PUSHing Core-collapse Supernovae to Explosions in Spherical Symmetry. III. Nucleosynthesis Yields

Curtis, Sanjana; Ebinger, Kevin; Fröhlich, Carla; Hempel, Matthias; Perego, Albino; Liebendörfer, Matthias; Thielemann, Friedrich-Karl

doi:10.3847/1538-4357/aae7d2

PUSHing Core-collapse Supernovae to Explosions in Spherical Symmetry. III. Nucleosynthesis Yields

Journal Article · Thu Dec 27 00:00:00 EST 2018 · The Astrophysical Journal (Online)

DOI:https://doi.org/10.3847/1538-4357/aae7d2· OSTI ID:1611371

^[1]; Ebinger, Kevin ^[2]; ^[3]; Hempel, Matthias ^[4]; ^[5]; Liebendörfer, Matthias ^[4]; Thielemann, Friedrich-Karl ^[6]

North Carolina State Univ., Raleigh, NC (United States); DOE/OSTI
North Carolina State Univ., Raleigh, NC (United States); GSI-Helmholtzzentrum fur Schwerionenforschung, Darmstadt (Germany)
North Carolina State Univ., Raleigh, NC (United States)
Univ. of Basel (Switzerland)
Istituto Nazionale di Fisica Nucleare (INFN), Parma (Italy); Univ. degli Studi di Milano (Italy); Univ. of Parma (Italy)
GSI-Helmholtzzentrum fur Schwerionenforschung, Darmstadt (Germany); Univ. of Basel (Switzerland)

In a previously presented proof-of-principle study, we established a parameterized spherically symmetric explosion method (PUSH) that can reproduce many features of core-collapse supernovae (CCSNe) for a wide range of preexplosion models. The method is based on the neutrino-driven mechanism and follows collapse, bounce, and explosion. There are two crucial aspects of our model for nucleosynthesis predictions. First, the mass cut and explosion energy emerge simultaneously from the simulation (determining, for each stellar model, the amount of Fe-group ejecta). Second, the interactions between neutrinos and matter are included consistently (setting the electron fraction of the innermost ejecta). In the present paper, we use the successful explosion models from Ebinger et al. that include two sets of pre-explosion models at solar metallicity, with combined masses between 10.8 and 120 M_⊙. We perform systematic nucleosynthesis studies and predict detailed isotopic yields. The resulting 56Ni ejecta are in overall agreement with observationally derived values from normal CCSNe. The Fe-group yields are also in agreement with derived abundances for metal-poor star HD 84937. We also present a comparison of our results with observational trends in alpha element to iron ratios.

View Accepted Manuscript (DOE)

Research Organization:: North Carolina State Univ., Raleigh, NC (United States)

Sponsoring Organization:: USDOE Office of Science (SC)

Grant/Contract Number:: SC0010263

OSTI ID:: 1611371

Journal Information:: The Astrophysical Journal (Online), Journal Name: The Astrophysical Journal (Online) Journal Issue: 1 Vol. 870; ISSN 1538-4357

Publisher:: Institute of Physics (IOP)Copyright Statement

Country of Publication:: United States

Language:: English

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High-Resolution Spectroscopic Study of Extremely Metal-Poor Star Candidates from the SkyMapper Survey Jacobson, Heather. R.; Keller, Stefan; Frebel, Anna arXiv https://doi.org/10.48550/arxiv.1504.03344	text	January 2015
Neutrino-driven explosion of a 20 solar-mass star in three dimensions enabled by strange-quark contributions to neutrino-nucleon scattering Melson, Tobias; Janka, Hans-Thomas; Bollig, Robert arXiv https://doi.org/10.48550/arxiv.1504.07631	text	January 2015
Three-dimensional core-collapse supernova simulated using a 15 $M_\odot$ progenitor Lentz, Eric J.; Bruenn, Stephen W.; Hix, W. Raphael arXiv https://doi.org/10.48550/arxiv.1505.05110	text	January 2015
High-resolution spectroscopic studies of ultra metal-poor stars found in LAMOST survey Li, Haining; Aoki, Wako; Zhao, Gang arXiv https://doi.org/10.48550/arxiv.1506.05684	text	January 2015
Extremely metal-poor stars from the cosmic dawn in the bulge of the Milky Way Howes, L. M.; Casey, A. R.; Asplund, M. arXiv https://doi.org/10.48550/arxiv.1511.03930	text	January 2015
The Multi-Dimensional Character of Core-Collapse Supernovae Hix, W. R.; Lentz, E. J.; Bruenn, S. W. arXiv https://doi.org/10.48550/arxiv.1602.05553	text	January 2016
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Implications for Post-Processing Nucleosynthesis of Core-Collapse Supernova Models with Lagrangian Particles Harris, J. Austin; Hix, W. Raphael; Chertkow, Merek A. arXiv https://doi.org/10.48550/arxiv.1701.08876	text	January 2017
Very Low Energy Supernovae: Light Curves and Spectra of Shock Breakout Lovegrove, Elizabeth; Woosley, S. E.; Zhang, Weiqun arXiv https://doi.org/10.48550/arxiv.1706.02440	text	January 2017
Nucleosynthesis in 2D Core-Collapse Supernovae of 11.2 and 17.0 M$_{\odot}$ Progenitors: Implications for Mo and Ru Production Eichler, M.; Nakamura, K.; Takiwaki, T. arXiv https://doi.org/10.48550/arxiv.1708.08393	text	January 2017
JINAbase: A database for chemical abundances of metal-poor stars Abohalima, Abdu; Frebel, Anna arXiv https://doi.org/10.48550/arxiv.1711.04410	text	January 2017
Conservative General Relativistic Radiation Hydrodynamics in Spherical Symmetry and Comoving Coordinates Liebendoerfer, Matthias; Mezzacappa, Anthony; Thielemann, Friedrich-Karl arXiv https://doi.org/10.48550/arxiv.astro-ph/0012201	text	January 2000
Nucleosynthesis of Zinc and Iron-Peak Elements in Pop III Type II Supernovae : Comparison with abundances of Very Metal-Poor Halo Stars Umeda, Hideyuki; Nomoto, Ken'ichi arXiv https://doi.org/10.48550/arxiv.astro-ph/0103241	text	January 2001
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First stars V - Abundance patterns from C to Zn and supernova yields in the early Galaxy Cayrel, R.; Depagne, E.; Spite, M. arXiv https://doi.org/10.48550/arxiv.astro-ph/0311082	text	January 2003
Composition of the Innermost Core Collapse Supernova Ejecta Frohlich, C.; Hauser, P.; Liebendoerfer, M. arXiv https://doi.org/10.48550/arxiv.astro-ph/0410208	text	January 2004
Effects of rotation on the revival of a stalled shock in supernova explosions Yamasaki, T.; Yamada, S. arXiv https://doi.org/10.48550/arxiv.astro-ph/0412625	text	January 2004
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The rp-Process in Neutrino-driven Winds Wanajo, Shinya arXiv https://doi.org/10.48550/arxiv.astro-ph/0602488	text	January 2006
Nucleosynthesis Yields of Core-Collapse Supernovae and Hypernovae, and Galactic Chemical Evolution Nomoto, Ken'ichi; Tominaga, Nozomu; Umeda, Hideyuki arXiv https://doi.org/10.48550/arxiv.astro-ph/0605725	text	January 2006
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