Lifetimes of states in 19Ne above the 15O+ alpha threshold
Astrophysical models that address stellar energy generation and nucleosynthesis require a considerable amount of input from nuclear physics and are very sensitive to the detailed structure of nuclei, both stable and unstable. Radioactive nuclei play a dominant role in several stellar environments su...
Main Author: | |
---|---|
Language: | English |
Published: |
University of British Columbia
2008
|
Subjects: | |
Online Access: | http://hdl.handle.net/2429/792 |