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Related papers: The origin of galactic cosmic rays

200 papers

The origin of cosmic rays is one of the major unresolved astrophysical questions. In particular, the highest energy cosmic rays observed possess macroscopic energies and their origin is likely to be associated with the most energetic…

Astrophysics · Physics 2007-05-23 Guenter Sigl

Cosmic ray nuclei, cosmic ray electrons with energy above a few GeV, and the diffuse gamma-ray background radiation (GBR) above a few MeV, presumed to be extragalactic, could all have their origin or residence in our galaxy and its halo.…

Astrophysics · Physics 2007-05-23 Arnon Dar , A. De Rújula , Nikos Antoniou

A model is proposed for the origin of cosmic rays (CRs) from ~10^14 eV to the highest energies, >10^20 eV. Gamma-Ray Bursts (GRBs) are assumed to inject CR protons and ions into the interstellar medium of star-forming galaxies--including…

Astrophysics · Physics 2008-11-26 Stuart D. Wick , Charles D. Dermer , Armen Atoyan

The origin of Galactic cosmic rays (GCRs) remains a mystery after more than one century of their discovery. The diffusive propagation of charged particles in the turbulent Galactic magnetic field makes us unable to trace back to their…

High Energy Astrophysical Phenomena · Physics 2019-10-22 Wei Liu , Yi-Qing Guo , Qiang Yuan

Supernova remnants (SNRs) are the prime candidates for the acceleration of the Galactic Cosmic Rays. Tracers for interactions of Cosmic Rays with ambient material are gamma rays at TeV energies, which can be observed with ground based…

High Energy Astrophysical Phenomena · Physics 2019-08-14 Nukri Komin

Determining the spatial distribution of Galactic cosmic rays (CRs) is fundamental to understand how these particles propagate in interstellar space and to infer their source spectra. The most sensitive method of studying this problem is…

High Energy Astrophysical Phenomena · Physics 2025-09-26 Paolo Lipari , Silvia Vernetto

Supernova remnants (SNRs) have long been suspected to be the primary sources of Galactic cosmic rays. Over the past decades, great strides have been made in the modelling of particle acceleration, magnetic field amplification, and escape…

High Energy Astrophysical Phenomena · Physics 2025-09-25 Anton Stall , Chun Khai Loo , Philipp Mertsch

Motivated by recent measurements of the major components of the cosmic radiation around 10 TeV/nucleon and above, we discuss the phenomenology of a model in which there are two distinct kinds of cosmic ray accelerators in the galaxy.…

Astrophysics · Physics 2011-05-12 Peter L. Biermann , T. K. Gaisser , Todor Stanev

Although cosmic rays were discovered 90 years ago, we do not know how and where they are accelerated. There is compelling evidence that the highest energy cosmic rays are extra-galactic -- they cannot be contained by our galaxy's magnetic…

Astrophysics · Physics 2009-11-07 F. Halzen

Recent observations provide compelling evidence that the bulk of the high energy cosmic rays (CRs) and gamma-ray bursts (GRBs) are co-produced by highly relativistic jets of plasmoids of stellar matter. These jets are launched by fall back…

High Energy Astrophysical Phenomena · Physics 2024-02-06 Shlomo Dado , Arnon Dar

Understanding the origins of ultrahigh energy cosmic rays (UHECRs) - which reach energies in excess of $10^{20}~{\rm eV}$ - stretches particle acceleration physics to its very limits. In this review, we discuss how such energies can be…

High Energy Astrophysical Phenomena · Physics 2023-01-10 James H. Matthews , Andrew M. Taylor

Cosmic-ray interactions with interstellar gas and photons produce diffuse gamma-ray emission. In this talk we will review the current understanding of this diffuse emission and its relationship to the problem of the origin of cosmic rays.…

Astrophysics · Physics 2009-11-07 S. W. Digel , S. D. Hunter , I. V. Moskalenko , J. F. Ormes , M. Pohl

Cosmic rays (CRs) are charged particles that arrive at Earth isotropically from all directions and interact with the atmosphere. The presence of a spectral knee feature seen in the CR spectrum at $\sim$3 PeV energies is an evidence that…

High Energy Astrophysical Phenomena · Physics 2023-05-23 E. O. Angüner

There is evidence that cosmic rays were present in galaxies at moderately high redshift. This suggests that magnetic fields were also present. If cosmic rays and magnetic fields must always be close to equipartition, as they are to an order…

Astrophysics · Physics 2009-11-07 Ellen G. Zweibel

We propose a new hypothesis for the origin of non-solar hadronic cosmic rays (CRs) at all energies: Highly relativistic, narrowly collimated jets from the birth or collapse of neutron stars (NSs) in our Galaxy accelerate ambient disk and…

Astrophysics · Physics 2007-05-23 R. Plaga , O. C. de Jager , A. Dar

A short overview is presented of current issues concerning the production and evolution of Li, Be and B in the Milky Way. In particular, the observed "primary-like" evolution of Be is re-assessed in the light of a novel idea: it is argued…

Astrophysics of Galaxies · Physics 2015-05-18 Nikos Prantzos

We present a theory of non-solar cosmic rays (CRs) in which the bulk of their observed flux is due to a single type of CR source at all energies. The total luminosity of the Galaxy, the broken power-law spectra with their observed slopes,…

High Energy Physics - Phenomenology · Physics 2009-09-29 Arnon Dar , Alvaro De Rujula

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

A new conceptual approach for examining the origin of cosmic rays is developed by considering the characteristics of particle trajectory distributions in four-dimensional Euclidean space-time. Transformation of an isotropic distribution…

General Physics · Physics 2015-06-26 C. L. Herzenberg

It is shown that the acceleration of particles by a powerful relativistic jet associated with the activity of a supermassive black hole in the Galactic center several million years ago may explain the observed cosmic ray spectrum at…

High Energy Astrophysical Phenomena · Physics 2024-06-05 V. N. Zirakashvili , V. S. Ptuskin , S. I. Rogovaya
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