Observations and implications of the ultrahigh-energy cosmic rays

By M. Nagano, A. Watson. 2000

604 citations recorded by the source corpus.

Subfields: Nuclear and High Energy Physics

View Paper: https://www.semanticscholar.org/paper/d27e7e610f200fa0d765317d66db765ad5b17349

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In Nuclear and High Energy Physics

Citations in the corpus

Constraining the New Aether: gravitational Cherenkov radiation (2005, background): “The study of Lorentz invariance violation has also been stimulated by the apparent non-observation of the GZK cutoff in the cosmic ray flux [4] (for a recent review see [5]).”
Magnetars in the Metagalaxy: An Origin for Ultra-High-Energy Cosmic Rays in the Nearby Universe (2002, background): “See Nagano & Watson (2000) for a thorough discussion of the strong evidence for the spectral hardening at the highest energies, including the uncertainties in the value of Ea.”
The Astrophysics of Ultrahigh-Energy Cosmic Rays (2011, methodology): “Due to the limited space, we refer readers interested in details of observational techniques to Letessier-Selvon & Stanev (2011), Beatty & Westerhoff (2009), Bluemer et al. (2009), and Nagano & Watson (2000).”
Electron-positron pairs in physics and astrophysics: from heavy nuclei to black holes (2009, background): “20)) that 〈E〉PD is in the range of energies of UHECR (see [420] and references therein), while for ξ ∼ 0.”
Science with a lunar low-frequency array: From the dark ages of the Universe to nearby exoplanets (2009, background): “Ultra-high energy cosmic rays (UHECRs) are a rare population of elementary particles, likely composed of protons, atomic nuclei, and potentially photons or neutrinos (Nagano and Watson, 2000).”
Cosmic ray anisotropy analysis with a full-sky observatory (2000, background): “Recent reports [8, 9, 10] suggest that the spectrum might continue without a strong GZK effect.”