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Related papers: From cosmic ray source to the Galactic pool

200 papers

The escape of cosmic rays from the Galaxy leads to a gradient in the cosmic ray pressure that acts as a force on the background plasma, in the direction opposite to the gravitational pull. If this force is large enough to win against…

High Energy Astrophysical Phenomena · Physics 2016-08-17 S. Recchia , P. Blasi , G. Morlino

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

In this paper, a probable interpretation of a remarkable fine structure of all particle spectra between the knee and the ankle, as well as a high content of heavy nuclei around 10^17 eV measured recently in Tunka-133 and KASCADE Grande…

High Energy Astrophysical Phenomena · Physics 2013-03-18 L. G. Sveshnikova , E. E. Korosteleva , L. A. Kuzmichev , V. A. Prosin , V. S. Ptuskin , O. N. Strelnikova

We have argued [J. Szabelski et al. (2002)] that the well-known `ankle' in the cosmic ray energy spectrum, at logE (eV) ~ 18.7-19.0, marks the transition from mainly Galactic sources at lower energies to mainly extragalactic above.…

Astrophysics · Physics 2007-05-23 Tadeusz Wibig , Arnold W. Wolfendale

Cosmic rays represent one of the most important energy transformation processes of the universe. They bring information about the surrounding universe, our galaxy, and very probably also the extragalactic space, at least at the highest…

High Energy Astrophysical Phenomena · Physics 2022-06-07 G. Di Sciascio , INFN - Roma Tor Vergata

We consider a cosmic ray spectrum that is a power law in momentum down to a cutoff and derive a lower cutoff corresponding to $E_{kin} \sim (30-60)$ MeV from the observed ionization rates in nearby diffuse clouds. While the real spectra of…

Astrophysics · Physics 2015-06-24 Biman B. Nath , Peter L. Biermann

We evaluate the current status of supernova remnants as the sources of Galactic cosmic rays. We summarize observations of supernova remnants, covering the whole electromagnetic spectrum and describe what these obser- vations tell us about…

High Energy Astrophysical Phenomena · Physics 2015-06-05 E. A. Helder , J. Vink , A. M. Bykov , Y. Ohira , J. C. Raymond , R. Terrier

In this article, momentum transport generated by the combined effects of pitch-angle diffusion and Background Flow Velocity Inhomogeneities (BFVIs) is proposed to obtain a cosmic rays acceleration mechanism, starting from the well-known…

High Energy Astrophysical Phenomena · Physics 2025-05-28 J. -F. Wang , G. Qin

A rapidly growing amount of evidences, mostly coming from the recent gamma-ray observations of Galactic supernova remnants (SNRs), is seriously challenging our understanding of how particles are accelerated at fast shocks. The cosmic-ray…

High Energy Astrophysical Phenomena · Physics 2015-06-05 Damiano Caprioli

The role of nearby galactic sources, the supernova remnants, in formation of observed energy spectrum and anisotropy of high-energy cosmic rays is studied. The list of these sources is made up based on radio, X-ray and gamma-ray catalogues.…

High Energy Astrophysical Phenomena · Physics 2013-12-20 L. G. Sveshnikova , O. N. Strelnikova , V. S. Ptuskin

The description of the transport of cosmic rays in magnetized media is central to both acceleration and propagation of these particles in our Galaxy and outside. The investigation of the process of particle acceleration, especially at shock…

High Energy Astrophysical Phenomena · Physics 2017-03-21 P. Blasi

Cosmic rays may have contributed to the start of life on Earth. Here, we investigate the evolution of the Galactic cosmic ray spectrum at Earth from ages $t = 0.6-6.0\,$Gyr. We use a 1D cosmic ray transport model and a 1.5D stellar wind…

Solar and Stellar Astrophysics · Physics 2020-10-28 D. Rodgers-Lee , A. A. Vidotto , A. M. Taylor , P. B. Rimmer , T. P. Downes

We analyse the results of recent measurements of nonthermal emission from individual supernova remnants (SNRs) and their correspondence to the nonlinear kinetic theory of cosmic ray (CR) acceleration in SNRs. It is shown that the theory…

Astrophysics · Physics 2008-11-26 E. G. Berezhko

The origin of Galactic cosmic rays (with energies up to 10^15 eV) remains unclear, though it is widely believed that they originate in the shock waves of expanding supernova remnants. Currently the best way to investigate their acceleration…

Astrophysics · Physics 2012-08-27 The H. E. S. S. Collaboration , : , F. A. Aharonian

Recent measurements revealed the presence of several features in the cosmic ray spectrum. In particular, the proton and helium spectra exhibit a spectral hardening at $\approx$ 300 GV and a spectral steeping at $\approx$ 15 TV, followed by…

High Energy Astrophysical Phenomena · Physics 2024-12-04 Sarah Recchia , Stefano Gabici

The maximum cosmic ray energy achievable by acceleration by a relativistic blast wave is derived. It is shown that forward shocks from long GRB in the interstellar medium are powerful enough to produce the Galactic cosmic-ray component up…

High Energy Astrophysical Phenomena · Physics 2015-05-27 David Eichler , Martin Pohl

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

One century ago Viktor Hess carried out several balloon flights that led him to conclude that the penetrating radiation responsible for the discharge of electroscopes was of extraterrestrial origin. One century from the discovery of this…

High Energy Astrophysical Phenomena · Physics 2015-06-18 Pasquale Blasi

The present paper deals with calculations based on a standard model of cosmic ray acceleration in Supernova remnants (SNR) and on the latest astronomical data concerning the variety in Supernovae types, energies as well as the sites of…

Astrophysics · Physics 2009-11-07 Lyubov G. Sveshnikova

We derive constraints that must be satisfied by the sources of ~10^{15} to ~10^{18} eV cosmic rays, under the assumption that the sources are Galactic. We show that while these constraints are not satisfied by ordinary supernovae (SNe),…

Astrophysics · Physics 2010-11-11 R. Budnik , B. Katz , A. MacFadyen , E. Waxman
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