Gamow-Teller strength distributions for nuclei in presupernova stellar cores
Author:
Publisher
American Physical Society (APS)
Subject
Nuclear and High Energy Physics
Link
http://harvest.aps.org/v2/journals/articles/10.1103/PhysRevC.52.3460/fulltext
Reference32 articles.
1. Supernova theory
2. Equation of state in the gravitational collapse of stars
3. Neutron shell blocking of electron capture during gravitational collapse
4. Beta-decay rates of FP shell nuclei with A greater than 60 in massive stars at the presupernova stage
5. Stellar weak interaction rates for intermediate-mass nuclei. II - A = 21 to A = 60
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3. Thermal effects on electron capture for neutron-rich nuclei;Bulletin of the Russian Academy of Sciences: Physics;2009-02
4. The gross theory model for neutrino-nucleus cross-section;New Journal of Physics;2008-03-06
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