s-Process Branching at 186Re, the Abundance of 186Os, and Presolar Grains

Details s-Process Branching at 186Re, the Abundance of 186Os, and Presolar Grains s-Process Branching at 186Re, the Abundance of 186Os, and Presolar Grains

Mar 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007lpi....38.2055m&link_type=abstract

38th Lunar and Planetary Science Conference, (Lunar and Planetary Science XXXVIII), held March 12-16, 2007 in League City, Texas

Physics

3

Scientific paper

Current s-process models overproduce 186Os while s-process carrying
presolar grains apparently have lower 186Os/188Os abundance ratios than
s-process models predict. We explore possible resolutions to these two
puzzles.

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