Decay of a muon-probability of decay

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SUMMARY

The discussion focuses on calculating the energy required for a muon created by cosmic rays to reach Earth with a 10% probability of decay. The key equation derived is Δt = [ln(10)= ln(2)]τ, which indicates that the time Δt for 10% of muons to be detected is approximately 3.3 times the half-life τ of the muon. The effects of time dilation on the half-life of relativistic particles are emphasized, necessitating adjustments to the decay equation to account for the muon's speed and energy.

PREREQUISITES
  • Understanding of muon decay and half-life concepts
  • Familiarity with the exponential decay formula N=N0 exp(-ln(2)Δt/τ)
  • Knowledge of time dilation effects in relativistic physics
  • Basic principles of cosmic ray interactions
NEXT STEPS
  • Study the implications of time dilation on particle decay rates
  • Explore the relationship between muon energy and velocity in relativistic contexts
  • Investigate the derivation and application of the exponential decay formula in various scenarios
  • Learn about cosmic ray physics and its impact on particle detection on Earth
USEFUL FOR

Students and educators in physics, particularly those focusing on particle physics, relativistic effects, and cosmic ray interactions. This discussion is beneficial for anyone involved in experimental physics or theoretical studies related to muon behavior and decay probabilities.

sawhai
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Homework Statement



An energetic muon is created by the interaction of a cosmic ray 20 km away from the surface of the earth. How energetic does the muon have to be to be detected on Earth before it decays with a 10% probability?
For a single muon, what is the probability that it will not have decayed after time Δt?

Show that, assuming the muon would be detected if it doesn’t decay, the length of time since creation of the muon Δt where 10% of the muons will be detected is given by Δt = [ln(10)= ln(2)]τ ' 3:3τ .

Homework Equations


For a decay half-life τ, the fractional proportion of a large population of N0 muons remaining after a time Δt is N=N0 = exp(- ln(2)Δt=τ ). How can relate this to a singe muon without having t and λ?

The Attempt at a Solution


I set up the decay equation but not sure what to do next.
 
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Any one with an idea?
 
The half-life of particles moving relativistically is greater than that of particles in the rest frame due to the effects of time dilation.

You need to modify the decay equation to take account of time dilation. You might want to think about how the energy of the muon depends upon its speed.
 

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