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Related papers: Galactic Ultra-High-Energy Cosmic Rays

200 papers

The origin of cosmic rays holds still many mysteries hundred years after they were first discovered. Supernova remnants have for long been the most likely sources of Galactic cosmic rays. I discuss here some recent evidence that suggests…

High Energy Astrophysical Phenomena · Physics 2012-06-13 Jacco Vink

Cosmic ray particles with energies in excess of 10**(20) eV have been detected. The sources as well as the physical mechanism(s) responsible for endowing cosmic ray particles with such enormous energies are unknown. This report gives a…

Astrophysics · Physics 2014-10-13 Pijushpani Bhattacharjee , Guenter Sigl

Ultra High Energy Cosmic Rays, UHECR, are charged particles with energies between $\sim10^{18}\,{\rm eV}$ and $\sim3\times10^{20}\,{\rm eV}\sim50\,{\rm J}$. They exhibit fundamental physics at energies inaccessible to terrestrial…

High Energy Astrophysical Phenomena · Physics 2025-05-29 Noémie Globus , Roger Blandford

Two extreme events in the universe, fast radio bursts (FRBs) and cosmic rays (CRs), could be correlated, where FRBs with extreme field strength near their sources may contribute to CRs. This study investigates localized particle…

High Energy Astrophysical Phenomena · Physics 2026-05-01 Lin Yu , Tianxing Hu , Zhiyu Lei , Xiangyan An , Dong Wu , Suming Weng , Min Chen , Jie Zhang , Zhengming Sheng

Active galaxies and gamma ray bursts are the sources of the highest energy photons detected by astronomical telescopes. We speculate that they may be the sources of the highest energy cosmic rays. This makes them true proton accelerators,…

Astrophysics · Physics 2007-05-23 F. Halzen

We critically review the common belief that ultrahigh energy cosmic rays are protons or atomic nuclei with masses not exceeding that of iron. We find that heavier nuclei are indeed possible, and discuss possible sources and acceleration…

Astrophysics · Physics 2010-01-15 L. A. Anchordoqui , M. T. Dova , T. P. McCauley , T. Paul , S. Reucroft , J. D. Swain

The rate of terrestrial irradiation events by galactic gamma-ray bursts (GRBs) is estimated using recent standard-energy results. We assume that GRBs accelerate high-energy cosmic rays, and present results of three-dimensional simulations…

Astrophysics · Physics 2009-11-10 Charles D. Dermer , Jeremy M. Holmes

In this lecture I give an overview of shock acceleration, interactions of high energy cosmic rays with, and propagation through, the background radiation, and the resulting electron-photon cascade. I argue that while the origin of the…

Astrophysics · Physics 2007-05-23 R. J. Protheroe

Fast spinning magnetars are discussed as strong sources of high energy neutrinos. Pulsars may be born with a short rotation period of milliseconds with the magnetic field amplified through dynamo processes up to $\sim 10^{15}-10^{16} \rm…

Astrophysics · Physics 2016-08-30 Qinghuan Luo

Bright gamma-ray flares observed from sources far beyond our Galaxy are best explained if enormous amounts of energy are liberated by black holes. The highest-energy particles in nature--the ultra-high energy cosmic rays--cannot be confined…

High Energy Astrophysical Phenomena · Physics 2010-01-13 Charles D. Dermer , Govind Menon

We consider the galactic population of gamma-ray pulsars as possible sources of cosmic rays at and just above the ``knee'' in the observed cosmic ray spectrum at $10^{15}$--$10^{16}$ eV. We suggest that iron nuclei may be accelerated in the…

Astrophysics · Physics 2008-11-26 W. Bednarek , R. J. Protheroe

The origin of cosmic rays above the knee in the spectrum is an unsolved problem. We present a wind model in which interstellar gas flows along a non-rotating, expanding flux tube with a changing speed and cross-sectional area. Cosmic rays…

High Energy Astrophysical Phenomena · Physics 2023-08-09 Payel Mukhopadhyay , Enrico Peretti , Noemie Globus , Paul Simeon , Roger Blandford

We consider the possibility that the particles in the Ultra High Energy Cosmic Rays arriving to Earth might be neutrons instead of protons. We stress that in such case the argument for the GZK cutoff is weaker and that it is conceivable…

High Energy Physics - Phenomenology · Physics 2008-11-26 Adolfo De Unánue , Sarira Sahu , Daniel Sudarsky

The origin of the ultra high energy cosmic rays via annihilation of heavy stable, fermions "f", of the cosmological dark matter (DM) is studied. The particles in question are supposed to be created by the scalaron decays in $R^2$ modified…

High Energy Physics - Phenomenology · Physics 2024-05-22 E. V. Arbuzova , A. D. Dolgov , A. A. Nikitenko

The mechanism accelerating cosmic rays in the Milky Way Galaxy and galaxy clusters is identified and described. The acceleration of cosmic rays is a purely electrostatic process which operates up to the maximum energies of $10^{23}$ eV in…

High Energy Astrophysical Phenomena · Physics 2021-09-10 Antonio Codino

Observations of cosmic rays with energies above ~ 4 x 10^{10} GeV have inspired several speculative suggestions concerning their origin. The crucial question is whether or not the spectrum exhibits the expected `GZK cutoff' at this energy…

High Energy Physics - Phenomenology · Physics 2011-02-16 Subir Sarkar

Fast-spinning newborn pulsars are intriguing candidate sources of ultrahigh energy cosmic rays (UHECRs). The acceleration of particles with a given composition in a fraction of the extragalactic pulsar population can give a consistent…

High Energy Astrophysical Phenomena · Physics 2016-02-09 Ke Fang , Kumiko Kotera , Kohta Murase , Angela V. Olinto

The origin of highest energy cosmic rays (UHECR) is yet unknown. In order to understand their propagation we determine the probability that an ultrahigh energy (above 5\cdot 10^{19} eV) proton created at a distance r with energy E arrives…

High Energy Physics - Phenomenology · Physics 2007-05-23 Z. Fodor

The origin of the ultrahigh-energy (UHE) cosmic rays (CRs) from the second knee ($\sim6\times10^{17}$eV) above in the CR spectrum is still unknown. Recently, there has been growing evidence that a peculiar type of supernovae, called…

Astrophysics · Physics 2008-12-18 Xiang-Yu Wang , Soebur Razzaque , Peter Meszaros , Zi-Gao Dai

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