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Implications of the recent [sup 59]Co([ital n],[ital p])[sup 59]Fe experiment for stellar electron capture rates

Journal Article · · Physical Review, C (Nuclear Physics); (United States)
; ; ;  [1]
  1. Physics Department, Lawrence Livermore National Laboratory, Livermore, California 94550 (United States)
We study results from the recent measurement of the 0[degree] [sup 59]Co([ital n],[ital p])[sup 59]Fe cross section in order to compute the stellar electron capture rate of [sup 59]Co. This nucleus is the second most important electron capture nucleus in the core of a type II supernova progenitor just before core collapse. It is also the first nucleus which has a large effect on the stellar neutronization rate for which Gamow-Teller strength has been measured. The Gamow-Teller resonance has been observed experimentally at a higher energy above the daughter ground state than one would expect from independent particle shell model arguments, but large-basis shell model calculations employing configuration mixing are more successful in predicting the location of the strength. Because of the high energy of the Gamow-Teller resonance, the stellar electron capture rate and associated neutronization is much less than previous estimates had indicated. Similar trends are seen for [sup 60]Co, the most important electron capture nucleus for supernova progenitors just before core collapse.
OSTI ID:
6497281
Journal Information:
Physical Review, C (Nuclear Physics); (United States), Journal Name: Physical Review, C (Nuclear Physics); (United States) Vol. 47:6; ISSN 0556-2813; ISSN PRVCAN
Country of Publication:
United States
Language:
English