The overarching framework of core-collapse supernova explosions as revealed by 3D fornax simulations

Burrows, Adam; Radice, David; Vartanyan, David; Nagakura, Hiroki; Skinner, M Aaron; Dolence, Joshua C

doi:10.1093/mnras/stz3223

Title: The overarching framework of core-collapse supernova explosions as revealed by 3D fornax simulations

Journal Article · Thu Nov 28 00:00:00 EST 2019 · Monthly Notices of the Royal Astronomical Society

DOI:https://doi.org/10.1093/mnras/stz3223· OSTI ID:1643757

Burrows, Adam ^[1];

^[2]; Vartanyan, David ^[1]; Nagakura, Hiroki ^[1]; Skinner, M Aaron ^[3]; Dolence, Joshua C ^[4]

Princeton Univ., NJ (United States)
Princeton Univ., NJ (United States); Pennsylvania State Univ., University Park, PA (United States)
Lawrence Livermore National Lab. (LLNL), Livermore, CA (United States)
Los Alamos National Lab. (LANL), Los Alamos, NM (United States)

We have conducted 19 state-of-the-art 3D core-collapse supernova simulations spanning a broad range of progenitor masses. This is the largest collection of sophisticated 3D supernova simulations ever performed. We have found that while the majority of these models explode, not all do, and that even models in the middle of the available progenitor mass range may be less explodable. This does not mean that those models for which we did not witness explosion would not explode in Nature, but that they are less prone to explosion than others. One consequence is that the ‘compactness’ measure is not a metric for explodability. We find that lower-mass massive star progenitors likely experience lower-energy explosions, while the higher-mass massive stars likely experience higher-energy explosions. Moreover, most 3D explosions have a dominant dipole morphology, have a pinched, wasp-waist structure, and experience simultaneous accretion and explosion. We reproduce the general range of residual neutron-star masses inferred for the galactic neutron-star population. The most massive progenitor models, however, in particular vis à vis explosion energy, need to be continued for longer physical times to asymptote to their final states. We find that while the majority of the inner ejecta have Ye = 0.5, there is a substantial proton-rich tail. This result has important implications for the nucleosynthetic yields as a function of progenitor. Finally, we find that the non-exploding models eventually evolve into compact inner configurations that experience a quasi-periodic spiral SASI mode. We otherwise see little evidence of the SASI in the exploding models.

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Research Organization:: Lawrence Livermore National Laboratory (LLNL), Livermore, CA (United States); Los Alamos National Laboratory (LANL), Los Alamos, NM (United States)

Sponsoring Organization:: USDOE National Nuclear Security Administration (NNSA); USDOE Laboratory Directed Research and Development (LDRD) Program; National Science Foundation (NSF); Extreme Science and Engineering Discovery Environment (XSEDE)

Grant/Contract Number:: AC52-07NA27344; SC0018297; AST-1714267; PHY-1144374; AC02-06CH11357; TG-AST170045; AC03-76SF00098; 89233218CNA000001

OSTI ID:: 1643757

Alternate ID(s):: OSTI ID: 1657130

Report Number(s):: LLNL-JRNL-787982; LA-UR-19-28512; 1365-2966; 986006; TRN: US2201965

Journal Information:: Monthly Notices of the Royal Astronomical Society, Vol. 491, Issue 2; ISSN 0035-8711

