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• W2894976469 endingPage "350" @default.
• W2894976469 startingPage "350" @default.
• W2894976469 abstract "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." @default.
• W2894976469 created "2018-10-12" @default.
• W2894976469 creator A5020247892 @default.
• W2894976469 creator A5035893527 @default.
• W2894976469 creator A5066574735 @default.
• W2894976469 date "2022-06-24" @default.
• W2894976469 modified "2023-09-25" @default.
• W2894976469 title "Critical Tests of Leading Gamma Ray Burst Theories" @default.
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