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Cosmic-rays with energies exceeding 10^{19} eV are referred to as Ultra High Energy Cosmic Rays (UHECRs). The sources of these particles and their acceleration mechanism are unknown, and for many years have been the issue of much debate.…

High Energy Astrophysical Phenomena · Physics 2015-03-17 E. Waxman

We present a brief introduction to the physics of Ultra High Energy Cosmic Rays (UHECRs), concentrating on the experimental results obtained so far and on what, from these results, can be inferred about the sources of UHECRs.

Astrophysics · Physics 2007-05-23 Daniel De Marco

Anisotropy in the arrival direction distribution of ultrahigh-energy cosmic rays (UHECRs) produced by powerful sources is numerically evaluated. We show that, taking account of the Galactic magnetic field, nondetection of significant…

High Energy Astrophysical Phenomena · Physics 2016-01-22 Hajime Takami , Kohta Murase , Charles D. Dermer

Large-scale accretion shocks around massive clusters of galaxies, generically expected in hierarchical scenarios of cosmological structure formation, are shown to be potential sources of the observed ultrahigh energy cosmic rays (UHECRs) by…

Astrophysics · Physics 2007-11-08 Susumu Inoue , Guenter Sigl , Francesco Miniati , Eric Armengaud

We discuss the GZK horizon of protons and present a method to constrain the injection spectrum of ultrahigh energy cosmic rays (UHECRs) from supposedly identified extragalactic sources. This method can be applied even when only one or two…

Astrophysics · Physics 2009-07-17 M. Kachelriess , E. Parizot , D. V. Semikoz

From deflections in galactic and extragalactic magnetic fields energy dependent structures in the arrival directions of ultra-high energy cosmic rays (UHECR) are expected. We propose to characterize these structures by the strength of…

Instrumentation and Methods for Astrophysics · Physics 2013-08-01 Martin Erdmann , Tobias Winchen

The detection of high-energy astrophysical multimessengers establishes a connection between ultra-high-energy cosmic rays (UHECRs) and powerful cosmic accelerators. Interactions of UHECRs with radiation fields and interstellar matter…

High Energy Astrophysical Phenomena · Physics 2025-11-14 Rodrigo Sasse , Rubens Costa , Adriel G. B Mocellin , Carlos H. Coimbra Araújo , Rita de Cássia dos Anjos

A checklist of criteria is presented to help establish the sources of ultra-high energy cosmic rays (UHECRs). These criteria are applied to long-duration GRBs in order to determine if they are UHECR sources. The evidence seems to favor…

High Energy Astrophysical Phenomena · Physics 2015-05-27 Charles D. Dermer

Analysing the available data relative to the anisotropies of the ultra-high-energy cosmic rays (UHECR) at intermediate angular scales, we examine to what extent they can be used to constrain the origin of these particles, and what could be…

High Energy Astrophysical Phenomena · Physics 2024-06-26 Denis Allard , Julien Aublin , Bruny Baret , Etienne Parizot

EGRET data are usually analysed on the basis of the Maximum-Likelihood method \cite{ma96} in a search for point sources in excess to a model for the background radiation (e.g. \cite{hu97}). This method depends strongly on the quality of the…

Astrophysics · Physics 2009-10-30 Martin Pohl

The gamma-ray burst (GRB) model for production of ultra-high-energy cosmic-rays (UHECRs) is based on the hypothesis that GRBs arise from the dissipation of the kinetic energy of relativistic fireballs at cosmological distances. Recent GRB…

Astrophysics · Physics 2009-10-31 E. Waxman

Large-scale accretion shocks around massive clusters of galaxies, generically expected in the cold dark matter scenario of cosmological structure formation, are shown to be plausible sources of the observed ultrahigh energy cosmic rays…

Astrophysics · Physics 2008-03-10 Susumu Inoue , Guenter Sigl , Francesco Miniati , Eric Armengaud

We present the results of simulations of the ultra-high energy cosmic ray (UHECR) propagation in the Galactic magnetic field (GMF). Different assumptions on the large-scale GMF structure and/or primary particle lead to distinctly different…

High Energy Astrophysical Phenomena · Physics 2009-12-08 S. Vorobiov , M. Hussain , D. Veberič

The angular clustering of 5 Ultrahigh Energy Cosmic Rays (UHECRs) in the combined published AGASA-HiRes data has a probability of ~ 2 10^-3 of occurring by chance. A first analysis of the implications of the event energies and angular…

