Results 21 to 30 of about 29,691 (229)

ATLAS and ultra high energy cosmic ray physics

open access: yesEPJ Web of Conferences, 2017
After a brief introduction to extended air shower cosmic ray physics the current and future deployment of forward detectors at ATLAS is discussed along with the various aspects of the current and future ATLAS programs to explore hadronic physics.
Pinfold James
doaj   +2 more sources

Search for the large-scale cosmic-ray anisotropies using the TA and TALE surface detector arrays [PDF]

open access: yesEPJ Web of Conferences, 2023
Origins of ultra-high-energy cosmic rays (UHECRs) are still largely unknown. In particular, the “2nd knee” around 1017 eV could be related to a transition of origins from the galactic to extra-galactic sources.
Kimura Yusuke   +3 more
doaj   +1 more source

Neutrinos and Ultra-high-energy Cosmic-ray Nuclei from Blazars [PDF]

open access: yes, 2017
We discuss the production of ultra-high-energy cosmic-ray (UHECR) nuclei and neutrinos from blazars. We compute the nuclear cascade in the jet for both BL Lac objects and flat-spectrum radio quasars (FSRQs), and in the ambient radiation zones for FSRQs ...
X. Rodrigues   +4 more
semanticscholar   +1 more source

Search for ultra high energy cosmic ray sources

open access: yesEPJ Web of Conferences, 2017
Earlier we suggested a new method to search for sources and anisotropy of the arrival directions of ultra high energy particles. Here using this method we analyzed the data of the Yakutsk EAS array and found that particle fluxes with energies E < 4.1019 ...
Mikhailov A.A., Kolosov V.A.
doaj   +2 more sources

Air shower observation by a simple structured Fresnel lens telescope with a single pixel for the next generation of ultra-high-energy cosmic ray observatories [PDF]

open access: yesProgress of Theoretical and Experimental Physics, 2019
Improved statistics and mass-composition-sensitive observation are required to clarify the origin of ultra-high energy cosmic rays (UHECRs). Inevitably in the future, the UHECR observatories will have to be expanded due to the small flux; however, the ...
Y. Tameda   +11 more
semanticscholar   +1 more source

Constraints on the Hosts of UHECR Accelerators

open access: yesThe Astrophysical Journal Letters, 2023
Interactions of ultra-high-energy cosmic rays (UHECRs) in the surroundings of their accelerators can naturally explain the observed spectrum and composition of UHECRs, including the abundance of protons below the ankle.
Marco Stein Muzio, Glennys R. Farrar
doaj   +1 more source

An Indication of Anisotropy in Arrival Directions of Ultra-high-energy Cosmic Rays through Comparison to the Flux Pattern of Extragalactic Gamma-Ray Sources [PDF]

open access: yes, 2018
A new analysis of the data set from the Pierre Auger Observatory provides evidence for anisotropy in the arrival directions of ultra-high-energy cosmic rays on an intermediate angular scale, which is indicative of excess arrivals from strong, nearby ...
T. P. A. C. A. Aab   +391 more
semanticscholar   +1 more source

Ultra-High-Energy Gamma-Ray Astronomy [PDF]

open access: yesAnnual Review of Nuclear and Particle Science, 2023
Ultra-high-energy (UHE, >0.1 PeV) γ-ray astronomy is rapidly evolving into an expanding branch of γ-ray astronomy with the surprising discovery of 12 PeVatrons and the detection of a handful of photons above 1 PeV. Nearly all known celestial object types
Z. Cao   +3 more
semanticscholar   +1 more source

Active Galactic Nuclei as Potential Sources of Ultra-High Energy Cosmic Rays [PDF]

open access: yesUniverse, 2022
Active Galactic Nuclei (AGNs) and their relativistic jets belong to the most promising class of ultra-high-energy cosmic ray (UHECR) accelerators. This compact review summarises basic experimental findings by recent instruments, and discusses possible ...
F. Rieger
semanticscholar   +1 more source

Effects of the Galactic Magnetic Field on the UHECR Correlation Studies with Starburst Galaxies

open access: yesThe Astrophysical Journal, 2023
We estimate the biases caused by the coherent deflection of cosmic rays due to the Galactic magnetic field (GMF) in maximum likelihood analyses for searches of ultrahigh-energy cosmic-ray sources in the literature. We simulate mock event data sets with a
Ryo Higuchi   +4 more
doaj   +1 more source

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