Secondary Photons from High-Energy Protons Accelerated in Hypernovae
Author:
Publisher
American Astronomical Society
Subject
Space and Planetary Science,Astronomy and Astrophysics
Reference24 articles.
1. On the origin of highest energy gamma-rays from Mkn 501
2. Cooling of Accelerated Nucleons and Neutrino Emission in Gamma‐Ray Bursts
3. Prompt GeV–TeV Emission of Gamma‐Ray Bursts Due to High‐Energy Protons, Muons, and Electron‐Positron Pairs
4. Very High Energy Neutrinos Originating from Kaons in Gamma-Ray Bursts
5. Cosmic ray acceleration to very high energy through the non-linear amplification by cosmic rays of the seed magnetic field
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3. Mini-radio lobes in AGN core illumination and their hadronic gamma-ray afterlight;Monthly Notices of the Royal Astronomical Society: Letters;2010-12-30
4. Diffuse high energy neutrinos and cosmic rays from hyperflares of soft-gamma repeaters;New Astronomy;2010-03
5. Broadband Radiation from Primary Electrons in Very Energetic Supernovae;The Astrophysical Journal;2008-12-10
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