Laboratorial radiative shocks with multiple parameters and first quantifying verifications to core-collapse supernovae  

核心缩超新星中辐射冲击波的实验室模拟及首次量化校验

作　　者：Lu Zhang Jianhua Zheng Zhenghua Yang Tianming Song Shuai Zhang Tong Liu Yunfeng Wei Longyu Kuang Longfei Jing Zhiwei Lin Liling Li Hang Li Jinhua Zheng Pin Yang Yuxue Zhang Zhiyu Zhang Yang Zhao Zhibing He Ping Li Dong Yang Jiamin Yang Zongqing Zhao Yongkun Ding 张璐;郑建华;杨正华;宋天明;张帅;刘彤;韦云锋;况龙钰;景龙飞;林雉伟;李丽灵;黎航;郑金华;杨品;张玉雪;张志宇;赵阳;何智兵;李平;杨冬;杨家敏;赵宗清;丁永坤

机构地区：[1]Research Center of Laser Fusion,China Academy of Engineering Physics,Mianyang 621900,China [2]Department of Astronomy,Xiamen University,Xiamen 361005,China [3]Institute of Applied Physics and Computational Mathematics,Beijing 100088,China

出　　处：《Science Bulletin》2024年第20期3188-3191,共4页科学通报（英文版）

基　　金：supported by the National Natural Science Foundation of China(12335015,12375238,12173031,12303049,and 12105269)。

摘　　要：A radiative shock(RS)is one in which the density and temperature structures are affected by radiation from the shock-heated matter.RS plays a special role in astrophysics as it nontrivially combines both hydrodynamics and radiation physics.In most astrophysical shocks,the temperature and density conditions lead to strong emission,with radiation thus playing a major role therein.

关 键 词：SHOCKS RADIATIVE shock 

分 类 号：P145.3[天文地球—天体物理]