教师姓名：鲍必文

职称：讲师

系所：统计系

研究领域：数值模拟

电子邮件：baobiwen@ynu.edu.cn

教育背景：

2007.09-2011.0737000gcom威尼斯数理基础科学本科

2011.09-2014.0737000gcom威尼斯理论物理硕士

2015.09-2019.0737000gcom威尼斯理论物理博士

工作经历：

2019.07-2021.0737000gcom威尼斯统计学博士后流动站师资博士后

2021.09-至今37000gcom威尼斯统计系

主要研究领域：超新星遗迹的数值模拟与数据分析

代表性学术论著：

1.Bao, Biwen;Peng, Qiyong; Yang, Chuyuan; Zhang, Li; Evolutions of Young Type Ia Supernova Remnants with Two Initial Density Profiles in a Turbulent Medium; The Astrophysical Journal; 2021, 909, 173

2. Peng, Qiyong;Bao, Biwen*;Yang, Chuyuan; Zhang, Li; Simulations of Young Type Ia Supernova Remnants Undergoing Shock Acceleration in a Turbulent Medium; The Astrophysical Journal; 2020, 891, 75

3.Bao, Biwen;Yang, Chuyuan; Zhang, Li; 3D MHD Numerical Simulations of Polarized Emission in the Turbulent Background from Young Type Ia Supernova Remnants; The Astrophysical Journal; 2018, 866, 37

4. Yang, Chu-yuan;Bao, Bi-wen;Liu, Si-ming; MHD simulations of inward shocks in Cassiopeia A; Research in Astronomy and Astrophysics; 2020, 20, 48

5. Lin, Wen-hui;Bao, Bi-wen;Jiang, Ze-jun; Zhang, Li; Spectral hardening of cosmic ray protons and helium nuclei in supernova remnant shocks; Chinese Physics C; 2019, 43, 5

6. Wang, Yueyang;Bao, Biwen;Yang, Chuyuan; Zhang, Li; The impact of different interstellar medium structures on the dynamical evolution of supernova remnants; Monthly Notices of the Royal Astronomical Society; 2018, 478, 2948

7. Lin, Wen-hui;Bao, Bi-wen;Jiang, Ze-jun; Zhang, Li; A possible explanation of the knee of cosmic light component spectrum from 100 TeV to 3 PeV; Chinese Physics C; 2017, 41, 10 

代表性教学科研项目：2020.10云南省博士后科学基金主持