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Experiments for explosive nuclear reactions in stellar environments

Title
Experiments for explosive nuclear reactions in stellar environments
Authors
Hahn, IS
Ewha Authors
한인식
SCOPUS Author ID
한인식scopus
Issue Date
2004
Journal Title
JOURNAL OF THE KOREAN PHYSICAL SOCIETY
ISSN
0374-4884JCR Link
Citation
vol. 45, pp. S132 - S135
Keywords
nuclear synthesisradioactive ion beamexplosive hydrogen burning
Publisher
KOREAN PHYSICAL SOC
Indexed
SCI; SCIE; SCOPUS; KCI WOS scopus
Abstract
One of the major ways of studying the Universe is laboratory measurements of the nuclear reactions that are responsible for energy generation and creating new elements in stellar environments. There are many key nuclear reactions that require laboratory measurements for understanding stellar sites such as the Sun, novae, supernovae, and x-ray bursts. Two such reactions that are important for understanding the break-out mechanism from the Hot CNO cycle in explosive hydrogen burnings are the O-14(alpha,p)F-17 and O-15(alpha,gamma)Ne-19 reactions. A brief review of the above reactions and some new experimental methods to measure one of the reactions, the O-14(alpha,p)F-17 reaction, using radioactive beams at Oak Ridge National Laboratory in U.S. and CNS in Japan will be discussed.
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사범대학 > 과학교육과 > Journal papers
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