Low-energy nuclear reaction studies with RI beams in nuclear astrophysics

Details Low-energy nuclear reaction studies with RI beams in nuclear astrophysics Low-energy nuclear reaction studies with RI beams in nuclear astrophysics

Jul 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003nupha.722...17k&link_type=abstract

Nuclear Physics A, Volume 722, p. C17-C23.

Physics

Nuclear Physics

Scientific paper

After a brief discussion on the recent development in nuclear astrophysics, two reaction studies of typical astrophysical reactions at low energies where nuclear reactions play the main contributions to the nucleosynthesis in the universe, are discussed. One is the proton capture reaction, 11C(p, γ)12N, studied by the direct method using a 11C beam produced with a new low-energy RIB separator CRIB at CNS, Japan. The second one is the 13C(α, n)16O rearrangement reaction, which is believed to be the main neutron source for the s-process at low temperatures, investigated by an indirect method using the direct α-transfer reaction 13C(6Li, d)17O. Detailed investigations are suggested on the nuclear reactions relevant.

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