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The suggested association between the sources of gamma-ray bursts (GRB's) and the sources of ultra-high energy cosmic rays (UHECR's) is based on two arguments: (i) The average energy generation rate of UHECR's is similar to the gamma-ray…

Astrophysics · Physics 2010-11-15 E. Waxman

The origin and nature of the ultrahigh energy cosmic rays (UHECRs) are still unknown. However, great progress has been achieved in past years due to the observations performed by the Pierre Auger Observatory and Telescope Array. Above…

High Energy Astrophysical Phenomena · Physics 2019-05-22 A. D. Supanitsky

We outline two concepts to explain Ultra High Energy Cosmic Rays (UHECRs), one based on radio galaxies and their relativistic jets and terminal hot spots, and one based on relativistic Super-Novae (SNe) or Gamma Ray Bursts (GRBs) in…

Gamma ray burst (GRB) fireballs provide one of very few astrophysical environments where one can contemplate the acceleration of cosmic rays to energies that exceed 10^20 eV. The assumption that GRBs are the sources of the observed cosmic…

High Energy Astrophysical Phenomena · Physics 2015-03-19 M. Ahlers , M. C. Gonzalez-Garcia , F. Halzen

The statistical distribution of energies among particles responsible for long Gamma Ray Burst (GRB) emission is analyzed in light of recent results of the Fermi Observatory. The allsky flux, $F_{\gamma}$, recorded by the Gamma Ray Burst…

High Energy Astrophysical Phenomena · Physics 2011-01-27 David Eichler , Dafne Guetta , Martin Pohl

We study the production of cosmogenic neutrinos and photons during the extragalactic propagation of ultra-high-energy cosmic rays (UHECRs). For a wide range of models in cosmological evolution of source luminosity, composition and maximum…

High Energy Astrophysical Phenomena · Physics 2011-11-16 Guillaume Decerprit , Denis Allard

The paper is devoted to the analysis of particle acceleration in Gamma-Ray Bursts and its radiative consequences. Therefore we get on one hand constraints on the physics and on the other hand possible signatures of particle acceleration…

Astrophysics · Physics 2009-11-10 Denis Gialis , Guy Pelletier

The origin of ultra-high energy cosmic rays $($UHECRs$)$ remains a mystery. It has been suggested that UHECRs can be produced by the stochastic acceleration in relativistic jets of gamma-ray bursts $($GRBs$)$ at the early afterglow phase.…

High Energy Astrophysical Phenomena · Physics 2021-11-17 Ze-Lin Zhang , Ruo-Yu Liu , Xiang-Yu Wang

A model for high-energy (>10^14 eV) cosmic rays (HECRs) from galactic and extragalactic gamma-ray bursts (GRBs) is summarized. Relativistic outflows in GRBs are assumed to inject power-law distributions of CR protons and ions to the highest…

Astrophysics · Physics 2009-11-10 S. D. Wick , C. D. Dermer , A. Atoyan

Gamma-ray bursts (GRBs) have long been considered potential sources of ultra-high-energy cosmic rays (UHECRs; with energy $\gtrsim 10^{18} {\rm~eV}$). In this work, we propose a novel model generating MeV emission lines in GRB, which can…

High Energy Astrophysical Phenomena · Physics 2024-06-11 Yu-Jia Wei , Jia Ren , Hao-Ning He , Yuan-Pei Yang , Da-Ming Wei , Zi-Gao Dai , B. Theodore Zhang

Low-luminosity gamma-ray bursts (GRBs) with luminosity . 10^49erg/s probably consititute a distinct population from the classic high-luminosity GRBs. They are the most luminous objects detected so far within ~ 100 Mpc, the horizon distance…

High Energy Astrophysical Phenomena · Physics 2015-05-30 Ruo-Yu Liu , Xiang-Yu Wang , Zi-Gao Dai

The discoveries of the GZK cutoff with the HiRes and Auger Observatories and the discovery by Auger of clustering of >~60 EeV ultra-high energy cosmic rays (UHECRs) towards nearby <~75 Mpc) AGNs along the supergalactic plane establishes the…

Astrophysics · Physics 2011-11-10 Charles D. Dermer

GeV-TeV gamma-rays and PeV-EeV neutrino backgrounds provide a unique window on the nature of the ultra-high-energy cosmic-rays (UHECRs). We discuss the implications of the recent Fermi-LAT data regarding the extragalactic gamma-ray…

High Energy Astrophysical Phenomena · Physics 2017-04-26 Noemie Globus , Denis Allard , Etienne Parizot , Tsvi Piran

The sources of ultra-high energy cosmic rays (UHECRs) are still one of the main open questions in high-energy astrophysics. If UHECRs are accelerated in astrophysical sources, they are expected to produce high-energy photons and neutrinos…

High Energy Astrophysical Phenomena · Physics 2020-01-27 A. Barbano

The origin of ultra-high energy cosmic rays (UHECRs) is one of the most mystifying issues in astroparticle physics. It has been suggested that gamma-ray bursts (GRBs) are excellent acceleration sites for cosmic rays. The propagation of…

High Energy Astrophysical Phenomena · Physics 2023-03-08 Nestor Mirabal

The recent discovery of extragalactic PeV neutrinos opens a new window to the exploration of cosmic-ray accelerators. The observed PeV neutrino flux is close to the Waxman-Bahcall upper bound implying that gamma-ray bursts (GRBs) may be the…

High Energy Astrophysical Phenomena · Physics 2015-06-19 Maria Petropoulou , Dimitrios Giannios , Stavros Dimitrakoudis

There is mounting evidence from observations of long duration gamma ray bursts (GRBs), supernova remnants (SNR) and the supernova (SN) explosion 1987A, that SN explosions eject highly relativistic bipolar jets of plasmoids (cannonballs) of…

Astrophysics · Physics 2007-05-23 Arnon Dar

This paper presents the theoretical basis of the fireball/blast wave model, and some implications of recent results on GRB source models and cosmic-ray production from GRBs. BATSE observations of the prompt gamma-ray luminous phase, and…

Astrophysics · Physics 2007-05-23 C. D. Dermer

The diffuse neutrino flux measured in IceCube is comparable with the ultrahigh-energy cosmic ray (UHECR) flux, which has led to the concept of a unified origin of high-energy neutrino and UHECR backgrounds. We construct a generic…

High Energy Astrophysical Phenomena · Physics 2020-10-28 Shigeru Yoshida , Kohta Murase

We study the acceleration of CR protons and nuclei at GRB internal shocks. Physical quantities and their time evolution are estimated using the internal shock modeling implemented by Daigne & Mochkovitch 1998. We consider different…

High Energy Astrophysical Phenomena · Physics 2015-08-06 Noemie Globus , Denis Allard , Robert Mochkovitch , Etienne Parizot