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The origin of Galactic cosmic rays (CRs), particularly around the knee region ($\sim$3 PeV), remains a major unsolved question. Recent observations by LHAAASO suggest that the knee is shaped mainly by protons, with a transition to heavier…

High Energy Astrophysical Phenomena · Physics 2025-12-09 B. Theodore Zhang , Shigeo S. Kimura , Kohta Murase

The change in the fluxes of the lightest and heaviest nuclei in the mass composition of primary cosmic radiation in the energy range of E0 = 1-100 PeV is analyzed on the basis of data from the KASCADE-Grande experiment. This analysis is…

High Energy Astrophysical Phenomena · Physics 2021-12-30 S. E. Pyatovsky , A. D. Erlykin , V. S. Puchkov

Recently, the Large High Altitude Air Shower Observatory (LHAASO) published measurements of the all-particle CR energy spectrum and the mean logarithmic mass of CRs with unprecedented accuracy in 0.3-30 PeV. The mean logarithmic mass shows…

High Energy Astrophysical Phenomena · Physics 2025-09-03 A. A. Lagutin , N. V. Volkov

The cosmic-ray (CR) knee and the compositions contain abundant information for probing the CR's origin, acceleration and propagation mechanisms, as well as the frontier of the fundamental physics. Realizing that major proposals toward the…

High Energy Astrophysical Phenomena · Physics 2019-11-19 Chao Jin , Li-Qiao Yin , Song-zhan Chen , Hui-Hai He

The origin of the knee in the energy spectrum of cosmic rays is an outstanding problem in astroparticle physics. Numerous mechanisms have been proposed to explain the structure in the all-particle spectrum. In the article basic ideas of…

Astrophysics · Physics 2015-06-24 Joerg R. Hoerandel

The energies of cosmic rays, fully ionized charged nuclei, extend over a wide range up to 10^20 eV. A particularly interesting energy region spans from 10^14 to 10^18 eV, where the all-particle energy spectrum exhibits two interesting…

Astrophysics · Physics 2016-08-31 Joerg R. Hoerandel

Thanks to recent technological development, a new generation of cosmic ray experiments have been developed with more sensitivity to study these particles in the primary energy interval from 10 TeV to 1 PeV, such as HAWC. Due to its design…

High Energy Astrophysical Phenomena · Physics 2021-08-23 J. A. Morales-Soto , J. C. Arteaga-Velázquez

We report on the cosmic ray mass composition measured by the Telescope Array Low-energy Extension (TALE) hybrid detector. The TALE detector consists of a fluorescence detector (FD) station with 10 FD telescopes located at the Telescope…

High Energy Astrophysical Phenomena · Physics 2026-03-30 Telescope Array Collaboration , R. U. Abbasi , T. Abu-Zayyad , M. Allen , J. W. Belz , D. R. Bergman , F. Bradfield , I. Buckland , W. Campbell , B. G. Cheon , K. Endo , A. Fedynitch , T. Fujii , K. Fujisue , K. Fujita , M. Fukushima , G. Furlich , A. Gálvez Ureña , Z. Gerber , N. Globus , T. Hanaoka , W. Hanlon , N. Hayashida , H. He , K. Hibino , R. Higuchi , D. Ikeda , D. Ivanov , S. Jeong , C. C. H. Jui , K. Kadota , F. Kakimoto , O. Kalashev , K. Kasahara , Y. Kawachi , K. Kawata , I. Kharuk , E. Kido , H. B. Kim , J. H. Kim , J. H. Kim , S. W. Kim , R. Kobo , I. Komae , K. Komatsu , K. Komori , A. Korochkin , C. Koyama , M. Kudenko , M. Kuroiwa , Y. Kusumori , M. Kuznetsov , Y. J. Kwon , K. H. Lee , M. J. Lee , B. Lubsandorzhiev , J. P. Lundquist , H. Matsushita , A. Matsuzawa , J. A. Matthews , J. N. Matthews , K. Mizuno , M. Mori , S. Nagataki , K. Nakagawa , M. Nakahara , H. Nakamura , T. Nakamura , T. Nakayama , Y. Nakayama , K. Nakazawa , T. Nonaka , S. Ogio , H. Ohoka , N. Okazaki , M. Onishi , A. Oshima , H. Oshima , S. Ozawa , I. H. Park , K. Y. Park , M. Potts , M. Przybylak , M. S. Pshirkov , J. Remington , C. Rott , G. I. Rubtsov , D. Ryu , H. Sagawa , N. Sakaki , R. Sakamoto , T. Sako , N. Sakurai , S. Sakurai , D. Sato , K. Sekino , T. Shibata , J. Shikita , H. Shimodaira , H. S. Shin , K. Shinozaki , J. D. Smith , P. Sokolsky , B. T. Stokes , T. A. Stroman , H. Tachibana , K. Takahashi , M. Takeda , R. Takeishi , A. Taketa , M. Takita , Y. Tameda , K. Tanaka , M. Tanaka , M. Teramoto , S. B. Thomas , G. B. Thomson , P. Tinyakov , I. Tkachev , T. Tomida , S. Troitsky , Y. Tsunesada , S. Udo , F. R. Urban , M. Vrábel , D. Warren , K. Yamazaki , Y. Zhezher , Z. Zundel , J. Zvirzdin

