Production of Secondary Radioactive 21Na Beam for the Study of 21Na(α,p)24Mg Stellar Reaction

Details Production of Secondary Radioactive 21Na Beam for the Study of 21Na(α,p)24Mg Stellar Reaction Production of Secondary Radioactive 21Na Beam for the Study of 21Na(α,p)24Mg Stellar Reaction

Apr 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008pun..conf..431b&link_type=abstract

PHYSICS OF UNSTABLE NUCLEI. Proceedings of the International Symposium on the ISPUN07. Held 3-7 July 2007 in Hoi An, Vietnam. Ed

Physics

Scientific paper

The availability of radioactive beams has produced great opportunities for advances in our understanding of the nucleosynthesis occurring in stellar explosions such as novae, X-ray burst and supernovae. By using an in-flight low-energy radioisotope beam separator (CRIB) at Center for Nuclear Study (CNS), University of Tokyo, we have successfully produced the 21Na proton-rich beam for the study of 21Na(α,p)24Mg reaction which is related to the astrophysically important production of 22Na in the stellar explosive environments. Since it is the first time when this reaction is studied experimentally, we have performed a test experiment to produce the 21Na beam and to estimate the feasibility of the experimental study of 21Na(α,p)24Mg reaction.

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