Astrophysics · Physics 2007-08-14 Glennys R. Farrar

Combined recent data from cosmic-ray detectors and gamma-ray detectors have produced some surprising insights regarding the sources of ultrahigh-energy cosmic rays (UHECRs), magnetic fields inside and outside the Milky Way, and the…

High Energy Astrophysical Phenomena · Physics 2015-05-20 Alexander Kusenko

Our latest paper investigates the effects of UHECR propagation in a turbulent intergalactic magnetic field in the small-angle scattering regime, specifically focusing on the non-trivial caustic-like pattern that arises with strong deviation…

High Energy Astrophysical Phenomena · Physics 2024-12-03 K. Dolgikh , A. Korochkin , G. Rubtsov , D. Semikoz , I. Tkachev

The lack of a high energy cutoff in the cosmic ray spectrum together with an apparently isotropic distribution of arrival directions for the highest energy events have strongly constrained most models proposed for the generation of these…

Astrophysics · Physics 2009-10-31 Angela V. Olinto

The suggested association between the sources of gamma-ray bursts (GRB's) and the sources of ultra-high energy cosmic rays (UHECR's) is based on two arguments: (i) The average energy generation rate of UHECR's is similar to the gamma-ray…

Astrophysics · Physics 2010-11-15 E. Waxman

We report an estimation of the injected mass composition of ultra-high energy cosmic rays (UHECRs) at energies higher than 10 EeV. The composition is inferred from an energy-dependent sky distribution of UHECR events observed by the…

High Energy Astrophysical Phenomena · Physics 2024-07-04 Telescope Array Collaboration , R. U. Abbasi , Y. Abe , T. Abu-Zayyad , M. Allen , Y. Arai , R. Arimura , E. Barcikowski , J. W. Belz , D. R. Bergman , S. A. Blake , I. Buckland , B. G. Cheon , M. Chikawa , T. Fujii , K. Fujisue , K. Fujita , R. Fujiwara , M. Fukushima , G. Furlich , N. Globus , R. Gonzalez , W. Hanlon , N. Hayashida , H. He , R. Hibi , K. Hibino , R. Higuchi , K. Honda , D. Ikeda , N. Inoue , T. Ishii , H. Ito , D. Ivanov , A. Iwasaki , H. M. Jeong , S. Jeong , C. C. H. Jui , K. Kadota , F. Kakimoto , O. Kalashev , K. Kasahara , S. Kasami , S. Kawakami , K. Kawata , I. Kharuk , E. Kido , H. B. Kim , J. H. Kim , J. H. Kim , S. W. Kim , Y. Kimura , I. Komae , V. Kuzmin , M. Kuznetsov , Y. J. Kwon , K. H. Lee , B. Lubsandorzhiev , J. P. Lundquist , H. Matsumiya , T. Matsuyama , J. N. Matthews , R. Mayta , K. Mizuno , M. Murakami , I. Myers , K. H. Lee , S. Nagataki , K. Nakai , T. Nakamura , E. Nishio , T. Nonaka , H. Oda , S. Ogio , M. Onishi , H. Ohoka , N. Okazaki , Y. Oku , T. Okuda , Y. Omura , M. Ono , A. Oshima , H. Oshima , S. Ozawa , I. H. Park , K. Y. Park , M. Potts , M. S. Pshirkov , J. Remington , D. C. Rodriguez , C. Rott , G. I. Rubtsov , D. Ryu , H. Sagawa , R. Saito , N. Sakaki , T. Sako , N. Sakurai , D. Sato , K. Sato , S. Sato , K. Sekino , P. D. Shah , N. Shibata , T. Shibata , J. Shikita , H. Shimodaira , B. K. Shin , H. S. Shin , D. Shinto , J. D. Smith , P. Sokolsky , B. T. Stokes , T. A. Stroman , Y. Takagi , K. Takahashi , M. Takamura , M. Takeda , R. Takeishi , A. Taketa , M. Takita , Y. Tameda , K. Tanaka , M. Tanaka , Y. Tanoue , S. B. Thomas , G. B. Thomson , P. Tinyakov , I. Tkachev , H. Tokuno , T. Tomida , S. Troitsky , R. Tsuda , Y. Tsunesada , S. Udo , F. Urban , D. Warren , T. Wong , K. Yamazaki , K. Yashiro , F. Yoshida , Y. Zhezher , Z. Zundel

Some studies suggested that a correlation between locations of BL Lacertae objects (BL Lacs) and the arrival directions of the ultrahigh energy cosmic rays (UHECRs) exists. Especially by assuming the primary particles charged +1 and using a…

Astrophysics · Physics 2007-05-23 Zhen Cao , Ben Zhong Dai , Jian Ping Yang , Li Zhang