Nuclear astrophysics with radioactive beams

被引：87

作者：

Bertulani, C. A. ^{[1
]}

Gade, A. ^{[2
,3
]}

机构：

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

[2] Michigan State Univ, Natl Superconducting Cyclotron Lab, E Lansing, MI 48824 USA

[3] Michigan State Univ, Dept Phys & Astron, E Lansing, MI 48824 USA

来源：

PHYSICS REPORTS-REVIEW SECTION OF PHYSICS LETTERS | 2010年 / 485卷 / 06期

基金：

美国国家科学基金会;

关键词：

Nuclear astrophysics; Rare isotopes; Reactions; WEAK-INTERACTION RATES; NEUTRON-RICH ISOTOPES; EFFECTIVE-FIELD THEORY; CHARGE-EXCHANGE REACTIONS; PROTON-PROTON FUSION; RADIATIVE-CAPTURE REACTIONS; INTERMEDIATE-MASS NUCLEI; SHELL-MODEL CALCULATIONS; TOTAL CROSS-SECTION; ION-TRAP FACILITY;

D O I：

10.1016/j.physrep.2009.09.002

中图分类号：

O4 [物理学];

学科分类号：

0702 ;

摘要：

The quest to comprehend how nuclear processes influence astrophysical phenomena is driving experimental and theoretical research programs worldwide. One of the main goals in nuclear astrophysics is to understand how energy is generated in stars, how elements are synthesized in stellar events and what the nature of neutron stars is. New experimental capabilities, the availability of radioactive beams and increased computational power paired with new astronomical observations have advanced the present knowledge. This review summarizes the progress in the field of nuclear astrophysics with a focus on the role of indirect methods and reactions involving beams of rare isotopes. (C) 2009 Elsevier B.V. All rights reserved.

引用

页码：195 / 259

页数：65

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