Physics
Scientific paper
Feb 2006
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006sgrb.confe..15d&link_type=abstract
Presented at the KITP Conference: Supernova and Gamma-Ray Burst Remnants, Feb 10, 2006, Kavli Institute for Theoretical Physics,
Physics
Scientific paper
A unified theory of high energy astrophysical phenomena, which is based onan SN-CR-GRB association and the Cannonball Model of highly relativistic astrophysical jets explains (a) the origin and main properties of the high energy cosmic rays (CRS) at all energies, (b) the origin and main properties of gamma ray bursts (GRBs) (c) the origin of the extragalactic gamma-ray background radiation (GBR), (d) the origin of Galactic and extragalactic magnetic fields (e) the missing heat source in "cooling flow" galaxy clusters.
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