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相关论文: Gamma Ray Bursts as Possible High Energy Sources

200 篇论文

We explore several models which might be proposed to explain recent possible detections of high-energy (TeV) gamma rays in association with low-energy gamma-ray bursts (GRBs). Likely values (and/or upper limits) for the source energies in…

天体物理学 · 物理学 2009-11-07 P. C. Fragile , G. J. Mathews , J. Poirier , T. Totani

Gamma-ray bursts (GRBs) are the most luminous explosions in the Universe and are powered by ultra-relativistic jets. Their prompt $\gamma$-ray emission briefly outshines the rest of the $\gamma$-ray sky making them detectable from…

高能天体物理现象 · 物理学 2022-06-07 Ramandeep Gill , Jonathan Granot

Air shower experiments have detected cosmic ray events of energies upto 300 EeV. Most likely these cosmic rays have originated from compact objects. Their exact sources are yet to be identified. It has been suggested before that gamma ray…

宇宙学与河外天体物理 · 物理学 2010-01-05 Nayantara Gupta

Gamma-ray bursts (GRBs) are the most luminous electromagnetic burst in the Universe. They occur when a rapidly rotating massive star collapses or a binary neutron star merges. These events leave a newborn central compact object, either a…

高能天体物理现象 · 物理学 2022-02-15 Shigeo S. Kimura

Observations imply that gamma-ray bursts (GRBs) are produced by the dissipation of the kinetic energy of a highly relativistic fireball. Photo-meson interactions of protons with gamma-rays within the fireball dissipation region are expected…

天体物理学 · 物理学 2007-05-23 Dafne Guetta

We propose a new hypothesis for the origin of the major part of non-solar hadronic cosmic rays (CRs) at all energies: highly relativistic, narrowly collimated jets from the birth or collapse of neutron stars (NSs) in our Galaxy accelerate…

天体物理学 · 物理学 2011-05-23 A. Dar , R. Plaga

Statistical arguments show that the volume- and time-averaged kinetic power of GRBs and fireball transients (FTs) into an L* galaxy like the Milky Way is at the level of 10^40 ergs/s. This number, though with wide uncertainties related to…

天体物理学 · 物理学 2009-10-31 Charles D. Dermer

Gamma-ray bursts (GRBs) are short and intense flashes at the cosmological distances, which are the most luminous explosions in the Universe. The high luminosities of GRBs make them detectable out to the edge of the visible universe. So,…

高能天体物理现象 · 物理学 2016-02-17 Patrick Petitjean , F. Y. Wang , X. F. Wu , J. J. Wei

Gamma-ray bursts (GRB) are generally believed to be efficient particle accelerators. In the presence of energetic protons in a GRB jet, interactions between these protons and intense radiation field of the GRB are supposed to induce…

高能天体物理现象 · 物理学 2023-02-01 Ruo-Yu Liu , Hai-Ming Zhang , Xiang-Yu Wang

Long Gamma-Ray Bursts (GRBs) are the brightest electromagnetic explosions in the Universe, associated to the death of massive stars. As such, GRBs are potential tracers of the evolution of the cosmic massive star formation, metallicity, and…

天体物理学 · 物理学 2011-02-01 V. Avila-Reese , C. Firmani , G. Ghisellini , J. I. Cabrera

Gamma-ray bursts, which are among the most violent events in the universe, are one of the few viable candidates to produce ultrahigh energy cosmic rays. Recently, observations have revealed that GRBs generally originate from metal-poor…

天体物理学 · 物理学 2008-11-26 Hasan Yuksel , Matthew D. Kistler

Simple arguments concerning power and acceleration efficiency show that ultra-high energy cosmic rays (UHECRS) with energies >~ 10^{19} eV could originate from GRBs. Neutrons formed through photo-pion production processes in GRB blast waves…

天体物理学 · 物理学 2009-11-06 C. D. Dermer

$\gamma$-ray bursts have baffled theorists ever since their accidental discovery at the sixties. We suggest that these bursts originate in merger of neutron star binaries, taking place at cosmological distances. These mergers release…

天体物理学 · 物理学 2009-10-22 Tsvi Piran

We introduce neutrino astronomy starting from the observational fact that Nature accelerates protons and photons to energies in excess of 10^{20} and 10^{13} eV, respectively. Although the discovery of cosmic rays dates back a century, we…

天体物理学 · 物理学 2007-05-23 F. Halzen

Recent observations provide compelling evidence that the bulk of the high energy cosmic rays (CRs) and gamma-ray bursts (GRBs) are co-produced by highly relativistic jets of plasmoids of stellar matter. These jets are launched by fall back…

高能天体物理现象 · 物理学 2024-02-06 Shlomo Dado , Arnon Dar

I give a brief review of high energy gamma-ray signatures of dark matter. The decay of massive $X$-particles and subsequent hadronization have been suggested as the origin of the highest energy cosmic rays. Propagation over cosmological…

天体物理学 · 物理学 2009-10-31 R. J. Protheroe

The gamma-ray burst (GRB) model for production of ultra-high-energy cosmic-rays (UHECRs) is based on the hypothesis that GRBs arise from the dissipation of the kinetic energy of relativistic fireballs at cosmological distances. Recent GRB…

天体物理学 · 物理学 2009-10-31 E. Waxman

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…

天体物理学 · 物理学 2009-10-28 Jordi Miralda-Escude , Eli Waxman

The origin of ultra high energy cosmic rays promises to lead us to a deeper understanding of the structure of matter. This is possible through the study of particle collisions at center-of-mass energies in interactions far larger than…

Ground based extensive air showers arrays can observe GRBs in the 1-1000 GeV energy range using the "single particle" techique. The sensitivity to detect a GRB as a function of the burst parameters and the detector characteristics are…

天体物理学 · 物理学 2011-05-23 Silvia Vernetto