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Related papers: Ultrahigh Energy Cosmic Rays

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The origin of the ultra high energy cosmic rays (UHECR) with energies above E > 1017eV, is still unknown. The discovery of their sources will reveal the engines of the most energetic astrophysical accelerators in the universe. This is a…

High Energy Astrophysical Phenomena · Physics 2016-04-27 M. T. Dova

The existence of cosmic rays of energies exceeding 10^20 eV is one of the mysteries of high energy astrophysics. The spectrum and the high energy to which it extends rule out almost all suggested source models. The challenges posed by…

Astrophysics · Physics 2009-11-10 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

The status of the observations of Ultra High Energy Cosmic Rays will be reviewed, focusing on the the latest results of HiRes and Auger observatories. A comprehensive analytical computation scheme to compute the expected UHECR spectrum on…

High Energy Astrophysical Phenomena · Physics 2013-06-04 Roberto Aloisio

Here we discuss the latest developments in the debate, where the ultrahigh energy cosmic ray particles come from. In this brief review, we emphasize the predictions that necessarily follow from the various concepts proposed. We discuss both…

Astrophysics · Physics 2014-10-13 Peter L. Biermann , Gustavo Medina-Tanco

This paper begins with a pedagogical discussion of the propagation of cosmic rays and the showers produced when a cosmic ray primary hits the upper atmosphere. The paper focusses cosmic rays, with energy > 10^19 eV. Emphasis is placed on…

Astrophysics · Physics 2011-05-12 James W. Cronin

Over the last decade a number of important observational results have been reported using data from the Pierre Auger Observatory. We shall review some of the recent key findings that have significantly advanced our understanding of…

High Energy Astrophysical Phenomena · Physics 2017-08-02 Karl-Heinz Kampert

Ultra-high-energy cosmic rays (UHECRs) are the highest energy messengers in the universe, with energies up to $10^{20}$ eV. Studies of astrophysical particles (nuclei, electrons, neutrinos and photons) at their highest observed energies…

High Energy Astrophysical Phenomena · Physics 2020-12-25 Joao de Mello Neto

Experimental results from Haverah Park, Yakutsk, AGASA and Fly's Eye are reviewed. All these experiments work in the energy range above 0.1 EeV. The 'dip' structure around 3 EeV in the energy spectrum is well established by all the…

Astrophysics · Physics 2009-09-25 Shigeru Yoshida , Hongyue Dai

We give a summary of the theoretical attempts to make sense of the observational data concerning the highest energy cosmic rays, (E > 3x10^{19} eV).

High Energy Physics - Phenomenology · Physics 2015-06-25 S. Kovesi-Domokos , G. Domokos

The Pierre Auger Observatory has been detecting ultra-high energy cosmic rays (UHECRs) for more than fifteen years. An essential feature of the Observatory is its hybrid design: cosmic rays above $100~$PeV are detected through the…

High Energy Astrophysical Phenomena · Physics 2023-03-01 Olivier Deligny

Experimental results on ultra-high-energy cosmic rays are briefly reviewed and their interpretation is discussed. The results related to principal observables (arrival directions, energies and composition) of primary particles of extended…

High Energy Astrophysical Phenomena · Physics 2013-04-23 Sergey Troitsky

While several arguments can be proposed against the existence of particles with energy in excess of $(3-5)\times 10^{19}$ eV in the cosmic ray spectrum, these particles are actually observed and their origin seeks for an explanation. After…

Astrophysics · Physics 2007-05-23 Pasquale Blasi

We briefly review the status of cosmic ray studies between $10^{14}$ eV and the highest observed energies, namely a few times $10^{20}$ eV. Because of the rather low incident fluxes in this energy range, the studies mostly rely on ground…

Astrophysics · Physics 2009-10-31 Murat Boratav , Alan A. Watson

We have measured the cosmic ray spectrum above 10^17.2 eV using the two air fluorescence detectors of the High Resolution Fly's Eye observatory operating in monocular mode. We describe the detector, photo-tube and atmospheric calibrations,…

Astrophysics · Physics 2008-11-26 s Eye Collaboration

Since their first observation in 1962, the existence of Ultra High Energy Cosmic Rays (UHECR) remains a mystery in modern astrophysics. Those cosmic rays, with energies well above 50 EeV ($50\times 10^{18}$eV), can hardly be accelerated,…

Astrophysics · Physics 2007-05-23 A. Letessier-Selvon

Ultra High Energy Cosmic Rays, UHECR, are charged particles with energies between $\sim10^{18}\,{\rm eV}$ and $\sim3\times10^{20}\,{\rm eV}\sim50\,{\rm J}$. They exhibit fundamental physics at energies inaccessible to terrestrial…

High Energy Astrophysical Phenomena · Physics 2025-05-29 Noémie Globus , Roger Blandford

The year 2007 has furnished us with outstanding results about the origin of the most energetic cosmic rays: a flux suppression as expected from the GZK-effect has been observed in the data of the HiRes and Auger experiments and correlations…

Astrophysics · Physics 2009-06-23 Karl-Heinz Kampert

It has been argued that the observations of cosmic particles with energies in excess of $10^8$ TeV represent a puzzle. Its solution requires new astrophysics or new particle physics. We show that the latter is unlikely given that the scale…

High Energy Physics - Phenomenology · Physics 2009-10-30 G. Burdman , F. Halzen , R. Gandhi

Ultra-high-energy cosmic rays, accelerated hadrons that can exceed energies of $10^{20}$ eV, are the highest-energy particles ever observed. While the sources producing UHECRs are still unknown, the Pierre Auger Observatory has detected a…

High Energy Astrophysical Phenomena · Physics 2025-10-28 Angelina Sherman , Ke Fang , Rafael Alves Batista , Rogerio Menezes de Almeida