Stellar electron-capture rates inpf-shell nuclei from quasiparticle random-phase approximation calculations
Author:
Publisher
American Physical Society (APS)
Subject
Nuclear and High Energy Physics
Link
http://harvest.aps.org/v2/journals/articles/10.1103/PhysRevC.87.045801/fulltext
Reference77 articles.
1. Synthesis of the Elements in Stars
2. Synthesis of the elements in stars: forty years of progress
3. Stellar weak-interaction rates for sd-shell nuclei. I - Nuclear matrix element systematics with application to Al-26 and selected nuclei of importance to the supernova problem
4. Stellar weak interaction rates for intermediate-mass nuclei. II - A = 21 to A = 60
5. Stellar weak interaction rates for intermediate mass nuclei. III - Rate tables for the free nucleons and nuclei with A = 21 to A = 60
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