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A detailed investigation of radio galaxies has recently stressed these sources as the possible origin of the cosmic rays observed above $3\,\text{EeV}$. Here, the relevance of this model at energies below $3\,\text{EeV}$ is investigated.…

High Energy Astrophysical Phenomena · Physics 2019-06-12 Björn Eichmann

Accretion and merger shocks in clusters of galaxies are potential accelerators of high-energy protons, which can give rise to high-energy neutrinos through pp interactions with the intracluster gas. We discuss the possibility that protons…

Astrophysics · Physics 2012-01-18 Kohta Murase , Susumu Inoue , Shigehiro Nagataki

We present preliminary results obtained by a novel difference method for the study of the nature of the knee in the energy spectrum of the primary cosmic radiation. We have applied this method to data from the GAMMA experiment in Armenia.…

Investigations of the energy spectrum as well as the mass composition of cosmic rays in the energy range of PeVto EeV are important for understanding both, the origin of the galactic and the extragalactic cosmic rays. Recently, three modern…

High Energy Astrophysical Phenomena · Physics 2015-04-09 Andreas Haungs

Recent observations of cosmic ray protons in the energy range $10^2$--$10^5$~GeV have revealed that the spectrum cannot be described by a simple power law. A hardening of the spectrum around an energy of order few hundred~GeV, first…

High Energy Astrophysical Phenomena · Physics 2020-04-01 Paolo Lipari , Silvia Vernetto

We have carried out a detailed study to understand the observed energy spectrum and composition of cosmic rays with energies up to ~10^18 eV. Our study shows that a single Galactic component with subsequent energy cut-offs in the individual…

High Energy Astrophysical Phenomena · Physics 2016-11-15 S. Thoudam , J. P. Rachen , A. van Vliet , A. Achterberg , S. Buitink , H. Falcke , J. R. Hörandel

This review focuses on high-energy cosmic rays in the PeV energy range and above. Of particular interest is the knee of the spectrum around 3 PeV and the transition from cosmic rays of Galactic origin to particles from extra-galactic…

High Energy Astrophysical Phenomena · Physics 2013-03-15 Thomas K. Gaisser , Todor Stanev , Serap Tilav

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

High statistical accuracy of experiments KASCADE and ANI allowed to obtain approximations of primary energy spectra and elemental composition in the "knee" region. Obtained results point out to the correctness of QGSJET interaction model…

Astrophysics · Physics 2007-05-23 Samvel Ter-Antonyan , Peter Biermann

The nature of the knee in the all-particle spectrum of cosmic rays remains subject of much investigation, especially in the aftermath of recent measurements claiming the detection of a knee-like feature in the spectrum of the light…

High Energy Astrophysical Phenomena · Physics 2019-06-13 Carlo Mascaretti , Pasquale Blasi , Carmelo Evoli

The present experimental status concerning the composition of cosmic rays in the PeV region is reviewed. The results are compared to predictions of contemporary models for the acceleration and propagation of galactic cosmic rays.

Astrophysics · Physics 2009-11-10 Joerg R Hoerandel

Our study exploits the Constant Intensity Cut principles applied simultaneously to muonic and electromagnetic detectors of cosmic rays. We use the fact that the ordering of events according to their signal sizes induced in different types…

High Energy Astrophysical Phenomena · Physics 2017-08-22 Jakub Vicha , Dalibor Nosek , Petr Travnicek , Jan Ebr

Ground-based cosmic ray experiments detect cosmic ray mainly by measuring the longitudinal and lateral distribution of secondary particles produced in the extensive air shower (EAS). The EAS of cosmic ray in the knee energy region is…

High Energy Astrophysical Phenomena · Physics 2024-09-30 Feng Zhang , Hu Liu , Fengrong Zhu , Jacob Oloketuyi

Primary energy spectral models are tested in the energy range of 1-200 PeV using standardized extensive air shower responses from BASJE-MAS, Tibet, GAMMA and KASCADE scintillation shower arrays. Results point towards the two-component…

High Energy Astrophysical Phenomena · Physics 2014-10-07 Samvel Ter-Antonyan

Some recent measurements of the chemical composition of the cosmic radiation indicate that at the energy of 3 x 10 **18 eV, around the ankle, light cosmic ions dominate the spectrum as it occurs in the preknee energy region. Taking…

High Energy Astrophysical Phenomena · Physics 2010-02-28 Antonio Codino , Francois Plouin

We perform a fit to measurements of the cosmic ray spectrum and of the depth of shower maximum in the energy range between $10^{15}$~eV and $10^{18}$~eV. We consider a Galactic component that is a mixture of five representative nuclear…

High Energy Astrophysical Phenomena · Physics 2019-03-15 Silvia Mollerach , Esteban Roulet

The average mass composition of cosmic rays with primary energies between $10^{17}$eV and $10^{18}$eV has been studied using a hybrid detector consisting of the High Resolution Fly's Eye (HiRes) prototype and the MIA muon array.…

We present a study of the high energy spectra of hadrons in cores of extensive air showers. These data were obtained for the first time in the hybrid {\it HADRON} experiment (Tien-Shan) by means of a large X-ray emulsion chamber combined…

High Energy Astrophysical Phenomena · Physics 2019-05-27 Sergey Shaulov

Recent advances in measuring and interpreting cosmic rays from the spectral ankle to the highest energies are briefly reviewed. A knee of heavy primaries and an ankle of light primaries have been observed at about 10^{17} eV. The light…

High Energy Astrophysical Phenomena · Physics 2014-04-28 Karl-Heinz Kampert

A sudden steepening of the cosmic-ray energy spectrum (the knee) is observed at an energy of about 3 PeV (1 PeV = $10^{15}$ eV). The experimental study of the PeV cosmic rays has intensified greatly during the last 3 years. The recent…

Astrophysics · Physics 2009-10-31 A. D. Erlykin , A. W. Wolfendale
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