报告题目：The Probability Photosphere Model for the Prompt Emission of Gamma-ray Burst

报 告 人：蒙延智 南京尊龙凯时

报告时间：2020年9月22日（星期二）14：30（北京时间）

报告地点：在线报告 腾讯会议ID：676592 702

报告摘要：

Gamma-ray burst (GRB) is one of the most violent events in the deep universe. Ithas two emission stages. The earlier one is the prompt emission inγ-ray band. After theprompt emission, we can see its multi-wavelength afterglows.After decades of investigation, the origin of the prompt emission remainsunclear, especially the radiation mechanism. The synchrotron emission or the photosphericemission origin has been long-debated.

Iwill give a detailed review on the researches of GRB prompt emission, both theobservations and models. Then, I will talk about my theoretical studies withinthe framework of the probability photosphere model, considering the morenatural and reasonable physical conditions of jet structure, jet compositionand viewing angle. Also, which observational and statistic features can be reproducedby the modified model will be shown.

主办单位：尊龙凯时物理学院

尊龙凯时理论物理中心