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The origin of the highest energy cosmic rays represents one of the most conspicuous enigmas of modern astrophysics, in spite of gigantic experimental efforts in the past fifty years, and of active theoretical research. The past decade has…

High Energy Astrophysical Phenomena · Physics 2015-06-11 M. Lemoine

We give a brief (and highly incomplete) overview of the current experimental and theoretical status of high energy cosmic rays and their secondary gamma-rays and neutrinos. We focus on the role of large scale magnetic fields and on…

Astrophysics · Physics 2009-11-11 Guenter Sigl

Significant progress has been made over the past decades towards unveiling the sources of the most energetic particles in nature, the ultra-high-energy cosmic rays (UHECRs). Despite these advancements, the exact astrophysical sites capable…

High Energy Astrophysical Phenomena · Physics 2025-04-03 Rafael Alves Batista

The origin of highest energy cosmic rays is yet unknown. An appealing possibility is the so-called Z-burst scenario, in which a large fraction of these cosmic rays are decay products of Z bosons produced in the scattering of ultrahigh…

High Energy Physics - Phenomenology · Physics 2007-05-23 Z. Fodor , S. D. Katz , A. Ringwald

Reasons for the current interest in cosmic rays above 10^19 eV are described. The latest results on the energy spectrum, arrival direction distribution and mass composition of cosmic rays are reviewed, including data that were reported…

Astrophysics · Physics 2007-05-23 A. A. Watson

We study the effects that the diffusion of the cosmic rays in the magnetic field of the Local Supercluster can have on the spectrum of a nearby extragalactic source at ultrahigh energies. We find that the strong enhancement of the flux…

High Energy Astrophysical Phenomena · Physics 2019-05-22 Silvia Mollerach , Esteban Roulet

The understanding of the nature of ultra-high-energy cosmic rays is one of the most intriguing open questions for current and future observatories. These particles are expected to be accelerated in extragalactic sources. Because of their…

High Energy Astrophysical Phenomena · Physics 2016-12-28 Mariangela Settimo

Under the hypothesis that Gamma Ray Burst (GRB) might be responsible for the origin of Ultra High Energy Cosmic Ray (UHECR), we propose a two component (galactic and extra-galactic) model for the UHECR origin. The model is based on two…

Astrophysics · Physics 2007-05-23 C. E. Navia , C. R. A. Augusto , K. H. Tsui

The cosmological gamma-ray burst (GRB) model for the production of ultra- high energy cosmic rays is described, and the current observational evidence which support it discussed. Several predictions of the model are presented, which would…

Astrophysics · Physics 2007-05-23 Eli Waxman

The propagation trajectories of ultra-high-energy cosmic rays (UHECRs) are inevitably affected by Galactic magnetic field (GMF). Because of the inevitability, the importance of the studies of the propagation in GMF have increased to…

High Energy Astrophysical Phenomena · Physics 2015-05-27 Hajime Takami

Ultra high energy cosmic rays have been see coming from the direction of the local cosmic void. We use this fact to argue that at least some of these these cosmic rays are relatively light magnetic monopoles and that their relative fraction…

High Energy Physics - Phenomenology · Physics 2026-04-24 Michael J. Padgett , Thomas W. Kephart

This is a written version of a series of lectures aimed at graduate students in astrophysics/particle theory/particle experiment. In the first part, we explain the important progress made in recent years towards understanding the…

High Energy Physics - Phenomenology · Physics 2015-03-19 Luis Alfredo Anchordoqui

The present white paper is submitted as part of the "Snowmass" process to help inform the long-term plans of the United States Department of Energy and the National Science Foundation for high-energy physics. It summarizes the science…

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

We explore scenarios where the highest energy cosmic rays are produced by new particle physics near the grand unification scale. Using detailed numerical simulations of extragalactic nucleon, gamma-ray, and neutrino propagation, we show the…

High Energy Physics - Phenomenology · Physics 2009-10-31 Guenter Sigl , Sangjin Lee , Pijushpani Bhattacharjee , Shigeru Yoshida

Cosmic rays accelerated to ultra-high energies (E>4x10^19 eV) in electric fields in accretion discs around supermassive black holes are discussed. Particle injection spectra are assumed to be harder than those formed in acceleration on…

High Energy Astrophysical Phenomena · Physics 2020-01-08 A. Uryson

The search for the origin of cosmic rays is a quest of almost a hundred years. A recent theoretical proposal gives quantitative predictions, which can be tested with data. Specifically, it has been suggested, that all cosmic rays can be…

Astrophysics · Physics 2016-08-30 Peter L. Biermann

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

The observation of neutrinos from cosmic accelerators will be revolutionary. High energy neutrinos are closely connected to ultrahigh energy cosmic rays and their sources. Cosmic ray sources are likely to produce neutrinos and the…

High Energy Astrophysical Phenomena · Physics 2015-05-27 Angela V. Olinto , Kumiko Kotera , Denis Allard

Ultra high energy cosmic ray events presently show a spectrum, which we interpret here as galactic cosmic rays due to a starburst in the radio galaxy Cen A pushed up in energy by the shock of a relativistic jet. The knee feature and the…

High Energy Astrophysical Phenomena · Physics 2010-11-02 P. L. Biermann , J. K. Becker , L. Caramete , L. A. Gergely , I. C. Maris , A. Meli , V. de Souza , T. Stanev
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