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One of the most striking astrophysical phenomena today is the existence of cosmic ray particles with energies in excess of 10^20 eV. While their presence has been confirmed by a number of experiments, it is not clear where and how these…

High Energy Physics - Experiment · Physics 2009-11-11 Stefan Westerhoff

The detection of cosmic rays with energy around and in excess of $10^{20}$ eV raises many questions that future experiments will help answering to. I address here my view of some of these open issues, as they are now and as they might be…

Astrophysics · Physics 2017-08-23 Pasquale Blasi

Cosmic rays with energies above $10^{18}$ eV are currently of considerable interest in astrophysics and are to be further studied in a number of projects which are either currently under construction or the subject of well-developed…

Astrophysics · Physics 2009-11-10 R. J. Protheroe , R. W. Clay

Recent measurements of the properties of cosmic rays above 10^17 eV are summarized and implications on our contemporary understanding of their origin are discussed. Cosmic rays with energies exceeding 10^20 eV have been measured, they are…

Astrophysics · Physics 2015-05-13 Joerg R. Hoerandel

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

The present situation with regard to experimental data on ultra high-energy cosmic rays is briefly reviewed. Whilst detailed knowledge of the shape of the energy spectrum is still lacking, it is clear that events above 10^20 eV do exist.…

Astrophysics · Physics 2017-08-23 A. A. Watson

The highest energy cosmic rays observed possess macroscopic energies and their origin is likely to be associated with the most energetic processes in the Universe. Their existence triggered a flurry of theoretical explanations ranging from…

High Energy Physics - Phenomenology · Physics 2014-11-17 Guenter Sigl

It is commonly accepted that high energy cosmic rays up to $10^{19}$ eV can be produced in catastrophic astrophysical processes. However the source of a few observed events with higher energies remains mysterious. We propose that they may…

High Energy Physics - Phenomenology · Physics 2025-01-30 E. V. Arbuzova

The origin of cosmic rays is one of the major unresolved questions in astrophysics. In particular, the highest energy cosmic rays observed possess macroscopic energies and their origin is likely associated with the most energetic processes…

Astrophysics · Physics 2009-11-06 Guenter Sigl

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

A fundamental question that can be answered in the next decade is: WHAT IS THE ORIGIN OF THE HIGHEST ENERGY COSMIC PARTICLES? The discovery of the sources of the highest energy cosmic rays will reveal the workings of the most energetic…

High Energy Astrophysical Phenomena · Physics 2009-03-03 A. V. Olinto , J. H. Adams , C. D. Dermer , J. F. Krizmanic , J. W. Mitchell , P. Sommers , T. Stanev , F. W. Stecker , Y. Takahashi

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 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

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

High Energy Astrophysical Phenomena · Physics 2016-06-22 João R. T. de Mello Neto

Although cosmic rays were discovered 90 years ago, we do not know how and where they are accelerated. There is compelling evidence that the highest energy cosmic rays are extra-galactic -- they cannot be contained by our galaxy's magnetic…

Astrophysics · Physics 2009-11-07 F. Halzen

We discuss theoretical issues and experimental data that brought the ultra high energy cosmic rays in the list of Nature's greatest puzzles. After many years of research we still do not know how astrophysical acceleration processes can…

Astrophysics · Physics 2016-08-30 Todor Stanev

Over the last third of the century, a few tens of events, detected by ground-based cosmic ray detectors, have opened a new window in the field of high-energy astrophysics. These events have macroscopic energies, unobserved sources, an…

Astrophysics · Physics 2014-10-13 Xavier Bertou , Murat Boratav , Antoine Letessier-Selvon

This is a review of the most resent results from the investigation of the Ultrahigh Energy Cosmic Rays, particles of energy exceeding 10$^{18}$ eV. After a general introduction to the topic and a brief review of the lower energy cosmic rays…

High Energy Astrophysical Phenomena · Physics 2015-05-27 Antoine Letessier-Selvon , Todor Stanev

Cosmic rays have been observed up to energies $10^8$ times larger than those of the best particle accelerators. Studies of astrophysical particles (hadrons, neutrinos and photons) at their highest observed energies have implications for…

Astrophysics · Physics 2009-11-10 F. W. Stecker

This review summarizes recent developments in the understanding of high-energy cosmic rays. It focuses on galactic and presumably extragalactic particles in the energy range from the knee (10^15 eV) up to the highest energies observed…

High Energy Astrophysical Phenomena · Physics 2009-10-06 J. Bluemer , R. Engel , J. R. Hoerandel
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