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

Abstract

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.

Authors:
; ; ; ; ; ; ; ; ;
Publication Date:
Research Org.:
Oak Ridge National Laboratory (ORNL), Oak Ridge, TN (United States). Oak Ridge Leadership Computing Facility (OLCF) and Joint Institute for Computational Sciences (JICS)
Sponsoring Org.:
USDOE Office of Science (SC)
OSTI Identifier:
1201295
Grant/Contract Number:  
AC05-00OR22725
Resource Type:
Accepted Manuscript
Journal Name:
The Astrophysical Journal. Letters (Online)
Additional Journal Information:
Journal Name: The Astrophysical Journal. Letters (Online); Journal Volume: 807; Journal Issue: 2; Journal ID: ISSN 2041-8213
Publisher:
Institute of Physics (IOP)
Country of Publication:
United States
Language:
English
Subject:
79 ASTRONOMY AND ASTROPHYSICS

Citation Formats

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, and Yakunin, Konstantin N. Three dimensional core-collapse supernova simulated using a 15 M⊙ progenitor. United States: N. p., 2015. Web. doi:10.1088/2041-8205/807/2/l31.
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. Three dimensional core-collapse supernova simulated using a 15 M⊙ progenitor. United States. https://doi.org/10.1088/2041-8205/807/2/l31
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, and Yakunin, Konstantin N. Fri . "Three dimensional core-collapse supernova simulated using a 15 M⊙ progenitor". United States. https://doi.org/10.1088/2041-8205/807/2/l31. https://www.osti.gov/servlets/purl/1201295.
@article{osti_1201295,
title = {Three dimensional core-collapse supernova simulated using a 15 M⊙ progenitor},
author = {Lentz, Eric J. and Bruenn, Stephen W. and Hix, W. Raphael and Mezzacappa, Anthony and Messer, O. E. Bronson and Endeve, Eirik and Blondin, John M. and Harris, J. Austin and Marronetti, Pedro and Yakunin, Konstantin N.},
abstractNote = {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.},
doi = {10.1088/2041-8205/807/2/l31},
journal = {The Astrophysical Journal. Letters (Online)},
number = 2,
volume = 807,
place = {United States},
year = {Fri Jul 10 00:00:00 EDT 2015},
month = {Fri Jul 10 00:00:00 EDT 2015}
}

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Self-induced flavor conversion of supernova neutrinos on small scales
text, January 2015


Shock-Turbulence Interaction in Core-Collapse Supernovae
text, January 2016


Gravitational Wave Signals from 3D Neutrino Hydrodynamics Simulations of Core-Collapse Supernovae
text, January 2016


Flavor-dependent neutrino angular distribution in core-collapse supernovae
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Simulations of core-collapse supernovae in spatial axisymmetry with full Boltzmann neutrino transport
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Muon Creation in Supernova Matter Facilitates Neutrino-driven Explosions
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text, January 2017


Parameterizing the Supernova Engine and its Effects on Remnants and Basic Yields
text, January 2017


Impact of Neutrino Opacities on Core-Collapse Supernova Simulations
text, January 2018


Revival of the Fittest: Exploding Core-Collapse Supernovae from 12 to 25 M$_{\odot}$
text, January 2018


The Morphologies and Kinematics of Supernova Remnants
text, January 2018


Core collapse with magnetic fields and rotation
text, January 2018


Dynamics of supernova bounce in laboratory
text, January 2018


Effects of rotation and magnetic field on the revival of a stalled shock in supernova explosions
text, January 2018


A Successful 3D Core-Collapse Supernova Explosion Model
text, January 2018


Characterizing the Gravitational Wave Signal from Core-Collapse Supernovae
text, January 2018


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Turbulence Generation by Shock-Acoustic-Wave Interaction in Core-Collapse Supernovae
preprint, January 2018


Core collapse with magnetic fields and rotation
text, January 2018


Physical, numerical, and computational challenges of modeling neutrino transport in core-collapse supernovae
preprint, January 2020