Electron Capture and Beta-Decay Rates for the Collapse of O+Ne+Mg Cores
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Publisher
EDP Sciences
Link
http://www.epj-conferences.org/10.1051/epjconf/20146607011/pdf
Reference11 articles.
1. Evolution of 8-10 solar mass stars toward electron capture supernovae. I - Formation of electron-degenerate O + NE + MG cores
2. r -Process Nucleosynthesis in Shocked Surface Layers of O-Ne-Mg Cores
3. Rate Tables for the Weak Processes of sd-Shell Nuclei in Stellar Matter
4. Jones S.et al., Astrophys. J.772, 1 (2013).
5. Microscopic calculation of the rates of electron captures which induce the collapse of O+Ne+Mg cores
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1. Do electron-capture supernovae make neutron stars?;Astronomy & Astrophysics;2016-09
2. Modified Fermi energy of electrons in a superhigh magnetic field;Modern Physics Letters A;2016-04-10
3. Numerically fitting the electron Fermi energy and the electron fraction in a neutron star;International Journal of Modern Physics D;2016-01
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