Muons are the most penetrating radiographic probe that exists today. These elementary particles possess a unique combination of physical properties that allows them to pass through dense, heavily shielded objects that are opaque to typical photon/neutron probes, and emerge with useful radiographic information on the object's internal substructure. Interactions of cosmic rays in the Earth's upper atmosphere provide a constant, natural source of muons that can be used for passive interrogation, eliminating the need for artificial sources of radiation. These proceedings discuss specific applications of muon radiography in nuclear safeguards and arms control treaty verification.
I. INTRODUCTIONHighly energetic radiation produced in astrophysical processes is constantly bombarding the Earth. These naturally occurring cosmic rays provide a window into the dynamics of distant events in our universe, and as such have been the subject of intense scrutiny. Among recent work, measurements have shown that the incident high-energy cosmic ray flux includes neutrinos [1], gamma rays [2, 3], positrons and electrons [4], and heavy nuclei [5,6]. These particles can have energies much higher than can produced in terrestrial accelerators: iron nuclei with energies above 10 5 GeV have been observed (see [7] for a review). When these heavy, energetic cosmic ray nuclei collide with nitrogen or oxygen nuclei that are present in the atmosphere, a short-lived phase of quark-gluon plasma is created, which immediately freezes out and produces hundreds of charged pions. Charged pions have a lifetime of 2.6×10 −8 s and have a nearly 100% branching ratio to decay into a neutrino and a muon.