Fusion cross-sections for inertial fusion energy

被引：32
|
作者：
Li, XZ [1 ]
Liu, B
Chen, S
Wei, QM
Hora, H
机构：
[1] Tsinghua Univ, Dept Phys, Beijing 100084, Peoples R China
[2] Tsinghua Univ, Dept Engn Phys, Beijing 100084, Peoples R China
[3] Univ New S Wales, Dept Theoret Phys, Sydney, NSW, Australia
来源：
LASER AND PARTICLE BEAMS | 2004年 / 22卷 / 04期
关键词：
astrophysical S-function; fusion cross-section; inertial fusion; light nucleus fusion; selective resonant tunneling;
D O I：
10.1017/S026303460404011X
中图分类号：
O59 [应用物理学];
学科分类号：
摘要：
The application of selective resonant tunneling model is extended from d + t fusion to other light nucleus fusion reactions, such as d + d fusion and d + He-3. In contrast to traditional formulas, the new formula for the cross-section needs only a few parameters to fit the experimental data in the energy range of interest. The features of the astrophysical S-function are derived in terms of this model. The physics of resonant tunneling is discussed.
引用
收藏
页码：469 / 477
页数：9
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