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We revisit the idea that the Galactic center (GC) is the dominant source of Galactic cosmic rays (GCRs), based on a series of new observational evidence. A unified model is proposed to explain the new phenomena of GCRs and $\gamma$-rays…

High Energy Astrophysical Phenomena · Physics 2013-01-24 Yiqing Guo , Zhaoyang Feng , Qiang Yuan , Cheng Liu , Hongbo Hu

The suggestion has been made that the energy spectrum from point sources such as AGN (Active Galactic Nuclei) and GBHC (Galactic Black Hole Candidates) is universal, irrespective of the nature of the emitted particles. A comparison of the…

Astrophysics · Physics 2009-10-22 Yukio Tomozawa

The energy losses and spectra of Ultra High Energy Cosmic Rays (UHECR) are calculated for protons as primary particles. The attention is given to the energy losses due to electron-positron production in collisions with the microwave 2.73 K…

High Energy Physics - Phenomenology · Physics 2007-05-23 V. Berezinsky , A. Z. Gazizov , S. I. Grigorieva

The problem in identifying the sites of origin of Galactic Cosmic Rays (CRs) is reviewed. Recent observational evidence from very-high energy (VHE, energies above 100 GeV) gamma-ray measurements is in contradiction with the surmise that…

Astrophysics · Physics 2007-05-23 R. Plaga

We find the general requirements, set by classical electrodynamics, to the sources of extremely high-energy cosmic rays (EHECRs). It is shown that the parameters of EHECR accelerators are strongly limited not only by the particle…

The Ultra-high energy cosmic ray energy spectrum summarized by the AGASA collaboration indicates clearly that the cosmic ray spectrum extends well beyond the Greisen-Zatsepin-Kuzmin (GZK) cut-off at \sim 5 x 10^19 eV. Furthermore, despite…

Astrophysics · Physics 2007-05-23 Gustavo Medina Tanco

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 composition of the overall spectrum of cosmic rays (CRs) is studied under the assumption that ultra high energy CRs above the energy 10^{17} eV are produced at the shock created by the expanding cocoons around active galactic nuclei…

High Energy Astrophysical Phenomena · Physics 2011-02-11 E. G. Berezhko

In many models, the sources of ultra-high-energy cosmic rays (UHECRs) are assumed to accelerate particles to the same maximum energy. Motivated by the fact that candidate astrophysical accelerators exhibit a vast diversity in terms of their…

High Energy Astrophysical Phenomena · Physics 2023-05-29 Domenik Ehlert , Foteini Oikonomou , Michael Unger

The flux of Ultra High Energy Cosmic Rays (UHECRs) at $E>10^{18.5}$ eV is believed to arise in plasma shock environments in extragalactic sources. In this paper, we present a systematic study of particle acceleration by relativistic shocks,…

Astrophysics · Physics 2009-11-13 Athina Meli , Julia K. Becker , John J. Quenby

The Galactic cosmic ray spectrum is a remarkably straight power law. Our current understanding is that the dominant sources that accelerate cosmic rays up to the knee ($3 \times 10^{15}$ eV) or perhaps even the ankle ($3 \times 10^{18}$…

High Energy Astrophysical Phenomena · Physics 2015-06-17 K. M. Schure , A. R. Bell

Despite significant progress over more than 100 years, no accelerator has been unambiguously identified as the source of the locally measured flux of cosmic rays. High-energy electrons and positrons are of particular importance in the…

High Energy Astrophysical Phenomena · Physics 2018-11-30 Philipp Mertsch

It has been suggested that cosmological gamma-ray bursts (GRBs) can produce the observed flux of cosmic rays at the highest energies. However, recent studies of GRBs indicate that their redshift distribution likely follows that of the…

Astrophysics · Physics 2009-10-31 S. T. Scully , F. W. Stecker

The arguments suggesting an association between the sources of cosmological gamma-ray bursts (GRBs) and the sources of ultra-high energy cosmic rays (UHECRs) are presented. Recent GRB and UHECR observations are shown to strengthen these…

Astrophysics · Physics 2009-11-10 E. Waxman

An observation-based Galactic Cosmic Ray (GCR) spectral model for heavy nuclei is developed. Zhao and Qin (J. Geophys. Res. Space Phys.118, 1837(2013)) proposed an empirical elemental GCR spectra model for nuclear charge 5-28 over the…

Instrumentation and Methods for Astrophysics · Physics 2020-05-05 Shuai Fu , LingLing Zhao , Gary P. Zank , Miao Wang , Yong Jiang

We aim to explain in a unified way the experimental data on ultrahigh energy cosmic rays (UHECR) and neutrinos, using a single source class and obeying limits on the extragalactic diffuse gamma-ray background (EGRB). If UHECRs only interact…

High Energy Astrophysical Phenomena · Physics 2017-10-11 M. Kachelriess , O. Kalashev , S. Ostapchenko , D. V. Semikoz

Spectra at the Earth of ultra-high energy cosmic rays (UHECR) from Seyfert nuclei with red shifts z<=0.0092 and from Blue Lacertae objects (BL Lac's) are calculated. The spectra are compared with the experimental data. It is shown that in…

Astrophysics · Physics 2007-05-23 A. V. Uryson

Context. Recent observations of unexpected structures in the Galactic Cosmic Ray (GCR) spectrum and composition, as well as growing evidence for episodes of intense dynamical activity in the inner regions of the Galaxy, call for an…

High Energy Astrophysical Phenomena · Physics 2018-11-07 Etienne Jaupart , Etienne Parizot , Denis Allard

We discuss the GZK horizon of protons and present a method to constrain the injection spectrum of ultrahigh energy cosmic rays (UHECRs) from supposedly identified extragalactic sources. This method can be applied even when only one or two…

Astrophysics · Physics 2009-07-17 M. Kachelriess , E. Parizot , D. V. Semikoz

We discuss a scenario in which the highest energy cosmic rays (CR's) and cosmological $\gamma$-ray bursts (GRB's) have a common origin. This scenario is consistent with the observed CR flux above $10^{20}\text{eV}$, provided that each burst…

Astrophysics · Physics 2009-10-28 Eli Waxman