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Title: Crucial Physical Dependencies of the Core-Collapse Supernova Mechanism

Abstract

We explore with self-consistent 2D FORNAX simulations the dependence of the outcome of collapse on many-body corrections to neutrino-nucleon cross sections, the nucleon-nucleon bremsstrahlung rate, electron capture on heavy nuclei, pre-collapse seed perturbations, and inelastic neutrino-electron and neutrino-nucleon scattering. Importantly, proximity to criticality amplifies the role of even small changes in the neutrino-matter couplings, and such changes can together add to produce outsized effects. When close to the critical condition the cumulative result of a few small effects (including seeds) that individually have only modest consequence can convert an anemic into a robust explosion, or even a dud into a blast. Such sensitivity is not seen in one dimension and may explain the apparent heterogeneity in the outcomes of detailed simulations performed internationally. A natural conclusion is that the different groups collectively are closer to a realistic understanding of the mechanism of core-collapse supernovae than might have seemed apparent.

Authors:
 [1];  [1];  [2];  [3];  [4]
  1. Princeton Univ., NJ (United States). Dept. of Astrophysical Sciences
  2. Los Alamos National Lab. (LANL), Los Alamos, NM (United States)
  3. Lawrence Livermore National Lab. (LLNL), Livermore, CA (United States)
  4. Princeton Univ., NJ (United States). Schmidt Fellow and Inst. for Advanced Study
Publication Date:
Research Org.:
Los Alamos National Laboratory (LANL), Los Alamos, NM (United States); Lawrence Berkeley National Laboratory (LBNL), Berkeley, CA (United States); Lawrence Livermore National Laboratory (LLNL), Livermore, CA (United States); Lawrence Livermore National Laboratory (LLNL), Livermore, CA (United States) Center (NERSC).
Sponsoring Org.:
USDOE Office of Science (SC), Nuclear Physics (NP); National Science Foundation (NSF)
OSTI Identifier:
1460629
Alternate Identifier(s):
OSTI ID: 1461881
Report Number(s):
LA-UR-16-28849
Journal ID: ISSN 0038-6308
Grant/Contract Number:  
AC52-06NA25396; PHY-1144374; AST-1714267; AC03-76SF00098; ACI-1440032; OCI-0725070; ACI-1238993
Resource Type:
Accepted Manuscript
Journal Name:
Space Science Reviews
Additional Journal Information:
Journal Volume: 214; Journal Issue: 1; Journal ID: ISSN 0038-6308
Publisher:
Springer
Country of Publication:
United States
Language:
English
Subject:
79 ASTRONOMY AND ASTROPHYSICS; Supernova theory; Neutrino physics; Multi-dimensional radiation/hydrodynamics

Citation Formats

Burrows, A., Vartanyan, D., Dolence, J. C., Skinner, M. A., and Radice, D. Crucial Physical Dependencies of the Core-Collapse Supernova Mechanism. United States: N. p., 2018. Web. doi:10.1007/s11214-017-0450-9.
Burrows, A., Vartanyan, D., Dolence, J. C., Skinner, M. A., & Radice, D. Crucial Physical Dependencies of the Core-Collapse Supernova Mechanism. United States. https://doi.org/10.1007/s11214-017-0450-9
Burrows, A., Vartanyan, D., Dolence, J. C., Skinner, M. A., and Radice, D. Tue . "Crucial Physical Dependencies of the Core-Collapse Supernova Mechanism". United States. https://doi.org/10.1007/s11214-017-0450-9. https://www.osti.gov/servlets/purl/1460629.
@article{osti_1460629,
title = {Crucial Physical Dependencies of the Core-Collapse Supernova Mechanism},
author = {Burrows, A. and Vartanyan, D. and Dolence, J. C. and Skinner, M. A. and Radice, D.},
abstractNote = {We explore with self-consistent 2D FORNAX simulations the dependence of the outcome of collapse on many-body corrections to neutrino-nucleon cross sections, the nucleon-nucleon bremsstrahlung rate, electron capture on heavy nuclei, pre-collapse seed perturbations, and inelastic neutrino-electron and neutrino-nucleon scattering. Importantly, proximity to criticality amplifies the role of even small changes in the neutrino-matter couplings, and such changes can together add to produce outsized effects. When close to the critical condition the cumulative result of a few small effects (including seeds) that individually have only modest consequence can convert an anemic into a robust explosion, or even a dud into a blast. Such sensitivity is not seen in one dimension and may explain the apparent heterogeneity in the outcomes of detailed simulations performed internationally. A natural conclusion is that the different groups collectively are closer to a realistic understanding of the mechanism of core-collapse supernovae than might have seemed apparent.},
doi = {10.1007/s11214-017-0450-9},
journal = {Space Science Reviews},
number = 1,
volume = 214,
place = {United States},
year = {Tue Jan 23 00:00:00 EST 2018},
month = {Tue Jan 23 00:00:00 EST 2018}
}

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Simulations of Core-collapse Supernovae in Spatial Axisymmetry with Full Boltzmann Neutrino Transport
journal, February 2018

  • Nagakura, Hiroki; Iwakami, Wakana; Furusawa, Shun
  • The Astrophysical Journal, Vol. 854, Issue 2
  • DOI: 10.3847/1538-4357/aaac29

