Gamow-Teller electron capture strength distributions in stars: Unblocked iron and nickel isotopes

[1]  J. Wambach.  Electron Capture in Stellar Collapse , 1984 .

[2]  S. D. Bloom.  Gamow-teller strength functions with the Lanczos algorithm , 1984 .

[3]  A. Burrows,et al.  The effect of trapped lepton number and entropy on the outcome of stellar collapse , 1983 .

[4]  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 .

[5]  G. Fuller.  Neutron shell blocking of electron capture during gravitational collapse , 1982 .

[6]  S. Grimes,et al.  Gamow-Teller strength function for 26Mg→26Al , 1981 .

[7]  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 .

[8]  A. Watt,et al.  Shell-model calculation of strength functions , 1980 .

[9]  H. Bethe,et al.  Equation of state in the gravitational collapse of stars , 1979 .

[10]  Richard B. Firestone,et al.  Table of Isotopes , 1978 .

[11]  W. Arnett.  Neutrino trapping during gravitational collapse of stars. , 1977 .

[12]  J. Truran,et al.  Electron capture in carbon dwarf supernovae , 1974 .

[13]  P. Goode,et al.  WHY DOES $sup 56$Ni DECAY SO SLOWLY. , 1969 .

[14]  V. A. Madsen,et al.  Finite-Nucleus G Matrix in the Microscopic Description of Inelastic Proton Scattering , 1969 .

[15]  A. Kallio,et al.  An application of the separation method in shell-model calculation , 1964 .

[16]  K. Ikeda.  Collective Excitation of Unlike Pair States in Heavier Nuclei , 1964 .