The electron capture of nuclides 55Co and 56Ni in the process of stellar core collapse
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[1] Zhong He,et al. Gaussian modification of neutrino energy loss on strongly screening nuclides 55 Co and 56 Ni by electron capture in stellar interior , 2011 .
[2] Luo Zhi-quan,et al. Neutrino energy loss by electron capture in magnetic field at the crusts of neutron stars , 2008 .
[3] Luo Zhi-quan,et al. Effect of Strong Magnetic Field on Gamow–Teller Transition Electron Capture of Iron Group Nuclei at Crusts of Neutron Stars , 2008 .
[4] 刘晶晶,et al. Neutrino energy loss by electron capture on strongly screened iron group nuclei , 2007 .
[5] 刘晶晶,et al. Effect of strong magnetic field on electron capture of iron group nuclei in crusts of neutron stars , 2007 .
[6] G. Martínez-Pinedo,et al. Supernova electron capture rates for 55Co and 56Ni , 1998, nucl-th/9809081.
[7] A. University,et al. Electron capture on iron group nuclei , 1998, nucl-th/9801012.
[8] S. Woosley,et al. Search for Important Weak Interaction Nuclei in Presupernova Evolution , 1994 .
[9] G. E. Brown,et al. Electron Capture and beta -Decay in Presupernova Stars , 1990 .
[10] B. Labonte. Spectra of plages on the sun and stars. II: The H I Hα line , 1986 .
[11] J. Wambach. Electron Capture in Stellar Collapse , 1984 .
[12] W. Fowler,et al. Stellar weak interaction rates for intermediate mass nuclei. III. Rate tables for the free nucleons and nuclei with A = 21 TO A = 60 , 1982 .
[13] W. Fowler,et al. 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 , 1980 .