Measuring the Progenitor Masses and Dense Circumstellar Material of Type II Supernovae
journal, April 2018

  • Morozova, Viktoriya; Piro, Anthony L.; Valenti, Stefano
  • The Astrophysical Journal, Vol. 858, Issue 1
  • DOI: 10.3847/1538-4357/aab9a6

The Gravitational Wave Signal from Core-collapse Supernovae
journal, June 2018

  • Morozova, Viktoriya; Radice, David; Burrows, Adam
  • The Astrophysical Journal, Vol. 861, Issue 1
  • DOI: 10.3847/1538-4357/aac5f1

Progenitor Mass Distribution of Core-collapse Supernova Remnants in Our Galaxy and Magellanic Clouds Based on Elemental Abundances
journal, August 2018

  • Katsuda, Satoru; Takiwaki, Tomoya; Tominaga, Nozomu
  • The Astrophysical Journal, Vol. 863, Issue 2
  • DOI: 10.3847/1538-4357/aad2d8

PUSHing Core-collapse Supernovae to Explosions in Spherical Symmetry. II. Explodability and Remnant Properties
journal, December 2018

  • Ebinger, Kevin; Curtis, Sanjana; Fröhlich, Carla
  • The Astrophysical Journal, Vol. 870, Issue 1
  • DOI: 10.3847/1538-4357/aae7c9

PUSHing Core-collapse Supernovae to Explosions in Spherical Symmetry. III. Nucleosynthesis Yields
journal, December 2018

  • Curtis, Sanjana; Ebinger, Kevin; Fröhlich, Carla
  • The Astrophysical Journal, Vol. 870, Issue 1
  • DOI: 10.3847/1538-4357/aae7d2

An FFT-based Solution Method for the Poisson Equation on 3D Spherical Polar Grids
journal, January 2019


Effects of Rotation and Magnetic Field on the Revival of a Stalled Shock in Supernova Explosions
journal, February 2019

  • Fujisawa, Kotaro; Okawa, Hirotada; Yamamoto, Yu
  • The Astrophysical Journal, Vol. 872, Issue 2
  • DOI: 10.3847/1538-4357/aaffdd

On the Neutrino Distributions in Phase Space for the Rotating Core-collapse Supernova Simulated with a Boltzmann-neutrino-radiation-hydrodynamics Code
journal, February 2019

  • Harada, Akira; Nagakura, Hiroki; Iwakami, Wakana
  • The Astrophysical Journal, Vol. 872, Issue 2
  • DOI: 10.3847/1538-4357/ab0203

The ν -process with Fully Time-dependent Supernova Neutrino Emission Spectra
journal, May 2019

  • Sieverding, A.; Langanke, K.; Martínez-Pinedo, G.
  • The Astrophysical Journal, Vol. 876, Issue 2
  • DOI: 10.3847/1538-4357/ab17e2

One-, Two-, and Three-dimensional Simulations of Oxygen-shell Burning Just before the Core Collapse of Massive Stars
journal, August 2019

  • Yoshida, Takashi; Takiwaki, Tomoya; Kotake, Kei
  • The Astrophysical Journal, Vol. 881, Issue 1
  • DOI: 10.3847/1538-4357/ab2b9d

Chiral Effective Field Theory Description of Neutrino Nucleon–Nucleon Bremsstrahlung in Supernova Matter
journal, December 2019


Impact of the Rotation and Compactness of Progenitors on the Mass of Black Holes
journal, January 2020

  • Mapelli, Michela; Spera, Mario; Montanari, Enrico
  • The Astrophysical Journal, Vol. 888, Issue 2
  • DOI: 10.3847/1538-4357/ab584d

Comparing Treatments of Weak Reactions with Nuclei in Simulations of Core-collapse Supernovae
journal, February 2019

  • Nagakura, Hiroki; Furusawa, Shun; Togashi, Hajime
  • The Astrophysical Journal Supplement Series, Vol. 240, Issue 2
  • DOI: 10.3847/1538-4365/aafac9

Fornax: A Flexible Code for Multiphysics Astrophysical Simulations
journal, February 2019

  • Skinner, M. Aaron; Dolence, Joshua C.; Burrows, Adam
  • The Astrophysical Journal Supplement Series, Vol. 241, Issue 1
  • DOI: 10.3847/1538-4365/ab007f

Characterizing the Gravitational Wave Signal from Core-collapse Supernovae
journal, April 2019

  • Radice, David; Morozova, Viktoriya; Burrows, Adam
  • The Astrophysical Journal, Vol. 876, Issue 1
  • DOI: 10.3847/2041-8213/ab191a

Constraining Compact Object Formation with 2M0521
journal, June 2019

  • Breivik, Katelyn; Chatterjee, Sourav; Andrews, Jeff J.
  • The Astrophysical Journal, Vol. 878, Issue 1
  • DOI: 10.3847/2041-8213/ab21d3

Global comparison of core-collapse supernova simulations in spherical symmetry
text, January 2018


Simulations of core-collapse supernovae in spatial axisymmetry with full Boltzmann neutrino transport
text, January 2017


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


Core collapse with magnetic fields and rotation
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


Comparing treatments of weak reactions with nuclei in simulations of core-collapse supernovae
text, January 2018


Neutrino-driven Explosions
text, January 2017


Global comparison of core-collapse supernova simulations in spherical symmetry
text, January 2018