Cosmic Muons: Time Dilation Made Visible

1 · Predict

Muons created by cosmic rays high in the atmosphere have a proper lifetime of only about 2.2 microseconds — not nearly enough time, at nearly light speed, to reach the ground unaided. Yet muons are detected at sea level in large numbers. Does time dilation explain this?

2 · Set Up

  1. Open the muon-time-dilation preset and press Reset. The muon's proper lifetime is fixed at 2.2 µs, speed β = 0.995.
  2. Enable the Lorentz factor and dilated-lifetime readouts.
  3. Set the muon's speed for each trial and record its dilated (Earth-frame) lifetime.

3 · Collect Data

Speed fraction β = v/cLorentz factor γDilated lifetime Δt (µs)
0.9
0.995
0.999

Plot dilated lifetime Δt (y-axis) against γ (x-axis) for your three trials. Is the line straight through the origin?

4 · Analyze

  1. For one trial, compute γ = 1/√(1 − β²), then Δt = γ·(2.2 µs). Compare to the table. Confirm β = 0.995 gives roughly a tenfold lifetime extension.
  2. Without time dilation, even at nearly light speed a 2.2 µs proper lifetime lets a muon travel only about 660 m — far short of the ~15 km atmospheric height where most are created. Explain how the dilated lifetime you computed changes this picture.

5 · Extend

  1. From the muon's own reference frame, its lifetime is still just 2.2 µs — but the muon 'sees' the atmosphere length-contracted, so it doesn't need to travel as far. Explain why both explanations (Earth-frame time dilation, or muon-frame length contraction) predict the exact same experimental outcome: the muon reaches the ground.
  2. The 1941 Rossi-Hall experiment comparing muon counts at a mountaintop versus at sea level was one of the first direct experimental confirmations of special relativity's time dilation. Why might comparing counts at two different altitudes be a clever way to test this prediction?

The Physics Behind This Experiment

Muon Time Dilation

A muon moving at β = 0.995 (γ ≈ 10) has its 2.2 µs proper lifetime stretched to about 22 µs as observed from Earth — long enough, combined with its near-light speed, to traverse the atmosphere and reach detectors at sea level.

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