • Young's double slit — fringe width derivation — the parent derivation these drills exercise.
  • Path difference and phase difference — the we compute in every example.
  • Small angle approximation — why throughout.
  • Refractive index — Example 5's medium change.
  • Coherence and coherent sources — needed for fringes to exist at all (Ex 8a).
  • Diffraction grating — the single-opening limit.
  • Interference of light — the umbrella phenomenon.