Gamma-Ray Bursts at TeV Energies: Theoretical Considerations

Keyphrases

• Gamma-ray Bursts 100%
• TeV Energies 100%
• High Energy 57%
• Afterglow Emission 28%
• Spectral Components 28%
• Fermi-LAT 28%
• Afterglow 14%
• Relativistic Jets 14%
• Ultra-relativistic 14%
• High-energy Emissions 14%
• Prompt Emission 14%
• Lorentz Violation 14%
• Emission Mechanism 14%
• Emission Region 14%
• Delayed Onset 14%
• Energy Band 14%
• Galactic 14%
• Cosmological Distances 14%
• Intergalactic Magnetic Fields 14%
• Hadronic 14%
• Collisionless Shocks 14%
• Leptonic 14%
• Shock Physics 14%
• Imaging Atmospheric Cherenkov Telescope 14%
• Energy Domain 14%
• Background Light 14%
• Ground-based Imaging 14%
• Electromagnetic Window 14%

Physics

• Gamma Ray Burst 100%
• Afterglow 42%
• Physics 28%
• Relativistic Jets 14%
• Energetics 14%
• Magnetic Field 14%
• Energy Band 14%
• Atmospherics 14%
• Electromagnetism 14%