Abstract
We present postprocess asymptotic giant branch (AGB) nucleosynthesis models with different 13C-pocket internal structures to better explain zirconium isotope measurements in mainstream presolar SiC grains by Nicolussi et al. and Barzyk et al. We show that higher-than-solar 92Zr/ 94Zr ratios can be predicted by adopting a 13C-pocket with a flat 13C profile, instead of the previous decreasing-with-depth 13C profile. The improved agreement between grain data for zirconium isotopes and AGB models provides additional support for a recent proposal of a flat 13C profile based on barium isotopes in mainstream SiC grains by Liu et al. © 2014. The American Astronomical Society. All rights reserved..
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Liu, N., Gallino, R., Bisterzo, S., Davis, A. M., Savina, M. R., & Pellin, M. J. (2014). THE 13C-pocket structure in AGB models: Constraints from zirconium isotope abundances in single mainstream SiC grains. Astrophysical Journal, 788(2). https://doi.org/10.1088/0004-637X/788/2/163
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