Magnetar Driven Emission in Short Gamma-Ray Bursts

短伽马射线爆发中的磁星驱动发射

• 批准号: 2109183
• 金额: --
• 依托单位: University of Leicester
• 依托单位国家: 英国
• 项目类别: Studentship
• 财政年份: 2018
• 资助国家: 英国
• 起止时间: 2018 至 无数据
• 项目状态: 已结题
• 来源: https://gtr.ukri.org/projects?ref=studentship-2109183
• 关键词: Magnetar; Driven; Emission; Short; Gamma

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.

该项目将涉及使用磁星自旋下降作为能源的SGRB扩展发射的理论模型的开发。该项目将涉及开发两颗中子星合并后不久磁星自旋下降的分析和流体动力学模型。这些模型将用于生成理论上的高能光变曲线，这些光变曲线可以与来自美国宇航局斯威夫特伽马射线天文台等天文台的观测数据相拟合。