Indirect techniques in nuclear astrophysics: a review

被引：194

作者：

Tribble, R. E. ^{[1
]}

Bertulani, C. A. ^{[2
]}

La Cognata, M. ^{[3
]}

Mukhamedzhanov, A. M. ^{[1
]}

Spitaleri, C. ^{[3
,4
]}

机构：

[1] Texas A&M Univ, Inst Cyclotron, College Stn, TX 77843 USA

[2] Texas A&M Univ Commerce, Dept Phys, Commerce, TX 75429 USA

[3] Ist Nazl Fis Nucl, Lab Nazl Sud, I-95123 Catania, Italy

[4] Univ Catania, Dipartimento Fis & Astron, I-95123 Catania, Italy

来源：

REPORTS ON PROGRESS IN PHYSICS | 2014年 / 77卷 / 10期

基金：

美国国家科学基金会;

关键词：

nuclear reactions; stellar burning; explosive hydrogen burning; ASYMPTOTIC GIANT BRANCH; TROJAN HORSE METHOD; QUASI-FREE SCATTERING; COULOMB BREAK-UP; COUPLED-CHANNELS CALCULATIONS; ALPHA)N-15 REACTION-RATE; REACTION CROSS-SECTION; LOW-ENERGY; S-FACTOR; ANGULAR-DISTRIBUTION;

D O I：

10.1088/0034-4885/77/10/106901

中图分类号：

O4 [物理学];

学科分类号：

0702 ;

摘要：

In this review, we discuss the present status of three indirect techniques that are used to determine reaction rates for stellar burning processes, asymptotic normalization coefficients, the Trojan Horse method and Coulomb dissociation. A comprehensive review of the theory behind each of these techniques is presented. This is followed by an overview of the experiments that have been carried out using these indirect approaches.

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