Three dimensional core-collapse supernova simulated using a 15 M⊙ progenitor

Lentz, Eric J.; Bruenn, Stephen W.; Hix, W. Raphael; Mezzacappa, Anthony; Messer, O. E.  Bronson; Endeve, Eirik; Blondin, John M.; Harris, J. Austin; Marronetti, Pedro; Yakunin, Konstantin N.

doi:10.1088/2041-8205/807/2/l31

Title: Three dimensional core-collapse supernova simulated using a 15 M_⊙ progenitor

Journal Article · Fri Jul 10 00:00:00 EDT 2015 · The Astrophysical Journal. Letters (Online)

DOI:https://doi.org/10.1088/2041-8205/807/2/l31· OSTI ID:1201295

Lentz, Eric J.; Bruenn, Stephen W.; Hix, W. Raphael; Mezzacappa, Anthony; Messer, O. E. Bronson; Endeve, Eirik; Blondin, John M.; Harris, J. Austin; Marronetti, Pedro; Yakunin, Konstantin N.

We have performed ab initio neutrino radiation hydrodynamics simulations in three and two spatial dimensions (3D and 2D) of core-collapse supernovae from the same 15 M⊙ progenitor through 440 ms after core bounce. Both 3D and 2D models achieve explosions; however, the onset of explosion (shock revival) is delayed by ~100 ms in 3D relative to the 2D counterpart and the growth of the diagnostic explosion energy is slower. This is consistent with previously reported 3D simulations utilizing iron-core progenitors with dense mantles. In the ~100 ms before the onset of explosion, diagnostics of neutrino heating and turbulent kinetic energy favor earlier explosion in 2D. During the delay, the angular scale of convective plumes reaching the shock surface grows and explosion in 3D is ultimately lead by a single, large-angle plume, giving the expanding shock a directional orientation not dissimilar from those imposed by axial symmetry in 2D simulations. Finally, we posit that shock revival and explosion in the 3D simulation may be delayed until sufficiently large plumes form, whereas such plumes form more rapidly in 2D, permitting earlier explosions.

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Research Organization:: Oak Ridge National Laboratory (ORNL), Oak Ridge, TN (United States). Oak Ridge Leadership Computing Facility (OLCF) and Joint Institute for Computational Sciences (JICS)

Sponsoring Organization:: USDOE Office of Science (SC)

Grant/Contract Number:: AC05-00OR22725

OSTI ID:: 1201295

Journal Information:: The Astrophysical Journal. Letters (Online), Vol. 807, Issue 2; ISSN 2041-8213

