Speaker
yangfan he
(China Institute of Atomic Energy, Beijing 102413, China ; School of Physics and Space Sciences, China West Normal University, Nanchong 637002, China)
Description
核聚变反应是自然界中为恒星提供能量并产生新元素的最重要过程。因此，研究接近真实天体物理条件的全等离子体环境中的反应至关重要。强激光与物质相互作⽤时产⽣的⾼温、⾼压、⾼密的等离⼦体环境，是对天体环境很好的近似，我们使用了神光Ⅱ号装置驱动等离子体对撞的方法研究了2H(d, p)3H反应，用CR-39固体探测器分别记录了K型靶（LiD）、平面靶（LiD）、K型混合靶（LiD,LiH）、平面混合靶（LiD,LiH）发生2H(d, p)3H反应的质子。
| Abstract Type | Talk |
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Primary authors
bing guo
(China Institute of Atomic Energy, Beijing 102413, China)
yangfan he
(China Institute of Atomic Energy, Beijing 102413, China ; School of Physics and Space Sciences, China West Normal University, Nanchong 637002, China)
Co-authors
Donghai Zhang
(School of Physics and Information Engineering, Shanxi Normal University, Linfen 041004, China)
Jihong Wei
(China Institute of Atomic Energy, Beijing 102413, China ; College of Nuclear Science and Technology, Beijing Normal University, Beijing 100875, China)
Luohuan Wang
(School of Physics and Information Engineering, Shanxi Normal University, Linfen 041004, China)
Menglin Qiu
(College of Nuclear Science and Technology, Beijing Normal University, Beijing 100875, China)
Wansha Yang
(China Institute of Atomic Energy, Beijing 102413, China ; College of Nuclear Science and Technology, Beijing Normal University, Beijing 100875, China)
chuangye he
(China Institute of Atomic Energy, Beijing 102413, China)
di wu
(China Institute of Atomic Energy, Beijing 102413, China)
fulong liu
(China Institute of Atomic Energy, Beijing 102413, China ; College of Nuclear Science and Technology, Beijing Normal University, Beijing 100875, China)
guangfu wang
(College of Nuclear Science and Technology, Beijing Normal University, Beijing 100875, China)
shilun guo
(China Institute of Atomic Energy, Beijing 102413, China)
xiaofei lan
(School of Physics and Space Sciences, China West Normal University, Nanchong 637002, China)
