Ultrahigh-Energy Cosmic Rays: Physics and Astrophysics at Extreme Energies
Günter Sigl
The origin of cosmic rays is one of the major unresolved
questions in astrophysics. In particular, the highest energy cosmic rays observed have macroscopic energies up to several 1020
electron volts and thus provide a probe of physics and astrophysics at
energies unattained in laboratory experiments. Theoretical explanations
range from astrophysical acceleration of charged particles, to particle
physics beyond the established standard model, and processes taking
place at the earliest moments of our universe. Distinguishing between
these scenarios requires detectors with effective areas in the
1000-square-kilometer range, which are now under construction or in the
planning stage. Close connections with
-ray and neutrino
astrophysics add to the interdisciplinary character of this field.
Institut d'Astrophysique de Paris, CNRS, 98bis Boulevard Arago,
75014 Paris, France. E-mail: sigl{at}iap.fr