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Related papers: Cosmic Ray Astronomy

200 papers

The search for the origin of cosmic rays is as active as ever, mainly driven by new insights provided by recent pieces of observation. Much effort is being channelled in putting the so called supernova paradigm for the origin of galactic…

High Energy Astrophysical Phenomena · Physics 2018-05-02 R. Aloisio , P. Blasi , I. De Mitri , S. Petrera

The bulk of observed ultrahigh energy cosmic rays could be light or heavier elements, and originate from an either steady or transient population of sources. This leaves us with four general categories of sources. Energetic requirements set…

High Energy Astrophysical Phenomena · Physics 2016-11-21 Ke Fang , Kumiko Kotera

This is a summary of a series of lectures on the current experimental and theoretical status of our understanding of origin and nature of cosmic radiation. Specific focus is put on ultra-high energy cosmic radiation above ~10^17 eV,…

High Energy Astrophysical Phenomena · Physics 2012-02-03 Guenter Sigl

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

The origin of galactic cosmic rays is one of the most interesting unsolved problems in astroparticle physics. Experimentally, the problem is attacked by a multi-disciplinary effort, namely by direct measurements of cosmic rays above the…

Astrophysics · Physics 2008-11-26 Joerg R. Hoerandel

We briefly review the status of cosmic ray studies between $10^{14}$ eV and the highest observed energies, namely a few times $10^{20}$ eV. Because of the rather low incident fluxes in this energy range, the studies mostly rely on ground…

Astrophysics · Physics 2009-10-31 Murat Boratav , Alan A. Watson

The Global Cosmic-ray Observatory (GCOS) is a proposed large-scale observatory for studying ultra-high-energy cosmic particles, including ultra-high-energy cosmic rays (UHECRs), photons, and neutrinos. Its primary goal is to characterise…

High Energy Astrophysical Phenomena · Physics 2023-10-02 Rafael Alves Batista

This paper reviews recent progress in the field of direct measurements of Galactic cosmic rays. High-statistic measurements of cosmic ray energy spectra, chemical and isotopic composition, and the rare antimatter components have been made…

High Energy Astrophysical Phenomena · Physics 2023-02-02 Nicola Tomassetti

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

This article reviews the present status of high energy gamma-ray astronomy at energies above 30 MeV. Observations in the past decade using both space- and ground-based experiments have been primarily responsible for giving a tremendous…

Astrophysics · Physics 2010-12-03 R. Mukherjee

Recent measurements of ultra-high energy cosmic rays and neutrinos are briefly reviewed. With several new large scale observatories nearing completion or becoming fully operational only very recently, a large body of high quality and high…

High Energy Astrophysical Phenomena · Physics 2014-11-20 Karl-Heinz Kampert

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

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

Cosmic rays have been observed up to energies $10^8$ times larger than those of the best particle accelerators. Studies of astrophysical particles (hadrons, neutrinos and photons) at their highest observed energies have implications for…

Astrophysics · Physics 2009-11-10 F. W. Stecker

We will review the main physical aspects of Ultra High Energy Cosmic Rays. We will discuss in particular their propagation through astrophysical backgrounds, focusing on the latest experimental observations of HiRes, Telescope Array and…

High Energy Astrophysical Phenomena · Physics 2013-01-25 R. Aloisio

The article gives a brief overview, aimed at nonspecialists, about the goals and selected recent results of the detection of very-high energy gamma-rays (energies above 100 GeV) with ground based detectors. The stress is on the physics…

Astrophysics · Physics 2009-09-25 R. Plaga

In cosmic ray physics extensive progress has been made in recent years, both concerning theory and observation. The vast details in direct, indirect and secondary detections on the one hand provide the basis for a detailed modeling of the…

High Energy Astrophysical Phenomena · Physics 2020-05-11 Julia Becker Tjus , Lukas Merten

We address some current theoretical issues around ultra-high energy cosmic rays. We recall that scenarios producing more gamma-rays than cosmic rays up to high redshift can in general only provide a sub-dominant contribution to the…

Astrophysics · Physics 2007-05-23 Guenter Sigl

A cosmic ray detection system, consisting of standardized detector stations connected through the Internet, is described. The system can be used for detecting air showers that arrive over a wide area with correlated time. The data at each…

We discuss the production of ultra high energy neutrinos coming from the propagation of ultra high energy cosmic rays and in the framework of top-down models for the production of these extremely energetic particles. We show the importance…

High Energy Astrophysical Phenomena · Physics 2016-03-21 Roberto Aloisio
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