Light-Mass Cluster Reactions in Supernova R-Process

Details Light-Mass Cluster Reactions in Supernova R-Process Light-Mass Cluster Reactions in Supernova R-Process

Jul 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005nupha.758..639s&link_type=abstract

Nuclear Physics A, Volume 758, p. 639-642.

Physics

Nuclear Physics

1

Scientific paper

In explosive circumstances of the neutrino-driven winds in gravitational core-collapse Type II supernovae (SNe), not only heavy neutron-rich nuclei but also light unstable nuclei play the significant roles. We here study the efficiency and sensitivity of the SN r-process nucleosynthesis to many relevant nuclear reaction rates, and discuss quantitatively that several specific nuclear reactions on light neutron-rich nuclei take very critical keys to the final nucleosynthesis yields of r-process elements [Sasaqui, Kajino, T., T., Otsuki, K., Mathews, G. J. and Nakamura, T., Astrophys. J.(2004), submitted].

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