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Related papers: Surprising Results from Cosmic Rays

200 papers

Cosmic rays are energetic charged particles from extraterrestrial sources, with the highest energy events thought to come from extragalactic sources. Their arrival is infrequent, so detection requires instruments with large collecting…

High Energy Astrophysical Phenomena · Physics 2023-11-27 Telescope Array Collaboration

We argue that the data published by the Pierre Auger Collaboration (arXiv:0711.2256) disfavor at 99% confidence level their hypothesis that most of the highest-energy cosmic rays are protons from nearby astrophysical sources, either Active…

Astrophysics · Physics 2009-06-19 Dmitry Gorbunov , Peter Tinyakov , Igor Tkachev , Sergey Troitsky

The origin of the most energetic cosmic ray particles is one of the most important open problems in astrophysics. Despite a big experimental effort done in the past years, the sources of these very energetic particles remain unidentified.…

High Energy Astrophysical Phenomena · Physics 2015-06-17 A. D. Supanitsky , G. Medina-Tanco

Several phenomena in high energy astrophysics have been recently related to clusters of galaxies and to cosmic ray interactions occurring inside these structures. In many of these phenomena the observable effects depend on the energy…

Astrophysics · Physics 2009-10-30 P. Blasi , S. Colafrancesco

In the past few years, cosmic-rays beyond the GZK cut-off ($E > 5 \times 10^{19}$ eV) have been detected by leading collaborations such as Pierre Auger Observatory. Such observations raise many questions as to how such energies can be…

The problem of the origin of cosmic rays in the shocks produced by supernova explosions at energies below the so called 'knee' (at ~3*10$^6$ GeV) in the energy spectrum is addressed, with special attention to the propagation of the…

Astrophysics · Physics 2008-11-26 A. D. Erlykin , A. A. Lagutin , A. W. Wolfendale

Two processes of matter creation after inflation: 1) gravitational creation of superheavy (quasi)stable particles, and 2) non-thermal phase transitions leading to formation of topological defects, may be relevant to the resolution of the…

High Energy Physics - Phenomenology · Physics 2009-10-31 I. I. Tkachev

A review of the status of the knowledge in the field of High-energy cosmic particles is presented. The spectrum, arrival direction distribution and composition measurements are summarized, together with some implications for the…

High Energy Astrophysical Phenomena · Physics 2020-12-21 Silvia Mollerach

Fluctuations in high-redshift cosmic 21-cm radiation provide a new window for observing unconventional effects of high-energy physics in the primordial spectrum of density perturbations. In scenarios for which the initial state prior to…

High Energy Physics - Theory · Physics 2008-11-26 Matthew Kleban , Kris Sigurdson , Ian Swanson

We give a summary of the theoretical attempts to make sense of the observational data concerning the highest energy cosmic rays, (E > 3x10^{19} eV).

High Energy Physics - Phenomenology · Physics 2015-06-25 S. Kovesi-Domokos , G. Domokos

We examine the question of the origin of the Galactic cosmic-rays (GCRs) in the light of the data available at the highest energy end of the spectrum. We argue that the data of the Pierre Auger Observatory and of the KASCADE-Grande…

High Energy Astrophysical Phenomena · Physics 2015-06-23 Etienne Parizot

Ultrahigh energy cosmic rays are the most energetic of any subatomic particles ever observed in nature. The quest for their mysterious origin is currently a major scientific challenge. Here we explore the possibility that these particles…

High Energy Astrophysical Phenomena · Physics 2018-05-09 Reda Attallah , Dallel Bouchachi

We review the main experimental evidences on ultra high energy cosmic rays and their implications in the physics of these extremely energetic particles, also in connection with dark matter and cosmology. We discuss the basis of theoretical…

High Energy Astrophysical Phenomena · Physics 2023-03-01 Roberto Aloisio

A review of several analyses is presented that forces the conclusion that the mass composition of the highest-energy cosmic rays is not proton-dominated. This deduction, combined with the use of a modern hadronic interaction model, should…

High Energy Astrophysical Phenomena · Physics 2025-12-10 A A Watson

One of the models recently proposed to explain the origin of the ultra high energy cosmic rays assumes that these particles may be accelerated by the electromotive force around presently inactive quasar remnants. We study predictions for…

Astrophysics · Physics 2007-05-23 C. Isola , G. Sigl , G. Bertone

The general features of the cosmic-ray spectrum have been known for a long time. Although the basic approaches to understanding cosmic-ray propagation and acceleration have also been well understood for many years, there are several…

Astrophysics · Physics 2007-05-23 Thomas K. Gaisser

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

We present arguments aiming to reconcile the apparently contradictory results concerning the chemical composition of cosmic rays of highest energy, coming recently from Auger and HiRes collaborations. In particular, we argue that the energy…

High Energy Astrophysical Phenomena · Physics 2011-11-28 Grzegorz Wilk , Zbigniew Wlodarczyk

We discuss the region of transition between galactic and extragalactic cosmic rays. The exact shapes and compositions of these two components contains information about important parameters of powerful astrophysical sources and the…

Astrophysics · Physics 2008-11-26 Todor Stanev

Cosmic rays with energies above $10^{19}$ eV, observed in 1999-2004 by the High Resolution Fly's Eye (HiRes) experiment in the stereoscopic mode, were found to correlate with directions to distant BL Lac type objects (BL Lacs), suggesting…

High Energy Astrophysical Phenomena · Physics 2024-01-24 M. A. Kudenko , S. V. Troitsky