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Related papers: Progenitor model of Cosmic Ray knee

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The most recent experimental results on the cosmic ray composition and energy spectrum above 1 TeV are reviewed and discussed. All data agree on the presence of the so-called ``knee'' at an energy E(knee) = 3-4 PeV; the knee is seen in all…

Astrophysics · Physics 2009-10-31 A. Castellina

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

Cosmic rays around the so-called knee in the spectrum at around PeV primary energy are generally galactic in origin. Observations on the form of their energy spectrum and their mass composition are fundamental tools to understand the…

High Energy Astrophysical Phenomena · Physics 2025-09-01 Donghwa Kang , Andreas Haungs

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

Recent progress in cosmic ray physics covering the energy range from about 10^{14} eV to 10^{19} eV is reviewed. The most prominent features of the energy spectrum are the so called `knee' at E ~ 3 * 10^{15} eV and the `ankle' at few…

Astrophysics · Physics 2008-11-26 Karl-Heinz Kampert

I develop a theory to account for the cosmic ray spectrum. The essential assumption is that, due to fast convective motions, the free mean path perpendicular to the magnetic field is independent of energy and has the scale of the thickness…

Astrophysics · Physics 2007-05-23 Peter L. Biermann

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

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 recent results on extensive air showers allow us to conclude that: a) the knee has an astrophysical origin;…

Astrophysics · Physics 2007-05-23 A. D. Erlykin , A. W. Wolfendale

In a comprehensive model of Cosmic Rays (CRs) proposed a decade ago, the energies of the spectral "knees" of the various CR species were predicted to be proportional to mass, rather than charge. The model also predicts the knees to occur at…

High Energy Physics - Phenomenology · Physics 2019-02-12 A. De Rújula

In this work we examine with the help of Monte Carlo simulation whether a consistent primary energy spectrum of cosmic rays emerges from both the experimentally observed total charged particles and muon size spectra of cosmic ray extensive…

High Energy Astrophysical Phenomena · Physics 2016-09-07 Biplab Bijay , Prabir Banik , Arunava Bhadra

Cosmic rays around the knee are generally believed to be of galactic origin. Observations on their energy spectrum and chemical composition are important for understanding the acceleration and propagation of these cosmic rays. In addition,…

High Energy Astrophysical Phenomena · Physics 2017-03-01 Donghwa Kang

A "knee" in the cosmic-ray spectrum, characterized by a sudden steepening of the spectral shape at $\sim 4$ PeV, may be interpreted either as a global feature of Galactic cosmic rays or as a local signature. In the former scenario,…

High Energy Astrophysical Phenomena · Physics 2026-02-27 Ke Fang , Francis Halzen

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

The differential energy spectrum of the cosmic radiation from solar modulation energies up to 5x10**19 eV is correctly predicted by a recent theory of the knee and ankle which uses only one normalization point. This remarkable quantitative…

High Energy Astrophysical Phenomena · Physics 2014-11-18 Antonio Codino , François Plouin

Primary cosmic ray particles above energies of about 100 TeV are investigated by large-area ground based detector installations, observing various components of the development of extensive air-showers (EAS). By such an indirect access to…

Astrophysics · Physics 2008-11-26 A. Haungs

The main purpose of this work is to find the causes of the break of the cosmic ray spectrum at an energy of 3 PeV, which is called the knee. The solution of the problem is associated with the determination of the nuclear composition of…

High Energy Astrophysical Phenomena · Physics 2022-09-28 S. B. Shaulov , V. A. Ryabov , S. E. Pyatovsky , A. L. Shepetov , V. V. Zhukov

An update of the status of the knee in the cosmic ray energy spectrum at 3-4 PeV is presented. We argue that the evidence in favour of the presence of a 'single source' is even stronger than before.

High Energy Physics - Phenomenology · Physics 2009-06-25 A. D. Erlykin , A. W. Wolfendale

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

We propose that the knee in the cosmic ray spectrum at energies E ~ 10^{15.5} eV is due to "new physics", namely to a channel in the high energy (~ TeV in the CM) proton interactions hitherto unaccounted for in estimating the energies of…

Astrophysics · Physics 2007-05-23 D. Kazanas , A. Nicolaidis

The origin of the prominent 'knee' in the cosmic ray energy spectrum at an energy of several PeV is still uncertain. A recent mechanism has shown promise, however; this involves particles from a very young pulsar interacting with the…

High Energy Astrophysical Phenomena · Physics 2015-05-20 Tadeusz Wibig , Arnold W. Wolfendale
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