Nuclear Astrophysics with Radioactive Beams
arXiv:0909.5693 · doi:10.1016/j.physrep.2009.09.002
Abstract
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.
121 pages, 27 figures, 510 references, to appear in Physics Reports. Minor typos and references fixed
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- Reanalysis of N()O reaction and its role in stellar CNO cycle
- Charge Pickup Reaction Cross Section for Neutron-Rich p-Shell Isotopes at 900A MeV
- The Cosmological Lithium Problem Revisited
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