Nuclear Astrophysics from View Point of Few-Body Problems

被引：14
作者：
Tumino, A. [1 ,2 ]
Spitaleri, C. [1 ,3 ]
Bertulani, C. [4 ]
Mukhamedzhanov, A. M. [5 ]
机构：
[1] Ist Nazl Fis Nucl, Lab Nazl Sud, I-95129 Catania, Italy
[2] Univ Enna KORE, Enna, Italy
[3] Univ Catania, Dipartimento Fis & Astron, Catania, Italy
[4] Texas A&M Univ, Commerce, TX USA
[5] Texas A&M Univ, Inst Cyclotron, College Stn, TX 77843 USA
来源：
FEW-BODY SYSTEMS | 2013年 / 54卷 / 7-10期
关键词：
TROJAN HORSE METHOD; CROSS-SECTION; COULOMB DISSOCIATION; LOW-ENERGY; BREAKUP; B-8;
D O I：
10.1007/s00601-013-0690-5
中图分类号：
O4 [物理学];
学科分类号：
0702 ;
摘要：
Few-body systems provide very useful tools to solve different problems for nuclear astrophysics. This is the case of indirect techniques, developed to overcome some of the limits of direct measurements at astrophysical energies. Here the Coulomb dissociation, the asymptotic normalization coefficient and the Trojan Horse method are discussed.
引用
收藏
页码：869 / 875
页数：7
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