Coherence length of cosmic background radiation enlarges the attenuation length of the ultra-high energy proton [PDF]
Kenzo Ishikawa, Yutaka Tobita
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About chemical composition of the primary cosmic radiation at ultra-high energies [PDF]
T.M. Roganova L.G. Dedenko +7 more
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Physics and Astrophysics with Ultra-High Energy Cosmic Radiation [PDF]
G. Sigl
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On Gamma Rays as Predictors of Ultra-high-energy Cosmic-Ray Flux in Active Galactic Nuclei
Active galactic nuclei (AGN) are among the main candidates for ultra-high-energy cosmic-ray (UHECR) sources. However, while some theoretical and phenomenological works favor AGNs as the main sources, recent works have shown that using the very-high ...
Cainã de Oliveira +2 more
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Near-field effects of Cherenkov radiation induced by ultra high energy cosmic neutrinos [PDF]
Chia-Yu Hu, Chih-Ching Chen, Pisin Chen
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The Microwave Air Yield Beam Experiment (MAYBE): measurement of GHz radiation for Ultra-High Energy Cosmic Rays detection [PDF]
M. Monasor +20 more
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Monte Carlo simulations of induced extensive air showers (EASs) by ultra-high-energy cosmic rays are widely used in comparison with measured events at experiments to estimate the main cosmic ray characteristics, such as mass, energy, and arrival ...
Tudor Alexandru Calafeteanu +2 more
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The AMY experiment to measure GHz radiation for Ultra-High Energy Cosmic Ray detection [PDF]
Jaime Álvarez-Muñiz +24 more
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Cosmogenic Neutrino Point Source and KM3-230213A
Cosmogenic neutrinos (CNs) are produced by ultra-high-energy cosmic rays (UHECRs) interacting with cosmic background radiation. We investigated the properties of CN point/extended sources, i.e., the neutrino spectrum and angular profile as functions of ...
Qinyuan Zhang, Tian-Qi Huang, Zhuo Li
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A GPU-based Calculation Method for Near Field Effects of Cherenkov Radiation Induced by Ultra High Energy Cosmic Neutrinos [PDF]
Chia-Yu Hu, Chih-Ching Chen, Pisin Chen
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