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Related papers: Models and phenomenology

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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 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

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

All astrophysical explanations of the knee in cosmic ray spectrum accept the hypothesis of its existence {\it a priori} without any doubt. But, there exist experimental evidences against this hypothesis. Experimental data on the knee in…

Astrophysics · Physics 2015-06-24 Yuri V. Stenkin

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

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

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

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

Examples of the power law spectra observations in the Nature are given. It is shown that the observed meteoroid mass spectrum is very similar to the observed cosmic ray energy spectrum. It is concluded that the "knees" observed in both…

Astrophysics · Physics 2007-05-23 Yuri V. Stenkin

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

The search for a theory of the origin of cosmic rays that may be considered as a standard, agreeable model is still ongoing. On one hand, much circumstantial evidence exists of the fact that supernovae in our Galaxy play a crucial role in…

High Energy Astrophysical Phenomena · Physics 2015-06-23 P. Blasi

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

Two approaches to the old problem of the so-called "knee" in cosmic ray spectrum are compared with the existing experimental data. It is shown that "standard astrophysical model" of the knee is not supported by some experimental data, while…

Astrophysics · Physics 2016-08-30 Yuri V. Stenkin

An overview is given on results from direct and indirect measurements of galactic cosmic rays. Their implications on the contemporary understanding of the origin of cosmic rays and the knee in their energy spectrum are discussed.

Astrophysics · Physics 2009-11-10 Joerg R. Hoerandel

The knee phenomenon of the cosmic ray spectrum, which plays an important role in studying the acceleration mechanism of cosmic rays, is still an unsolved mystery. We try to reconcile the knee spectra measured by ARGO-YBJ and Tibet-III. A…

High Energy Astrophysical Phenomena · Physics 2015-10-22 Yi Zhao , Huan-Yu Jia , Feng-Rong Zhu

Several kinds of measurements are combined in an attempt to obtain a consistent estimate of the spectrum and composition of the primary cosmic radiation through the knee region. Assuming that the knee is a signal of the high-energy end of a…

Astrophysics · Physics 2016-11-09 Thomas K. Gaisser

The knee in the all-particle energy spectrum is scrutinized with a phenomenological model, named poly-gonato model, linking results from direct and indirect measurements. For this purpose, recent results from direct and indirect…

Astrophysics · Physics 2009-11-07 J. R. Hoerandel

Primary energy spectrum of cosmic rays exhibits a knee at about $3$ PeV where a change in the spectral index occurs. Despite many efforts the origin of such a feature of the spectrum is not satisfactorily solved yet. Here it is proposed…

High Energy Astrophysical Phenomena · Physics 2017-02-15 Biplab Bijay , Arunava Bhadra

An attempt to construct a phenomenological theory of earthquakes is being undertaken by a small research team, which includes the author. We have only taken the first steps towards goal, but the results already obtained convincingly…

Geophysics · Physics 2025-10-31 A. V. Guglielmi

Two structures in the all-particle energy spectrum of cosmic rays, the knee at 4 PeV and the second knee around 400 PeV are proposed to be explained by a phenomenological model, the poly gonato model, connecting direct and indirect…

Astrophysics · Physics 2016-08-30 Joerg R. Hoerandel , N. N. Kalmykov , A. V. Timokhin
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