OpenWorldLab

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Interference

Michelson interferometer

A beam splitter sends half of a laser beam to each of two mirrors. The two halves come back, meet again and land on a screen. Where their paths differ by a whole number of wavelengths they add; half a wavelength more and they cancel. A mirror moved by a quarter of a micrometre turns a bright fringe dark.

What you are looking at

The red beam leaves the laser, spreads through a weak negative lens, and splits at the cube. One half goes right to the moving mirror, the other up to the fixed one. Both come back through the cube, and the half of each that turns down lands on the screen.

The screen card shows straight fringes. The moving mirror is turned by 150 microradians, so the two returning beams cross at a small angle and their phase difference changes across the screen.

How the bench is set up

HeNe laser at 632.8 nm, a −50 mm lens to widen the beam, a 50:50 cube, two flat mirrors 200 mm from the cube and a screen 300 mm below it.

Select the moving mirror and open “Fine adjustment”: the horizontal knob sets the tilt, the piezo moves the mirror along its axis by nanometres.

The theory

Two beams of equal power with a phase difference Δϕ\Delta\phi give an intensity

I=2I0 (1+cos⁡Δϕ),Δϕ=2πλ ΔℓI = 2I_0\,(1 + \cos\Delta\phi), \qquad \Delta\phi = \frac{2\pi}{\lambda}\,\Delta\ell

where Δℓ\Delta\ell is the difference in optical path. Moving a mirror by dd changes the path by 2d2d, so one fringe passes for every λ/2\lambda/2 of travel. Two collimated beams crossing at a small angle 2θ2\theta, from a mirror turned by θ\theta, make straight fringes with a period λ/2θ\lambda/2\theta.

Here the beam spreads from the lens’s focus, so each returning beam seems to come from a point. Turning the mirror moves that point’s image sideways by 2θa2\theta a, where aa is the path from the focus to the mirror, and the fringes are those of two point sources a distance LL along the path from the screen:

Λ=λL2θa.\Lambda = \frac{\lambda L}{2\theta a}.

With a≈470a \approx 470 mm and L≈970L \approx 970 mm that is about 4.4 mm, twice the collimated value.

What to measure

Fringe spacing λL/2θa; one fringe per λ/2 of mirror travel

  1. Open the screen’s card and count the fringes across a known width to find their period.
  2. Change the horizontal knob of the moving mirror and check that the period goes as 1/θ.
  3. Move the piezo by 316 nm (half a wavelength) and watch the pattern shift by exactly one fringe.

What the model leaves out

  • The laser is a single, stable line here unless you give it more modes; a real HeNe runs on two or three, and its fringes fade and return as the arm lengths differ by multiples of the tube length.
  • Vibration and air currents are modelled as small random path changes, not from a model of the room.

Things to try

  • Turn table isolation off in the Room tab and watch the fringes dance.
  • Turn the laser’s linewidth up to 1 THz, a coherence length of about 0.1 mm: the fringes stay while both arms are equal and fade once the moving mirror is 0.2 mm out.
  • Set the horizontal knob to zero so the whole beam is one fringe, put a photodiode where the screen is, and step the piezo: the reading goes from bright to dark and back once per 316 nm of travel, which is how a fringe counter measures distance.

References

  • E. Hecht (2017), Optics, 5th edition, Pearson.
  • A. A. Michelson and E. W. Morley (1887), On the relative motion of the Earth and the luminiferous ether, American Journal of Science 34, 333.

More experiments, and how the lab works, are in the laser lab’s overview.