Cosmic-Ray Muon Survival Lab

One event, two descriptions. A muon is made high in the atmosphere; does it reach the ground before it decays?
Beam
The energy slider is logarithmic (0.12 to 100 GeV total energy). Lifetime is the proper (rest-frame) mean lifetime; 2.197 microseconds is the measured value.
Frame bookkeeping
Experiment: does relativity matter here?
Fires 20,000 random decay times at each of ten energies and counts the muons that reach the ground. The chart shows the Monte Carlo against the exact law and the Newtonian prediction.
E (GeV)gammaNewtonTheoryMonte Carlo
Independent numerical checks
Running...
CheckResultReference
The science

Setup. A muon has rest energy m c² = 105.658 MeV and a proper mean lifetime τ = 2.197 µs, so cτ = 658.6 m. For total energy E the Lorentz factor is γ = E/(m c²) and the speed is β = √(1 - 1/γ²).

Earth frame: time dilation. The muon's clock runs slow by γ, so its mean lab-frame lifetime is γτ and its mean decay length is βγ c τ. Survival over a height H is P = exp(-H / (βγ c τ)). Without relativity (γ = 1) it would be exp(-H / (β c τ)), which for 15 km is about e-22.8: essentially no muons.

Muon frame: length contraction. The atmosphere is moving past the muon at βc and is squashed to H/γ. Ground arrives after a proper time H/(γ β c), and survival is exp(-t'/τ) with that time, giving exactly the same number. Both views describe one pair of events (creation, ground arrival) with the same invariant interval (c Δt)² - (Δx)² = (c Δτ)², computed in the checks by an explicit Lorentz transformation.

Monte Carlo. Each muon draws a proper decay time t' = -τ ln(u) and reaches the ground if t' > H/(γ β c). Fractions from batches of N muons have a binomial uncertainty √(P(1-P)/N), shown in the checks as a z-score.

Simplifications. A straight vertical path at constant energy: no energy loss in air (a real muon loses roughly 2 GeV crossing the atmosphere), no scattering, no inclination (real muons arrive at all zenith angles, lengthening the path), and a single production height (real muons form over a range of altitudes, mostly 10 to 20 km). The pictured number of muons is a sample, not a flux. Quoted sea-level figures (mean energy near 4 GeV, roughly one muon per square centimetre per minute) are typical textbook values.