Abstract
In this study, an attempt was made to identify the most important nuclei for electron-capture and beta decay during the final stages of stellar evolution. A relevant quantity was obtained, which is a product of abundance of the nuclear species in the core composition and electron-capture rate.
Original language | English |
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Pages (from-to) | 1678-1681 |
Number of pages | 4 |
Journal | Physical Review Letters |
Volume | 86 |
Issue number | 9 |
DOIs | |
Publication status | Published - 26 Feb 2001 |
Externally published | Yes |