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Galactic Chemical Evolution of Radioactive Isotopes with an s-process Contribution

Trueman, Thomas C. L.; Côté, Benoit; Yagüe López, Andrés; Den Hartogh, Jacqueline; Pignatari, Marco; Soós, Benjámin; Karakas, Amanda I.; Lugaro, Maria

Authors

Thomas C. L. Trueman

Benoit Côté

Andrés Yagüe López

Jacqueline Den Hartogh

Marco Pignatari

Benjámin Soós

Amanda I. Karakas

Maria Lugaro



Abstract

Analysis of inclusions in primitive meteorites reveals that several short-lived radionuclides (SLRs) with half-lives of 0.1-100 Myr existed in the early solar system (ESS). We investigate the ESS origin of 107Pd, 135Cs, and 182Hf, which are produced by slow neutron captures (the s-process) in asymptotic giant branch (AGB) stars. We modeled the Galactic abundances of these SLRs using the OMEGA+ galactic chemical evolution (GCE) code and two sets of mass- and metallicity-dependent AGB nucleosynthesis yields (Monash and FRUITY). Depending on the ratio of the mean-life τ of the SLR to the average length of time between the formations of AGB progenitors γ, we calculate timescales relevant for the birth of the Sun. If τ/γ ⪆ 2, we predict self-consistent isolation times between 9 and 26 Myr by decaying the GCE predicted 107Pd/108Pd, 135Cs/133Cs, and 182Hf/180Hf ratios to their respective ESS ratios. The predicted 107Pd/182Hf ratio indicates that our GCE models are missing 9%-73% of 107Pd and 108Pd in the ESS. This missing component may have come from AGB stars of higher metallicity than those that contributed to the ESS in our GCE code. If τ/γ ≲ 0.3, we calculate instead the time (T LE) from the last nucleosynthesis event that added the SLRs into the presolar matter to the formation of the oldest solids in the ESS. For the 2 M o˙, Z = 0.01 Monash model we find a self-consistent solution of T LE = 25.5 Myr.

Citation

Trueman, T. C. L., Côté, B., Yagüe López, A., Den Hartogh, J., Pignatari, M., Soós, B., Karakas, A. I., & Lugaro, M. (2022). Galactic Chemical Evolution of Radioactive Isotopes with an s-process Contribution. The Astrophysical journal, 924(1), 10. https://doi.org/10.3847/1538-4357/ac31b0

Journal Article Type Article
Acceptance Date Oct 20, 2021
Online Publication Date Jan 5, 2022
Publication Date Jan 1, 2022
Deposit Date Jan 22, 2022
Publicly Available Date Jan 24, 2022
Journal Astrophysical Journal
Print ISSN 0004-637X
Electronic ISSN 1538-4357
Publisher American Astronomical Society
Peer Reviewed Peer Reviewed
Volume 924
Issue 1
Pages 10
DOI https://doi.org/10.3847/1538-4357/ac31b0
Keywords Space and Planetary Science; Astronomy and Astrophysics
Public URL https://hull-repository.worktribe.com/output/3916147
Additional Information Article Title: Galactic Chemical Evolution of Radioactive Isotopes with an s-process Contribution; Journal Title: The Astrophysical Journal; Article Type: paper; Copyright Information: © 2022. The Author(s). Published by the American Astronomical Society.; Date Received: 2021-04-30; Date Accepted: 2021-10-19; Online publication date: 2022-01-05

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Copyright Statement
© 2022. The Author(s). Published by the American Astronomical Society.
Original content from this work may be used under the terms of the Creative Commons Attribution 4.0 licence. Any further distribution of this work must maintain attribution to the author(s) and the title of the work, journal citation and DOI.






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