T(T,2n)4He and 3He(3He,2p)4He: The Reaction Mechanism from Solar Energies to 10 MeV

被引：0
|
作者：
Bacher, A. D. [1 ]
Brune, C. R. [2 ]
Sayre, D. B. [3 ]
Hale, G. M. [4 ]
Frenje, J. A. [5 ]
Johnson, M. Gatu [5 ]
机构：
[1] Indiana Univ, Dept Phys, Bloomington, IN 47405 USA
[2] Ohio Univ, Athens, OH 45701 USA
[3] Lawrence Livermore Natl Lab, Livermore, CA 94550 USA
[4] Los Alamos Natl Lab, Los Alamos, NM 87545 USA
[5] MIT, Cambridge, MA 02139 USA
来源：
21ST INTERNATIONAL CONFERENCE ON FEW-BODY PROBLEMS IN PHYSICS | 2016年 / 113卷
关键词：
D O I：
10.1051/epjconf/201611303003
中图分类号：
O57 [原子核物理学、高能物理学];
学科分类号：
070202 ;
摘要：
We have studied the energy dependence of the reaction mechanism of the T(t,2n)He-4 reaction at stellar energies and of its charge symmetric analog reaction He-3(He-3,(2)p)He-4 at energies up 10 MeV. We find that the reaction mechanism changes dramatically over this energy range in part due to the interference of the two identical fermions in the three-body final state.
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