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Gravitational waves · laser interferometry

LIGO · Listening to Spacetime

How can a length change smaller than a proton become a readable signal? Through interference. A passing gravitational wave stretches one four-kilometer arm while squeezing the other. When the two returning laser beams recombine, that tiny difference changes how well they cancel, and the strain becomes a light signal you can read. Two observatories have to see it together before it counts.

Fly through a virtual LIGO detector. Watch freely falling masses stretch and squeeze as a gravitational wave passes, then enter the two perpendicular four-kilometre arms. Follow the laser as it splits, travels out and back, and cancels. At the end, two observatories confirm a black-hole merger together.

Interactive modelLIGO · Listening to Spacetime
Current scene1 · Spacetime strain
What changesProper distance
Signalh(t)

Scientific explanation

Read the picture as a physical process

What is happening

Why does the ring of masses become an ellipse?

Treat the dots as disconnected test masses in free fall. A gravitational wave arriving perpendicular to the ring does not blow them outward; it changes their proper separations. Plus polarization stretches one transverse axis while squeezing the other. Cross polarization is the same pattern rotated by 45 degrees.

Causal chain

  1. 1
    The wave passesThe transverse spacetime metric oscillates
  2. 2
    Distances changex grows while y shrinks
  3. 3
    The ring deformsThe long and short axes swap half a cycle later

Mathematical model

Lx(t)≈L[1+12h+(t)]Ly(t)≈L[1−12h+(t)]\begin{aligned} L_x(t) &\approx L\left[1 + \frac{1}{2}h_{+}(t)\right] \\ L_y(t) &\approx L\left[1 - \frac{1}{2}h_{+}(t)\right] \end{aligned}

Symbols

LL
Reference separation with no wave
h+(t)h_{+}(t)
Dimensionless plus-polarized strain
Lx, LyL_x,\,L_y
Proper separations along two transverse axes

Model limitsThis is the standard long-wavelength, TT-gauge teaching picture. The animation exaggerates strain by roughly 10²⁰. Coordinate positions may remain fixed while proper distances change.

Related experiments and articles

Continue exploring

Understand, then measure

How does a tiny arm-length change become a signal at the output?

  1. You are hereLIGO · Listening to SpacetimeTake a visual tour of spacetime, arms and optical readout.
  2. LabLIGO InterferometerVary the bias, arm storage and recycling in the measurement model.
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