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Title: The 13C-Pocket Structure In AGB Models: Constraints From Zirconium Isotope Abundances In Single Mainstream SiC Grains

Abstract

In this paper, 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. Finally, 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.

Authors:
ORCiD logo [1]; ORCiD logo [2];  [3]; ORCiD logo [4];  [5];  [6]
  1. Univ. of Chicago, IL (United States). Dept. of the Geophysical Sciences; Chicago Center for Cosmochemistry, Chicago, IL (United States); Argonne National Lab. (ANL), Argonne, IL (United States). Materials Science Division
  2. Univ. of Turin (Italy). Dept. of Physics
  3. Univ. of Turin (Italy). Dept. of Physics; The INAF Astrophysical Observatory of Turin (Italy)
  4. Univ. of Chicago, IL (United States). Dept. of the Geophysical Sciences. Enrico Fermi Inst.; Chicago Center for Cosmochemistry, Chicago, IL (United States)
  5. Chicago Center for Cosmochemistry, Chicago, IL (United States); Argonne National Lab. (ANL), Argonne, IL (United States). Materials Science Division
  6. Univ. of Chicago, IL (United States). Dept. of the Geophysical Sciences. Enrico Fermi Inst.; Chicago Center for Cosmochemistry, Chicago, IL (United States); Argonne National Lab. (ANL), Argonne, IL (United States). Materials Science Division
Publication Date:
Research Org.:
Univ. of Chicago, IL (United States); Univ. of Turin (Italy); Argonne National Lab. (ANL), Argonne, IL (United States)
Sponsoring Org.:
USDOE; National Aeronautics and Space Administration (NASA); Joint Inst. for Nuclear Astrophysics (JINA) (United States); Karlsruhe Inst. of Technology (KIT) (Germany)
Contributing Org.:
Chicago Center for Cosmochemistry, Chicago, IL (United States); The INAF Astrophysical Observatory of Turin (Italy)
OSTI Identifier:
1357464
Grant/Contract Number:  
AC02-06CH11357; NNX11AN63H; NNX09AG39G
Resource Type:
Accepted Manuscript
Journal Name:
The Astrophysical Journal
Additional Journal Information:
Journal Volume: 788; Journal Issue: 2; Journal ID: ISSN 0004-637X
Publisher:
Institute of Physics (IOP)
Country of Publication:
United States
Language:
English
Subject:
79 ASTRONOMY AND ASTROPHYSICS; circumstellar matter; meteorites, meteors, meteoroids; nuclear reactions, nucleosynthesis, abundances; stars abundances; AGB and post-AGB stars

Citation Formats

Liu, Nan, Gallino, Roberto, Bisterzo, Sara, Davis, Andrew M., Savina, Michael R., and Pellin, Michael J. The 13C-Pocket Structure In AGB Models: Constraints From Zirconium Isotope Abundances In Single Mainstream SiC Grains. United States: N. p., 2014. Web. doi:10.1088/0004-637X/788/2/163.
Liu, Nan, Gallino, Roberto, Bisterzo, Sara, Davis, Andrew M., Savina, Michael R., & Pellin, Michael J. The 13C-Pocket Structure In AGB Models: Constraints From Zirconium Isotope Abundances In Single Mainstream SiC Grains. United States. https://doi.org/10.1088/0004-637X/788/2/163
Liu, Nan, Gallino, Roberto, Bisterzo, Sara, Davis, Andrew M., Savina, Michael R., and Pellin, Michael J. Wed . "The 13C-Pocket Structure In AGB Models: Constraints From Zirconium Isotope Abundances In Single Mainstream SiC Grains". United States. https://doi.org/10.1088/0004-637X/788/2/163. https://www.osti.gov/servlets/purl/1357464.
@article{osti_1357464,
title = {The 13C-Pocket Structure In AGB Models: Constraints From Zirconium Isotope Abundances In Single Mainstream SiC Grains},
author = {Liu, Nan and Gallino, Roberto and Bisterzo, Sara and Davis, Andrew M. and Savina, Michael R. and Pellin, Michael J.},
abstractNote = {In this paper, 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. Finally, 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.},
doi = {10.1088/0004-637X/788/2/163},
journal = {The Astrophysical Journal},
number = 2,
volume = 788,
place = {United States},
year = {Wed Jun 04 00:00:00 EDT 2014},
month = {Wed Jun 04 00:00:00 EDT 2014}
}

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