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Related papers: TOPOLOGICAL DEFECTS AND HIGHEST ENERGY COSMIC AND …

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We give an overview over models in which cosmic rays above 1 EeV = 10**(18) eV are produced by the decay of supermassive "X" particles released from topological defects possibly created in cosmological phase transitions. We note that, for…

Astrophysics · Physics 2007-05-23 Guenter Sigl

The topological defect scenario of origin of the observed highest energy cosmic rays is reviewed. Under a variety of circumstances, topological defects formed in the early Universe can be sources of very massive particles in the Universe…

Astrophysics · Physics 2009-10-30 Pijushpani Bhattacharjee

Cosmic rays with energies exceeding $10^{20}\eV$ have been detected. The origin of these highest energy cosmic rays remains unknown. Established astrophysical acceleration mechanisms encounter severe difficulties in accelerating particles…

Astrophysics · Physics 2009-10-22 P. Bhattacharjee , G. Sigl

Using the propagation of ultra high energy nucleons, photons and electrons in the universal radiation backgrounds, we obtain limits on the luminosity of topological defects scenarios for the origin of the highest energy cosmic rays. The…

Astrophysics · Physics 2011-05-12 R. J. Protheroe , Todor Stanev

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

Astrophysics · Physics 2008-02-03 Guenter Sigl , Sangjin Lee , Paolo Coppi

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

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

Astrophysics · Physics 2011-05-23 F. W. Stecker

We derive observational consequences of the hypothesis that cosmic rays (CR's) of energy $>10^{19}eV$ originate in the same cosmological objects producing gamma-ray bursts (GRB's). Inter-galactic magnetic fields $\gtrsim 10^{-12} G$ are…

Astrophysics · Physics 2009-10-28 Jordi Miralda-Escude , Eli Waxman

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

It is commonly accepted that high energy cosmic rays up to $10^{19}$ eV can be produced in catastrophic astrophysical processes. However the source of a few observed events with higher energies remains mysterious. We propose that they may…

High Energy Physics - Phenomenology · Physics 2025-01-30 E. V. Arbuzova

It is pointed out that the observed extremely high energy cosmic rays (EHECR) above $10^{11}$ GeV and the observed baryon asymmetry of the Universe (BAU), both may have a common origin in baryon number violating decays of supermassive ``X''…

High Energy Physics - Phenomenology · Physics 2009-10-31 Pijushpani Bhattacharjee

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

Physics beyond the standard model might imply the cosmological production of particles with grand unification scale energies. Nucleons and gamma-rays from such processes are candidates for the cosmic rays observed beyond 100 EeV [10**(20)…

Astrophysics · Physics 2009-10-28 Guenter Sigl , Sangjin Lee , David N. Schramm , Paolo Coppi

While several arguments can be proposed against the existence of particles with energy in excess of $(3-5)\times 10^{19}$ eV in the cosmic ray spectrum, these particles are actually observed and their origin seeks for an explanation. After…

Astrophysics · Physics 2007-05-23 Pasquale Blasi

Cosmic rays are charged relativistic particles that reach the Earth with extremely high energies, providing striking evidence of the existence of effective accelerators in the Universe. Below an energy around $\sim 10^{17}$ eV cosmic rays…

High Energy Astrophysical Phenomena · Physics 2018-04-25 Giovanni Morlino

A complete model for the origin of high-energy >~10^{14} eV) cosmic rays from gamma-ray bursts (GRBs) and implications of this hypothesis are described. Detection of high-energy neutrinos from GRBs provide an unambiguous test of the model.…

Astrophysics · Physics 2010-11-11 C. Dermer

The possibility for a self-consistent description of all the basic features of the observed cosmic ray spectra and primary composition variations in the energy range of $10^{15}\div 10^{20}$ eV within the Galactic origin scenario is…

High Energy Astrophysical Phenomena · Physics 2019-05-17 A. A. Lagutin , N. V. Volkov , A. G. Tyumentsev , R. I. Raikin

We review the basic ideas on the origin of cosmic rays with energy in excess of $\sim 10^{19}$ eV, in the light of the most recent observational findings. The limited statistics of events detected by the two largest experiments currently…

Astrophysics · Physics 2007-05-23 Pasquale Blasi

Considerations of the collision losses for protons traversing the 2.7 K black body microwave radiation field have led to the conclusion that the highest energy cosmic rays, those observed at $\geq 10^{20}$ eV, must come from sources within…

Astrophysics · Physics 2011-02-21 Elihu Boldt , Pranab Ghosh

We study the large-scale distribution of the arrival directions of the highest energy cosmic rays observed by various experiments. Despite clearly insufficient statistics, we find a deficit of cosmic rays at energies higher than 10^{20} eV…

Astrophysics · Physics 2008-11-26 D. S. Gorbunov , S. V. Troitsky
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