• Corpus ID: 118579008

Gamma Ray Bursts in the HAWC Era

  title={Gamma Ray Bursts in the HAWC Era},
  author={P'eter M'esz'aros and Katsuaki Asano and Kohta Murase and Derek W. Fox and He Gao and Nicholas Senno},
  journal={arXiv: High Energy Astrophysical Phenomena},
Gamma-Ray Bursts are the most energetic explosions in the Universe, and are among the most promising for detecting multiple non-electromagnetic signals, including cosmic rays, high energy neutrinos and gravitational waves. The multi-GeV to TeV gamma-ray range of GRB could have significant contributions from hadronic interactions, mixed with more conventional leptonic contributions. This energy range is important for probing the source physics, including overall energetics, the shock parameters… 

Effects of Goldstone bosons on gamma-ray bursts

Gamma-ray bursts (GRBs) are the most energetic explosion events in the universe. An amount of gravitational energy of the order of the rest-mass energy of the Sun is released from a small region

The Deep and Transient Universe in the SVOM Era: New Challenges and Opportunities - Scientific prospects of the SVOM mission

To take advantage of the astrophysical potential of Gamma-Ray Bursts (GRBs), Chinese and French astrophysicists have engaged the SVOM mission (Space-based multi-band astronomical Variable Objects

Cosmic lighthouses at high redshift : intervening material in sight-lines towards GRBs and QSOs

Despite the great progress of our understanding of the Universe in recent decades, largely due to technological advances in instrumentation and astronomical infrastructure, there are still countless

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Statistical studies of gamma-ray burst (GRB) spectra may result in important information on the physics of GRBs. The Fermi GBM catalog contains GRB parameters (peak energy, spectral indices,



Nuclear Instruments and Methods in Physics Research A278 (1989) 583-584 North-Holland, Amsterdam A MUON DETECTOR FOR ALARGE AIR SHOWER ARRAY

The possibility of detecting point sources of cosmic rays with energies above 10 14 eV has stimulated the construction of air shower arrays which distinguish between electrons and muons. Showers

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