High-energy cosmic rays are observed indirectly by detecting the extensive air showers
initiated in Earth's atmosphere. The interpretation of these observations relies on accurate …

In the last fifteen years radio detection made it back to the list of promising techniques for
extensive air showers, firstly, due to the installation and successful operation of digital radio …

The observation of electromagnetic radiation from radio to γ-ray wavelengths has provided a
wealth of information about the Universe. However, at PeV (10 15 eV) energies and above …

The present white paper is submitted as part of the “Snowmass” process to help inform the
long-term plans of the United States Department of Energy and the National Science …

We present a new version of the hadron interaction event generator sibyll. While the core
ideas of the model have been preserved, the new version handles the production of baryon …

In the six decades following the discovery of the neutrino by Cowan and Reines [1],
detectors have been realized that have explored the properties and sources of neutrinos …

A COMBINED MAXIMUM-LIKELIHOOD ANALYSIS OF THE HIGH-ENERGY ASTROPHYSICAL
NEUTRINO FLUX MEASURED WITH ICECUBE - IOPscience Skip to content IOP Science …

Since the recent detection of an astrophysical flux of high-energy neutrinos, the question of
its origin has not yet fully been answered. Much of what is known about this flux comes from …

This review focuses on high-energy cosmic rays in the PeV energy range and above. Of
particular interest is the knee of the spectrum around 3 PeV and the transition from cosmic …

We report on measurements of the all-particle cosmic ray energy spectrum and composition
in the PeV to EeV energy range using 3 years of data from the IceCube Neutrino …