Analysis of the experimental data on cosmic ray spectra in the framework of the proposed model with two types of sources leads to conclusion, that sources with particle generation spectral exponent $p\sim 2.85$ give the major contribution…

Astrophysics · Physics 2008-11-26 A. A. Lagutin , A. G. Tyumentsev , A. V. Yushkov

The paper discusses an approach that made it possible to estimate the distance to the nearest pevatrons, which form a knee in the spectrum of the cosmic ray nucleon component of about $4$ PeV. It is based on the spectra of nucleons and…

High Energy Astrophysical Phenomena · Physics 2025-09-09 A. A. Lagutin , N. V. Volkov

Experimental complex (EC) NEVOD includes a number of unique experimental facilities for studies of main components of cosmic rays on the Earth's surface. The complex is used for the basic research of CR flux characteristics and their…

The hypothesis that the electron neutrino is a tachyon with |m|=sqrt(-m^2) = 0.5 eV/c^2 is consistent with certain properties of the cosmic ray spectrum, including: the existence of a change in power law (the "knee") at E = 10^15 eV, the…

Astrophysics · Physics 2009-10-30 R. Ehrlich

A spectrum of cosmic rays within energy range 10^15 - 3x10^17 eV was derived from the data of the small Cherenkov setup, which is a part of the Yakutsk complex EAS array. In this, work a new series of observation is covered. These…

High Energy Astrophysical Phenomena · Physics 2015-06-03 S. P. Knurenko , A. Sabourov

The energy spectra for five elemental groups (p, He, C, Si, Fe) of cosmic rays, are simulated. Calculations are based on an analysis of superposition of few cosmic ray sources (Supernovae of different types) and principles of diffusive…

High Energy Astrophysical Phenomena · Physics 2011-04-20 Igor Lebedev

The energy spectrum of cosmic rays in the range 10^15 eV to 6*10^19 eV has been studied using the air Cherenkov light detectors of the Yakutsk array. The total flux of photons produced by relativistic electrons (including positrons as well,…

High Energy Astrophysical Phenomena · Physics 2009-08-05 A. A. Ivanov , S. P. Knurenko , I. Ye. Sleptsov

The origin of cosmic rays remains an unresolved fundamental problem in astrophysics. The synergy of multiple observational probes, including the energy spectra, the mass composition, and anisotropy is a viable way to jointly uncover this…

High Energy Astrophysical Phenomena · Physics 2026-05-27 Bing-Qiang Qiao , Qiang Yuan , Yi-Qing Guo

A new type of cosmic-ray experiment is under construction in the Pyh\"asalmi mine in the underground laboratory of the University of Oulu, Finland. It aims to study the composition of cosmic rays at and above the knee region. The…

This report presents a draft of a new detector designed to determine the chemical composition of primary cosmic rays based on the characteristics of the angular distribution of Cherenkov light from EAS. The installation, consisting of…

About 20 years ago we published the data concerning some peculiarities of the behavior of cosmic radiation EAS hadron component spectra. The results pointed to the possible existence in the interstellar space of the background of weakly…

High Energy Astrophysical Phenomena · Physics 2018-12-20 T. T. Barnaveli , N. A. Eristavi , I. V. Khaldeeva

The knee-like structure around 4 PeV is the most striking feature in the cosmic ray energy spectrum, whose origin remains enigmatic. We propose a novel concept of the total logarithmic mass energy spectrum to characterize the knee, taking…

High Energy Astrophysical Phenomena · Physics 2024-11-22 Huihai He , Hengying Zhang , Qinyi Cheng , Lingling Ma , Cunfeng Feng