Dr James Keegans J.D.Keegans@hull.ac.uk
Type Ia Supernova Nucleosynthesis: Metallicity-dependent Yields
Keegans, James D.; Pignatari, Marco; Stancliffe, Richard J.; Travaglio, Claudia; Jones, Samuel; Gibson, Brad K.; Townsley, Dean M.; Miles, Broxton J.; Shen, Ken J.; Few, Gareth
Authors
Marco Pignatari
Richard J. Stancliffe
Claudia Travaglio
Samuel Jones
Brad K. Gibson
Dean M. Townsley
Broxton J. Miles
Ken J. Shen
Dr Gareth Few G.Few@hull.ac.uk
Lecturer
Abstract
Type Ia supernova explosions (SN Ia) are fundamental sources of elements for the chemical evolution of galaxies. They efficiently produce intermediate-mass (with Z between 11 and 20) and iron group elements - for example, about 70% of the solar iron is expected to be made by SN Ia. In this work, we calculate complete abundance yields for 39 models of SN Ia explosions, based on three progenitors - a 1.4 M ⊙ deflagration detonation model, a 1.0 M ⊙ double detonation model, and a 0.8 M ⊙ double detonation model - and 13 metallicities, with 22Ne mass fractions of 0, 1 × 10-7, 1 × 10-6, 1 × 10-5, 1 × 10-4, 1 × 10-3, 2 × 10-3, 5 × 10-3, 1 × 10-2, 1.4 × 10-2, 5 × 10-2, and 0.1, respectively. Nucleosynthesis calculations are done using the NuGrid suite of codes, using a consistent nuclear reaction network between the models. Complete tables with yields and production factors are provided online at Zenodo:Yields (https://doi.org/10.5281/zenodo.8060323). We discuss the main properties of our yields in light of the present understanding of SN Ia nucleosynthesis, depending on different progenitor mass and composition. Finally, we compare our results with a number of relevant models from the literature.
Citation
Keegans, J. D., Pignatari, M., Stancliffe, R. J., Travaglio, C., Jones, S., Gibson, B. K., Townsley, D. M., Miles, B. J., Shen, K. J., & Few, G. (2023). Type Ia Supernova Nucleosynthesis: Metallicity-dependent Yields. Astrophysical Journal Supplement, 268(1), Article 8. https://doi.org/10.3847/1538-4365/ace102
Journal Article Type | Article |
---|---|
Acceptance Date | Jun 20, 2023 |
Online Publication Date | Aug 22, 2023 |
Publication Date | Sep 1, 2023 |
Deposit Date | Jun 26, 2024 |
Publicly Available Date | Jun 27, 2024 |
Journal | Astrophysical Journal, Supplement Series |
Print ISSN | 0067-0049 |
Publisher | American Astronomical Society |
Peer Reviewed | Peer Reviewed |
Volume | 268 |
Issue | 1 |
Article Number | 8 |
DOI | https://doi.org/10.3847/1538-4365/ace102 |
Keywords | Type Ia supernovae; Nucleosynthesis; Astrophysical explosive burning; Nuclear astrophysics |
Public URL | https://hull-repository.worktribe.com/output/4395414 |
Files
Published article
(1.9 Mb)
PDF
Publisher Licence URL
http://creativecommons.org/licenses/by/4.0
Copyright Statement
© 2023. 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.
You might also like
New Experimental 23Na(α, p)26Mg Reaction Rate for Massive Star and Type Ia Supernova Models
(2021)
Journal Article
Exploring the link between star and planet formation with Ariel
(2021)
Journal Article
A Large-scale Approach to Modeling Molecular Biosignatures: The Diatomics
(2022)
Journal Article
UVES analysis of red giants in the bulge globular cluster NGC 6522
(2021)
Journal Article
Downloadable Citations
About Repository@Hull
Administrator e-mail: repository@hull.ac.uk
This application uses the following open-source libraries:
SheetJS Community Edition
Apache License Version 2.0 (http://www.apache.org/licenses/)
PDF.js
Apache License Version 2.0 (http://www.apache.org/licenses/)
Font Awesome
SIL OFL 1.1 (http://scripts.sil.org/OFL)
MIT License (http://opensource.org/licenses/mit-license.html)
CC BY 3.0 ( http://creativecommons.org/licenses/by/3.0/)
Powered by Worktribe © 2024
Advanced Search