标题： 伽马射线暴的喷流盘共生模型：流量分布、宇宙线和$ν$ 显示英文标题

标题： A jet-disk symbiosis model for Gamma Ray Bursts: fluence distribution, CRs and $ν$'s

摘要： 我们考虑了一个喷流-盘共生模型来解释伽马射线暴及其余辉。 有人提出伽马射线暴是在一个双星系统中的中子星内部产生的喷流中形成的，由于吸积作用，这个中子星塌缩成了黑洞。 在我们的模型中，我们假设由于这种转变而释放出的初始能量的一部分通过磁场沉积到喷流中。 所观测到的辐射是由沿喷流传播的超高相对论激波引起的。 对于像银河系喷流源SS433这样的系统，我们可以很好地拟合观测数据。 具体来说，我们能够重现典型的观测到的余辉发射通量、其随时间变化的光谱以及修正后的4B BATSE目录中伽马暴的数据流量分布。 我们也研究了我们模型的宇宙学演化与宇宙射线能量分布之间的关系。 我们使用恒星形成率（SFR）作为红移的函数来获得我们模型中伽马暴流量的分布。 伽马射线带中的流量被用来计算银河系和河外距离处的宇宙射线能量。 这一能量输入与银河系和河外的宇宙射线和中微子谱进行了比较。 我们发现，在我们模型的框架下，伽马暴对河外或银河系宇宙射线谱没有任何贡献。 显示英文摘要

摘要： We consider a jet-disk symbiosis model to explain Gamma Ray Bursts and their afterglows. It is proposed that GRBs are created inside a pre-existing jet from a neutron star in a binary system which collapses to a black hole due to accretion. In our model we assume that a fraction of the initial energy due to this transition is deposited in the jet by magnetic fields. The observed emission is then due to an ultrarelativistic shock wave propagating along the jet. Good agreement with observational data can be obtained for systems such as the Galactic jet source SS433. Specifically, we are able to reproduce the typical observed afterglow emission flux, its spectrum as a function of time, and the fluence distribution of the corrected data for the 4B BATSE catalogue. We also studied the relation between the cosmological evolution of our model and the cosmic ray energy distribution. We used the Star Formation Rate (SFR) as a function of redshift to obtain the distribution in fluences of GRBs in our model. The fluence in the gamma ray band has been used to calculate the energy in cosmic rays both in our Galaxy and at extragalactic distances. This energy input has been compared with the Galactic and extragalactic spectrum of cosmic rays and neutrinos. We found that in the context of our model it is not possible to have any contribution from GRBs to either the extragalactic or the Galactic cosmic ray spectra.