论文标题
领先伽玛射线爆发理论的关键测试ii
Critical Tests of Leading Gamma Ray Burst Theories II
论文作者
论文摘要
从观察到IC型的超新星（SNE）产生长持续时间γ射线（GRB），而中子星的合并产生短的硬grb。无需SN的GRB大概起源于高质量X射线二进制中的中子星的相变。这些现象实际上是如何产生GRB的。 GRBS的火球和炮弹模型及其余潮已被广泛面临着巨大的观察数据，他们的后卫声称成功。但是，这些索赔可能反映了多种选择和许多可调参数的使用，而不是模型的有效性。只有使用可靠的观察数据对模型的关键伪造预测的对抗才能测试其有效性。本报告中审查了此类关键测试。
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.
