Georgios Magkotsios
44Ti and 56Ni in core-collapse supernovae
Magkotsios, Georgios; Timmes, Francis X.; Wiescher, Michael; Fryer, Christopher L.; Hungerford, Aimee; Young, Patrick; Bennett, Michael; Diehl, Steven; Herwig, Falk; Hirschi, Raphael; Pignatari, Marco; Rockefeller, Gabriel
Authors
Francis X. Timmes
Michael Wiescher
Christopher L. Fryer
Aimee Hungerford
Patrick Young
Michael Bennett
Steven Diehl
Falk Herwig
Raphael Hirschi r.hirschi@keele.ac.uk
Marco Pignatari
Gabriel Rockefeller
Abstract
We investigate the physical conditions where 44Ti and 56Ni are created in core-collapse supernovae. In this preliminary work we use a series of post-processing network calculations with parametrized expansion profiles that are representative of the wide range of temperatures, densities and electron-to-baryon ratios found in 3D supernova simulations. Critical flows that affect the final yields of 44Ti and 56Ni are assessed.
Citation
Magkotsios, G., Timmes, F. X., Wiescher, M., Fryer, C. L., Hungerford, A., Young, P., Bennett, M., Diehl, S., Herwig, F., Hirschi, R., Pignatari, M., & Rockefeller, G. (2008, July). 44Ti and 56Ni in core-collapse supernovae. Paper presented at 10th Symposium on Nuclei in the Cosmos, Mackinac Island, Michigan, USA
Presentation Conference Type | Conference Paper (unpublished) |
---|---|
Conference Name | 10th Symposium on Nuclei in the Cosmos |
Start Date | Jul 27, 2008 |
End Date | Aug 1, 2008 |
Publication Date | Nov 28, 2008 |
Public URL | https://keele-repository.worktribe.com/output/404364 |
Publisher URL | http://arxiv.org/abs/0811.4651v1 |
Related Public URLs | https://pos.sissa.it/053/ |
Files
0811.4651v1.pdf
(478 Kb)
PDF
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