Publisher:: Royal Astronomical SocietyCopyright Statement

Country of Publication:: United States

Language:: English

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Cited by: 122 works

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Core-collapse supernova equations of state based on neutron star observations Steiner, Andrew W.; Hempel, Matthias; Fischer, Tobias arXiv https://doi.org/10.48550/arxiv.1207.2184	text	January 2012
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Linear analysis on the growth of non-spherical perturbations in supersonic accretion flows Takahashi, Kazuya; Yamada, Shoichi arXiv https://doi.org/10.48550/arxiv.1408.3503	text	January 2014
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Revival of the Fittest: Exploding Core-Collapse Supernovae from 12 to 25 M$_{\odot}$ Vartanyan, David; Burrows, Adam; Radice, David arXiv https://doi.org/10.48550/arxiv.1801.08148	text	January 2018
Survey of astrophysical conditions in neutrino-driven supernova ejecta nucleosynthesis Bliss, Julia; Witt, Maximilian; Arcones, Almudena arXiv https://doi.org/10.48550/arxiv.1802.00737	text	January 2018
Production of Mo and Ru isotopes in neutrino-driven winds: implications for solar abundances and presolar grains Bliss, Julia; Arcones, Almudena; Qian, Yong-Zhong arXiv https://doi.org/10.48550/arxiv.1804.03947	text	January 2018
Exploring Fundamentally Three-dimensional Phenomena in High-fidelity Simulations of Core-collapse Supernovae O'Connor, Evan; Couch, Sean arXiv https://doi.org/10.48550/arxiv.1807.07579	text	January 2018
A Successful 3D Core-Collapse Supernova Explosion Model Vartanyan, David; Burrows, Adam; Radice, David arXiv https://doi.org/10.48550/arxiv.1809.05106	text	January 2018
Three-Dimensional Core-Collapse Supernova Simulations with Multi-Dimensional Neutrino Transport Compared to the Ray-by-Ray-plus Approximation Glas, Robert; Just, Oliver; Janka, H. -Thomas arXiv https://doi.org/10.48550/arxiv.1809.10146	text	January 2018
Characterizing the Gravitational Wave Signal from Core-Collapse Supernovae Radice, David; Morozova, Viktoriya; Burrows, Adam arXiv https://doi.org/10.48550/arxiv.1812.07703	text	January 2018
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Comparing treatments of weak reactions with nuclei in simulations of core-collapse supernovae Nagakura, Hiroki; Furusawa, Shun; Togashi, Hajime arXiv https://doi.org/10.48550/arxiv.1812.09811	text	January 2018
The Evolution of Massive Helium Stars Including Mass Loss Woosley, S. E. arXiv https://doi.org/10.48550/arxiv.1901.00215	text	January 2019
One-, Two-, and Three-dimensional Simulations of Oxygen Shell Burning Just Before the Core-Collapse of Massive Stars Yoshida, Takashi; Takiwaki, Tomoya; Kotake, Kei arXiv https://doi.org/10.48550/arxiv.1903.07811	text	January 2019
Mass discrepancy analysis for a select sample of Type II-Plateau supernovae Martinez, Laureano; Bersten, Melina C. arXiv https://doi.org/10.48550/arxiv.1908.01828	text	January 2019
General Relativistic Effects in the Core Collapse Supernova Mechanism Bruenn, S. W.; De Nisco, K. R.; Mezzacappa, A. arXiv https://doi.org/10.48550/arxiv.astro-ph/0101400	text	January 2001
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Stability of Standing Accretion Shocks, With an Eye Toward Core Collapse Supernovae Blondin, John M.; Mezzacappa, Anthony; DeMarino, Christine arXiv https://doi.org/10.48550/arxiv.astro-ph/0210634	text	January 2002
Shock Breakout in Core-Collapse Supernovae and its Neutrino Signature Thompson, Todd A.; Burrows, Adam; Pinto, Philip A. arXiv https://doi.org/10.48550/arxiv.astro-ph/0211194	text	January 2002
Multi-Dimensional Radiation/Hydrodynamic Simulations of Protoneutron Star Convection Dessart, L.; Burrows, A.; Livne, E. arXiv https://doi.org/10.48550/arxiv.astro-ph/0510229	text	January 2005
Neutron Star Observations: Prognosis for Equation of State Constraints Lattimer, James M.; Prakash, Maddapa arXiv https://doi.org/10.48550/arxiv.astro-ph/0612440	text	January 2006
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