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11. Coherence Length & Coherence Time

Module

Laser Light Concepts

Try it live

Explore this on the interactive simulator with real-time sliders and graphs: 🔬 Launch in Simulator

Aim

To study how the spectral linewidth of a source limits its coherence time and coherence length, and to observe the resulting loss of fringe visibility with increasing path difference.

Theoretical Background

An ideal monochromatic wave would maintain a perfectly definite phase relationship with itself indefinitely. Real sources, however, emit over a finite range of frequencies (linewidth Δν) because of finite emission-lifetime, Doppler, and other broadening mechanisms. This finite linewidth limits the time interval over which the wave's phase remains predictable — the coherence time, τc ≈ 1/Δν.

The corresponding coherence length, Lc = c·τc, is the maximum path difference between two beams derived from the same source for which a stable, high-contrast interference pattern can still be observed. Beyond this path difference, the fringes wash out because the relative phase between the two beams becomes effectively random from moment to moment.

A highly stabilized single-mode laser can have a coherence length of many metres, enabling holography and precision interferometry over large path differences, whereas an ordinary thermal source (LED or incandescent bulb) has a coherence length of only a few micrometres — far too short to show interference from two independently positioned sources of that type.

Governing Formulas

Coherence time:

\[ \tau_c \approx \dfrac{1}{\Delta\nu} \]

Coherence length:

\[ L_c = c\,\tau_c \]
Apparatus layout diagram for this experiment
Labelled apparatus layout — original illustration prepared for this guide (not a photograph). See the drag-to-rotate 3-D schematic below for a spatial view of the same setup.
3-D apparatus schematic · drag to rotate, scroll to zoom · Source → beamsplitter → variable-path mirror → detector

Simulator Controls

Control Symbol Range Unit
Source linewidth (via source type) Δν 1 MHz – hundreds of THz Hz
Path difference under test — 0 – 500 mm

Procedure

  1. Select the stabilized single-mode laser source and record τc and Lc from the readouts.
  2. Increase the tested path difference from 0 upward and record the fringe visibility at each value, noting the path difference at which visibility drops to about half its maximum.
  3. Repeat the procedure for the He-Ne laser, the LED and the white-light source, tabulating τc, Lc, and the visibility-versus-path-difference behaviour for each.
  4. Plot Lc for the four source types on a logarithmic scale to appreciate the many-orders-of-magnitude spread.

Observation Table

Table: Coherence time and length for four representative sources

S. No. Source Δν τc (calculated) Lc = cτc (calculated) Path diff. at half-visibility (observed)
1
2
3
4

Graph

Plot Fringe visibility (y-axis) against Path difference (mm) (x-axis).

Expected trend: visibility ≈ 1 for path difference ≪ Lc, falling toward 0 as path difference approaches/exceeds Lc.

Fringe visibility vs path difference for each source, showing the coherence-length cut-off

📋 Click the grid, then paste (Ctrl+V) a copied photo of your camera/CRO/DSO trace to overlay it for tracing — nothing is uploaded, it stays on your screen only.
Coherence Length vs Spectral Linewidth Linewidth, Δν (Hz, log scale suggested) Coherence length, L_c (m, log scale suggested)
15×15 grid — choose your own scale per square; plot from your observation table

Calculation

  1. For each source, compute τc = 1/Δν and Lc = c·τc from the given linewidth.
  2. Compare the calculated Lc with the path difference at which the simulator shows visibility dropping to ~50%, and comment on the agreement.

Result

Table: Coherence length: calculated vs observed

Source Lc (calculated) Lc (from visibility curve) Remarks
1
2
3

Maximum Permissible Error

L_c = c/Δν (c is exact), so the fractional error in coherence length equals the fractional error in your measurement of the source's spectral linewidth.

Precautions

  • Use a logarithmic scale when comparing coherence lengths across sources, since they differ by many orders of magnitude.
  • Keep in mind that Lc is a practical cut-off (visibility falling below usefulness), not an abrupt mathematical boundary.

Self-Check Quiz

1. A source with a broader spectral linewidth Δν has:
  • A) A longer coherence time
  • B) A shorter coherence time (τc ≈ 1/Δν)
  • C) The same coherence time regardless of linewidth
  • D) No relationship between linewidth and coherence

Answer: B — τc ≈ 1/Δν is inversely proportional to linewidth — a spectrally pure (narrow-linewidth) source has a longer coherence time.

2. Beyond the coherence length Lc, what happens to the interference fringes?
  • A) They become sharper
  • B) They wash out / lose contrast, because the relative phase becomes effectively random
  • C) They double in spacing
  • D) Nothing changes

Answer: B — Past Lc, the two beams' relative phase is no longer predictable moment to moment, so a stable pattern can no longer be sustained.

3. A single-mode stabilized laser typically has a much longer coherence length than a white-light source because:
  • A) Lasers are always more intense
  • B) The laser has a far narrower spectral linewidth Δν
  • C) White light travels slower
  • D) Coherence length doesn't depend on linewidth

Answer: B — Since Lc = c/Δν, a laser's extremely narrow linewidth directly gives it an enormously longer coherence length than a broadband thermal source.

4. Which relation correctly connects coherence length and coherence time?
  • A) Lc = c·τc
  • B) Lc = τc/c
  • C) Lc = c/τc
  • D) Lc and τc are unrelated

Answer: A — Coherence length is simply the distance light travels during one coherence time: Lc = c·τc.

Viva-Voce Questions

  1. Why can two separate light bulbs never produce a stationary interference pattern, however carefully arranged?
  2. How is coherence length exploited (or limited) in holography and in optical coherence tomography?
  3. Why do white-light sources produce fringes only very close to zero path difference, unlike a laser?
  4. How is coherence time τc related to the spectral bandwidth Δν of a source?
  5. Distinguish between temporal coherence and spatial coherence.
  6. Why does an LED have a much shorter coherence length than a single-mode laser?
  7. How would you experimentally estimate the coherence length of a source using an interferometer such as Michelson's?