Nuclear statistical equilibrium at core-collapse supernova

Details Nuclear statistical equilibrium at core-collapse supernova Nuclear statistical equilibrium at core-collapse supernova

Oct 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007chphy..16.3146l&link_type=abstract

Chinese Physics, Volume 16, Issue 10, pp. 3146-3149 (2007).

Physics

4

Scientific paper

A new improved nuclear partition function is employed to calculate the nuclear statistical equilibrium (NSE) in core-collapse supernova environment. The results show that the change of nucleus abundance is slight even though the temperature is higher than 1011 K when shock propagates, which indicates that the effect of the nuclear partition function is not so important as shown in the previous calculations, but it can also be considered in detailed simulation if it is sensitive to weak interaction rates in core-collapse supernova.

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