9 - Cosmic-ray muon probe for internal structure of geophysical-scale materials

Summary

The spatial profile of the depth or density times length of the substance can be known by observing the manner of penetration of the energetic particle determined by electromagnetic interaction between the incoming particle and the stopping substance, which is called radiography. The most popular radiography is X-ray photography of a human body. As summarized in Table 9.1 and Figure 9.1, among various possible particles, very-high-energy (≥ 100 GeV) muon is the most suitable for measuring the density profile of a large-scale (≥ 0.1 km) substance like a mountain.

As described in Chapter 9, GeV–TeV cosmic-ray muons are constantly irradiating every substance on the earth. Muons arriving vertically from the sky have an intensity of 1 muon/cm² per min with a mean energy of a few GeV. The potential use of such high-energy muons to explore the internal structure of large-scale objects has been recognized in the past, with the prime example being the work done by Alvarez (1970), who studied the inside of an Egyptian pyramid in order to find a hidden chamber.

Muons arriving nearly horizontally along the earth's surface with a θ_z slightly less than 90^° have a lower intensity on average, but have a higher intensity at energies higher than a few hundreds of GeV, as can be seen in Figure 2.10.