Publisher:: Institute of Physics (IOP)Copyright Statement

Country of Publication:: United States

Language:: English

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Cited by: 205 works

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Self-induced flavor conversion of supernova neutrinos on small scales Chakraborty, Sovan; Hansen, Rasmus Sloth; Izaguirre, Ignacio arXiv https://doi.org/10.48550/arxiv.1507.07569	text	January 2015
Two Dimensional Core-Collapse Supernova Explosions Aided by General Relativity with Multidimensional Neutrino Transport O'Connor, Evan; Couch, Sean arXiv https://doi.org/10.48550/arxiv.1511.07443	text	January 2015
Three-dimensional simulations of rapidly rotating core-collapse supernovae: finding a neutrino-powered explosion aided by non-axisymmetric flows Takiwaki, Tomoya; Kotake, Kei; Suwa, Yudai arXiv https://doi.org/10.48550/arxiv.1602.06759	text	January 2016
Three-dimensional Boltzmann-Hydro code for core-collapse in massive stars II. The Implementation of moving-mesh for neutron star kicks Nagakura, Hiroki; Iwakami, Wakana; Furusawa, Shun arXiv https://doi.org/10.48550/arxiv.1605.00666	text	January 2016
Shock-Turbulence Interaction in Core-Collapse Supernovae Abdikamalov, Ernazar; Zhaksylykov, Azamat; Radice, David arXiv https://doi.org/10.48550/arxiv.1605.09015	text	January 2016
Gravitational Wave Signals from 3D Neutrino Hydrodynamics Simulations of Core-Collapse Supernovae Andresen, Haakon; Mueller, Bernhard; Mueller, Ewald arXiv https://doi.org/10.48550/arxiv.1607.05199	text	January 2016
Flavor-dependent neutrino angular distribution in core-collapse supernovae Tamborra, Irene; Huedepohl, Lorenz; Raffelt, Georg arXiv https://doi.org/10.48550/arxiv.1702.00060	text	January 2017
Simulations of core-collapse supernovae in spatial axisymmetry with full Boltzmann neutrino transport Nagakura, Hiroki; Iwakami, Wakana; Furusawa, Shun arXiv https://doi.org/10.48550/arxiv.1702.01752	text	January 2017
Muon Creation in Supernova Matter Facilitates Neutrino-driven Explosions Bollig, R.; Janka, H. -Th.; Lohs, A. arXiv https://doi.org/10.48550/arxiv.1706.04630	text	January 2017
Rotation-supported Neutrino-driven Supernova Explosions in Three Dimensions and the Critical Luminosity Condition Summa, A.; Janka, H. -Th.; Melson, T. arXiv https://doi.org/10.48550/arxiv.1708.04154	text	January 2017
A physical model of mass ejection in failed supernovae Coughlin, Eric R.; Quataert, Eliot; Fernández, Rodrigo arXiv https://doi.org/10.48550/arxiv.1710.01746	text	January 2017
The state of matter in simulations of core-collapse supernovae -- Reflections and recent developments Fischer, Tobias; Bastian, Niels-Uwe; Blaschke, David arXiv https://doi.org/10.48550/arxiv.1711.07411	text	January 2017
Parameterizing the Supernova Engine and its Effects on Remnants and Basic Yields Fryer, Chris L.; Andrews, Sydney; Even, Wesley arXiv https://doi.org/10.48550/arxiv.1712.03415	text	January 2017
Impact of Neutrino Opacities on Core-Collapse Supernova Simulations Kotake, Kei; Takiwaki, Tomoya; Fischer, Tobias arXiv https://doi.org/10.48550/arxiv.1801.02703	text	January 2018
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
The Morphologies and Kinematics of Supernova Remnants Lopez, Laura A.; Fesen, Robert A. arXiv https://doi.org/10.48550/arxiv.1804.00024	text	January 2018
Core-collapse supernova simulations in one and two dimensions: comparison of codes and approximations Just, Oliver; Bollig, Robert; Janka, Hans-Thomas arXiv https://doi.org/10.48550/arxiv.1805.03953	text	January 2018
Core collapse with magnetic fields and rotation Obergaulinger, M.; Just, O.; Aloy, M. Á. arXiv https://doi.org/10.48550/arxiv.1806.00393	text	January 2018
Dynamics of supernova bounce in laboratory Blinnikov, S. I.; Ilkaev, R. I.; Mochalov, M. A. arXiv https://doi.org/10.48550/arxiv.1806.05398	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
Effects of rotation and magnetic field on the revival of a stalled shock in supernova explosions Fujisawa, Kotaro; Okawa, Hirotada; Yamamoto, Yu arXiv https://doi.org/10.48550/arxiv.1809.04358	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
Effects of the standing accretion-shock instability and the lepton-emission self-sustained asymmetry in the neutrino emission of rotating supernovae Walk, Laurie; Tamborra, Irene; Janka, Hans-Thomas arXiv https://doi.org/10.48550/arxiv.1901.06235	text	January 2019
Three-Dimensional Supernova Explosion Simulations of 9-, 10-, 11-, 12-, and 13-M$_{\odot}$ Stars Burrows, Adam; Radice, David; Vartanyan, David arXiv https://doi.org/10.48550/arxiv.1902.00547	text	January 2019
A Critical Assessment of Turbulence Models for 1D Core-Collapse Supernova Simulations Müller, Bernhard arXiv https://doi.org/10.48550/arxiv.1902.04270	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
Long-term Simulations of Multi-Dimensional Core-collapse Supernovae: Implications for Neutron Star Kicks Nakamura, Ko; Takiwaki, Tomoya; Kotake, Kei arXiv https://doi.org/10.48550/arxiv.1904.08088	text	January 2019
Generalized Kompaneets formalism for inelastic neutrino-nucleon scattering in supernova simulations Wang, Tianshu; Burrows, Adam Physical Review D, Vol. 102, Issue 2 https://doi.org/10.1103/physrevd.102.023017	journal	July 2020
Neutrino Emission from Supernovae Janka, H. -Th. arXiv https://doi.org/10.48550/arxiv.1702.08713	text	January 2017
Neutrino-driven Explosions Janka, H. -Th. arXiv https://doi.org/10.48550/arxiv.1702.08825	text	January 2017
Turbulence Generation by Shock-Acoustic-Wave Interaction in Core-Collapse Supernovae Abdikamalov, E.; Huete, C.; Nussupbekov, A. arXiv https://doi.org/10.48550/arxiv.1805.03957	preprint	January 2018
Hydrodynamics of core-collapse supernovae and their progenitors Müller, B. arXiv https://doi.org/10.48550/arxiv.2006.05083	text	January 2020
Physical, numerical, and computational challenges of modeling neutrino transport in core-collapse supernovae Mezzacappa, Anthony; Endeve, Eirik; Messer, O. E. Bronson arXiv https://doi.org/10.48550/arxiv.2010.09013	preprint	January 2020

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