Magnetar Driven Emission in Short Gamma-Ray Bursts

该项目将涉及开发利用磁星的自旋下降作为能源的SGRBs扩展发射的理论模型。该项目将涉及在两颗中子星合并后不久开发磁星自旋下降的分析和流体力学模型。这些模型将被用来生成理论上的高能光曲线，这些曲线可以与NASA的雨燕伽马射线天文台等天文台的观测数据相吻合。

This project will involve the development of theoretical models for the extended emission of SGRBs that use the spin-down of magnetars as the energy source. The project will involve the development of analytical and hydrodynamical models of the spin-down of magnetars shortly after a merger of two neutron stars. These models will be used to generate theoretical high-energy light curves, which can be fit to observational data from observatories such as NASA's Swift Gamma-ray Observatory.