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Chromium Nucleosynthesis and Silicon-Carbon Shell Mergers in Massive Stars

Côté, Benoit; Jones, Samuel; Herwig, Falk; Pignatari, Marco

Authors

Benoit Côté

Samuel Jones

Falk Herwig



Abstract

We analyze the production of the element Cr in galactic chemical evolution (GCE) models using the NuGrid nucleosynthesis yields set. We show that the unusually large [Cr/Fe] abundance at [Fe/H] ≈ 0 reported by previous studies using those yields and predicted by our Milky Way model originates from the merging of convective Si-burning and C-burning shells in a 20 {M}_{\odot } model at metallicity Z = 0.01, about an hour before the star explodes. This merger mixes the incomplete burning material in the Si shell, including 51V and 52Cr, out to the edge of the carbon/oxygen (CO) core. The adopted supernova model ejects the outer 2 {M}_{\odot } of the CO core, which includes a significant fraction of the Cr-rich material. When including this 20 M ⊙ model at Z = 0.01 in the yields interpolation scheme of our GCE model for stars between 15 and 25 {M}_{\odot }, we overestimate [Cr/Fe] by an order of magnitude at [Fe/H] ≈ 0 relative to observations in the Galactic disk. This raises a number of questions regarding the occurrence of Si–C shell mergers in nature, the accuracy of different simulation approaches, and the impact of such mergers on the presupernova structure and explosion dynamics. According to the conditions in this 1D stellar model, the substantial penetration of C-shell material into the Si shell could launch a convective–reactive global oscillation if a merger does take place. In any case, GCE provides stringent constraints on the outcome of this stellar evolution phase.

Citation

Côté, B., Jones, S., Herwig, F., & Pignatari, M. (2020). Chromium Nucleosynthesis and Silicon-Carbon Shell Mergers in Massive Stars. The Astrophysical journal, 892(1), https://doi.org/10.3847/1538-4357/ab77ac

Journal Article Type Article
Acceptance Date Feb 17, 2020
Online Publication Date Mar 27, 2020
Publication Date Mar 20, 2020
Deposit Date Mar 31, 2020
Publicly Available Date Apr 1, 2020
Journal Astrophysical Journal
Print ISSN 0004-637X
Electronic ISSN 1538-4357
Publisher American Astronomical Society
Peer Reviewed Peer Reviewed
Volume 892
Issue 1
Article Number 57
DOI https://doi.org/10.3847/1538-4357/ab77ac
Keywords Galaxy chemical evolution; Chemical enrichment; Stellar abundances; Massive stars ; Chemical abundances; Stellar nucleosynthesis; Galaxy abundances; Stellar evolutionary models
Public URL https://hull-repository.worktribe.com/output/3482228
Publisher URL https://iopscience.iop.org/article/10.3847/1538-4357/ab77ac
Additional Information Journal title: The Astrophysical Journal; Article type: paper; Article title: Chromium Nucleosynthesis and Silicon–Carbon Shell Mergers in Massive Stars; Copyright information: © 2020. The American Astronomical Society. All rights reserved.; Date received: 2019-06-11; Date accepted: 2020-02-17; Online publication date: 2020-03-27

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Copyright Statement
© 2020. The American Astronomical Society.







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