Research news on Ultra-high-energy cosmic radiation

Ultra-high-energy cosmic radiation as a research area investigates cosmic rays with energies typically above 10¹⁸ eV, focusing on their origins, acceleration mechanisms, propagation through intergalactic and galactic magnetic fields, and interactions with cosmic microwave background photons (e.g., Greisen–Zatsepin–Kuzmin suppression). The field integrates astroparticle physics, high-energy astrophysics, and cosmology, using extensive air-shower observatories, fluorescence telescopes, and surface detector arrays to measure energy spectra, arrival directions, and mass composition. Research addresses candidate sources such as active galactic nuclei or gamma-ray bursts, tests hadronic interaction models at energies beyond terrestrial accelerators, and constrains fundamental physics, including Lorentz invariance and particle cross-sections at extreme energies.

The most energetic neutrino ever detected could be primordial

In the exotic world of particle physics, neutrinos may be the most mysterious members. They rarely interact with other matter, have almost no mass, and have no electrical charge. These characteristics make them extremely ...

The Amaterasu particle: Cosmic investigation traces its origin

Cosmic rays are extremely fast, charged particles that travel through space at nearly the speed of light. The Amaterasu particle was detected in 2021 by the Telescope Array experiment in the U.S. It is the second-highest-energy ...

Cosmic rays' vast energy traced to magnetic turbulence

Ultra-high energy cosmic rays, which emerge in extreme astrophysical environments—like the roiling environments near black holes and neutron stars—have far more energy than the energetic particles that emerge from our sun. ...

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