Detailedβ-transition rates for URCA nuclear pairs in 8–10 solar-mass stars
Author:
Publisher
American Physical Society (APS)
Subject
Nuclear and High Energy Physics
Link
http://harvest.aps.org/v2/journals/articles/10.1103/PhysRevC.88.015806/fulltext
Reference20 articles.
1. Presupernova evolution of massive stars
2. Evolution of 8-10 solar mass stars toward electron capture supernovae. I - Formation of electron-degenerate O + NE + MG cores
3. Evolution of 8-10 solar mass stars toward electron capture supernovae. II - Collapse of an O + NE + MG core
4. Empirical strengths of spin operators in nuclei
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