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Related papers: In Search of a Source for the 320 Eev Fly's Eye Co…

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The origin of cosmic rays with energies higher than 10$^{20}$ eV remains a mystery. Accelerating particles up to these energies is a challenge even for the most energetic astrophysical objects known. While the isotropy in arrival directions…

Astrophysics · Physics 2017-08-23 A. V. Olinto

Candidate astrophysical acceleration sites capable of producing the highest energy cosmic rays (E > 10^{19.5} eV) appear to be at far greater distances than is compatible with their being known particles. The properties of a new particle…

Astrophysics · Physics 2009-10-30 Glennys R. Farrar

Almost three decades ago, the Fly's Eye experiment recorded the most energetic cosmic-ray ever observed. With an energy of 320 EeV, this event is well beyond the suppression region of the ultra-high energy cosmic rays (UHECR) spectrum.…

High Energy Astrophysical Phenomena · Physics 2020-02-05 Thomas Fitoussi , Gustavo Medina-Tanco , Juan-Carlos D'Olivo

It is presumed that the observed cosmic rays up to about $3\times 10^{18}$ eV are of Galactic origin, the particles being the ones which are found in the composition of the stellar winds of stars that explode as supernova into the…

Astrophysics · Physics 2007-05-23 Adrian Sabin Popescu

The primary cosmic rays particles with energies above 10**20 eV have been observed at many extensive air shower arrays since the beginning of observations over 40 years ago. The validity of measurements of signal s(600) used as energy…

Astrophysics · Physics 2008-11-06 L. G. Dedenko , D. A. Podgrudkov , T. M. Roganova , G. F. Fedorova

We report the detection of a 51-joule (320 +/- 90 EeV) cosmic ray by the Fly's Eye air shower detector in Utah. This is substantially greater than the energy of any previously reported cosmic ray. A Greisen-Zatsepin-Kuz'min cutoff of the…

Astrophysics · Physics 2009-10-22 D. J. Bird et al.

Extensive air showers still are our only access to the highest-energy particles in the universe, namely cosmic-ray nuclei with energies up to several 100 EeV. Studying open questions in cosmic-ray physics, like their yet unknown origin…

High Energy Astrophysical Phenomena · Physics 2017-04-21 Frank G. Schröder

In this Letter we examine the arrival directions of the most energetic cosmic rays (E > 2 * 10^19 eV) detected by several air shower experiments. We find that data taken by different air shower arrays show positive correlations, indicating…

Astrophysics · Physics 2008-11-26 Todor Stanev , Peter Biermann , Jeremy Lloyd-Evans , Joerg Rachen , Alan Watson

Cosmic rays are charged relativistic particles that reach the Earth with extremely high energies, providing striking evidence of the existence of effective accelerators in the Universe. Below an energy around $\sim 10^{17}$ eV cosmic rays…

High Energy Astrophysical Phenomena · Physics 2018-04-25 Giovanni Morlino

The existence of cosmic ray particles up to the ultra-high energy limit (> 10^20 eV) is now beyond any doubt. The detection of cosmic particles with such energies imposes a challenge for the comprehension of their sources and nature. On one…

An analysis of arrival directions of extensive air showers generated by cosmic rays in the PeV energy range and registered with the EAS MSU and EAS-1000 Prototype arrays reveals a considerable number of regions of excessive flux of cosmic…

High Energy Astrophysical Phenomena · Physics 2015-05-13 M. Yu. Zotov , G. V. Kulikov

The observation of twenty cosmic-ray air-showers at and above 10^{20} eV poses fascinating problems for particle astrophysics: how the primary particles are accelerated to these energies, how the primaries get here through the 2.7K…

High Energy Physics - Phenomenology · Physics 2009-11-07 Thomas J. Weiler

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 revisit and extend the analysis supporting a 60 year-old suggestion that cosmic rays air showers resulting from primary particles with energies above 10^{18} eV should be straightforward to detect with radar ranging techniques, where the…

High Energy Physics - Experiment · Physics 2011-05-23 Peter. W. Gorham

The cosmic rays spectrum has been shown to extend well beyond 10^20 eV. With nearly 20 events observed in the last 40 years, it is now established that particles with energies near or above 10^21 eV. No nearby astrophysical object has been…

High Energy Physics - Phenomenology · Physics 2007-05-23 Olivier Deligny

The origin of the highest energy Galactic cosmic rays is still not understood, nor is the transition to EeV extragalactic particles. Scientific progress requires enhancements of existing air-shower arrays, such as: IceCube with its surface…

A survey of the northern hemisphere for astrophysical point sources with continuous emission of high-energy cosmic rays is presented. Around 47 Mio extensive air showers with primary energies above $\approx$ 300 TeV measured by the KASCADE…

Astrophysics · Physics 2019-08-14 T. Antoni

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

Cosmic rays are the highest energy particles found in nature. Measurements of the mass composition of cosmic rays between 10^{17} eV and 10^{18} eV are essential to understand whether this energy range is dominated by Galactic or…

High Energy Astrophysical Phenomena · Physics 2016-05-03 S. Buitink , A. Corstanje , H. Falcke , J. R. Hörandel , T. Huege , A. Nelles , J. P. Rachen , L. Rossetto , P . Schellart , O. Scholten , S. ter Veen , S. Thoudam , T. N. G. Trinh , J. Anderson , A. Asgekar , I. M. Avruch , M. E. Bell , M. J. Bentum , G. Bernardi , P. Best , A. Bonafede , F. Breitling , J. W. Broderick , W. N. Brouw , M. Brüggen , H. R. Butcher , D. Carbone , B. Ciardi , J. E. Conway , F. de Gasperin , E. de Geus , A. Deller , R. -J. Dettmar , G. van Diepen , S. Duscha , J. Eislöffel , D. Engels , J. E. Enriquez , R. A. Fallows , R. Fender , C. Ferrari , W. Frieswijk , M. A. Garrett , J. M. Griessmeier , A. W. Gunst , M. P. van Haarlem , T. E. Hassall , G. Heald , J. W. T. Hessels , M. Hoeft , A. Horneffer , M. Iacobelli , H. Intema , E. Juette , A. Karastergiou , V. I. Kondratiev , M. Kramer , M. Kuniyoshi , G. Kuper , J. van Leeuwen , G. M. Loose , P. Maat , G. Mann , S. Markoff , R. McFadden , D. McKay-Bukowski , J. P. McKean , M. Mevius , D. D. Mulcahy , H. Munk , M. J. Norden , E. Orru , H. Paas , M. Pandey-Pommier , V. N. Pandey , M. Pietka , R. Pizzo , A. G. Polatidis , W. Reich , H. J. A. Röttgering , A. M. M. Scaife , D. J. Schwarz , M. Serylak , J. Sluman , O. Smirnov , B. W. Stappers , M. Steinmetz , A. Stewart , J. Swinbank , M. Tagger , Y. Tang , C. Tasse , M. C. Toribio , R. Vermeulen , C. Vocks , C. Vogt , R. J. van Weeren , R. A. M. J. Wijers , S. J. Wijnholds , M. W. Wise , O. Wucknitz , S. Yatawatta , P. Zarka , J. A. Zensus

The field of ultra-high energy cosmic rays made a lot of progresses last years with large area experiments such as the Pierre Auger Observatory, HiRes and the Telescope Array. A suppression of the cosmic ray flux at energies above…

High Energy Astrophysical Phenomena · Physics 2014-11-20 Benoît Revenu
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