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The earth is continually bombarded by high energy particles from outer space. These particles are mostly protons. Most are from galactic sources, primarily supernovae, but the very highest energy particles come from beyond the galaxy. The source of these is not well understood.

When these primary cosmic particles reach the top of the atmosphere, they interact, producing many secondary particles called pions. All of these quickly interact or decay and the only particles reaching the surface of the Earth are muons and neutrinos that come from decays of the pions. Neutrinos are nearly impossible to detect, but detecting the cosmic ray muons is easy since they are electrically charged and there are a lot of them. A good rule of thumb is that if you hold out your hand, about one muon per second will pass through it.

In the cosmic ray sessions, you will use a set detectors consisting of scintillation plastic that produces light (photons) when traversed by charged particles. Working in groups of three, you will use these to make measurements on the cosmic ray muons.

You will measure the muon flux and determine its dependence on direction (horizontal vs. vertical). You will measure the lifetime of the muon by measuring the time it takes a muon that stops in the detector to decay. The lifetime is on the order of one millionth of a second. You will be able to measure this to a precision of about 1%.

You will also measure the speed of the cosmic ray muons by measuring the time that it takes a muon to interact with two detectors separated by about a meter. Since the muons are traveling at nearly the speed of light, it will take about three billionths of a second for the muons to travel a distance of one meter. You will be able to measure this to a few percent, effectively measuring the speed of light to that precision.

Topics that we will cover in the sessions one cosmic rays include:

  • The sources and energy spectra of the primary cosmic rays
  • Cosmic ray showering in the atmosphere
  • Scintillating plastic detectors and photomultiplier tubes
  • Measurement of the exponential decay distribution of muons
  • Measurement of the speed of light.
  • Relativistic time dilation, the property of relativity that a moving clock ticks more slowly than one at rest
  • The physics of ultra high energy cosmic rays