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Critical Tests of Leading Gamma Ray Burst Theories II
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It has been observationally established that supernovae (SNe) of Type Ic produce long duration gamma ray bursts (GRBs) and that neutron star mergers generate short hard GRBs. SN-Less GRBs presumably originate in a phase transition of a neutron star in a high mass X-ray binary. How these phenomena actually generate GRBs is debated. The fireball and cannonball models of GRBs and their afterglows have been widely confronted with the huge observational data, with their defenders claiming success. The claims, however, may reflect multiple choices and the use of many adjustable parameters, rather than the validity of the models. Only a confrontation of key falsifiable predictions of the models with solid observational data can test their validity. Such critical tests are reviewed in this report.
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Cited by 1 Pith paper
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A revamped understanding of Cosmic Rays and Gamma-Ray Bursts
The paper claims new GRB and cosmic-ray data validate the Cannonball Model, with knees and positrons explained by relativistic supernova ejecta, though several 'predictions' rely on fitted parameters.
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