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NUCLEAR & PARTICLE PHYSICS · INTERACTIVE LAB 76

Cherenkov Radiation Laboratory

Explore the luminous shock cone produced when a charged particle outruns light’s phase velocity in a transparent medium.
Strong Cherenkov radiation in waterStrong Cherenkov emission
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Charged particleWavefrontCherenkov coneThreshold
Particle speed0.990c
Medium light speed0.750c
Threshold β0.750
Cherenkov angle40.8°
Threshold margin0.320
Relative intensityIllustrative

Cherenkov angle versus particle speed

Wavefront coherence

Speed comparison

particle β
c/n
vacuum c
0c/n < v < c — Cherenkov radiation is allowed without violating relativity.1.0c

Physics

v > c/ncos θ = 1/(nβ)βthreshold = 1/n

An optical shock wave

A charged particle polarises molecules along its path. If it travels faster than light’s phase velocity in that medium, the emitted wavefronts overlap coherently and form a cone—similar to a sonic boom.

No broken speed limit

The particle remains slower than light in vacuum. Transparent matter reduces light’s phase velocity to c/n, making c/n < v < c possible.

Why the glow is blue

The idealised emission spectrum favours shorter wavelengths. Real colour also depends on dispersion, absorption, detector sensitivity and the observer’s response.