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Title: Electron-capture and Low-mass Iron-core-collapse Supernovae: New Neutrino-radiation-hydrodynamics Simulations

Abstract

We present new 1D (spherical) and 2D (axisymmetric) simulations of electron-capture (EC) and low-mass iron-core-collapse supernovae (SN). We consider six progenitor models: the ECSN progenitor from Nomoto; two ECSN-like low-mass low-metallicity iron-core progenitors from A. Heger (2016, private communication); and the 9, 10, and 11 $${M}_{\odot }$$ (zero-age main-sequence) progenitors from Sukhbold et al. We confirm that the ECSN and ESCN-like progenitors explode easily even in 1D with explosion energies of up to a 0.15 Bethes ($$1\ {\rm{B}}\equiv {10}^{51}\ \mathrm{erg}$$), and are a viable mechanism for the production of very-low-mass neutron stars. However, the 9, 10, and 11 $${M}_{\odot }$$ progenitors do not explode in 1D and are not even necessarily easier to explode than higher-mass progenitor stars in 2D. We study the effect of perturbations and of changes to the microphysics and we find that relatively small changes can result in qualitatively different outcomes, even in 1D, for models sufficiently close to the explosion threshold. Finally, we revisit the impact of convection below the protoneutron star (PNS) surface. We analyze 1D and 2D evolutions of PNSs subject to the same boundary conditions. Lastly, we find that the impact of PNS convection has been underestimated in previous studies and could result in an increase of the neutrino luminosity by up to factors of two.

Authors:
ORCiD logo [1]; ORCiD logo [2];  [2];  [3]; ORCiD logo [4]
  1. Institute for Advanced Study, Princeton, NJ (United States); Princeton Univ., Princeton, NJ (United States)
  2. Princeton Univ., Princeton, NJ (United States)
  3. Lawrence Livermore National Lab. (LLNL), Livermore, CA (United States)
  4. Los Alamos National Lab. (LANL), Los Alamos, NM (United States)
Publication Date:
Research Org.:
Los Alamos National Lab. (LANL), Los Alamos, NM (United States)
Sponsoring Org.:
USDOE Office of Science (SC)
OSTI Identifier:
1414138
Report Number(s):
LA-UR-17-20973
Journal ID: ISSN 1538-4357; TRN: US1800662
Grant/Contract Number:  
AC52-06NA25396
Resource Type:
Accepted Manuscript
Journal Name:
The Astrophysical Journal (Online)
Additional Journal Information:
Journal Name: The Astrophysical Journal (Online); Journal Volume: 850; Journal Issue: 1; Journal ID: ISSN 1538-4357
Publisher:
Institute of Physics (IOP)
Country of Publication:
United States
Language:
English
Subject:
79 ASTRONOMY AND ASTROPHYSICS; supernovae: general

Citation Formats

Radice, David, Burrows, Adam, Vartanyan, David, Skinner, Michael Aaron, and Dolence, Joshua C. Electron-capture and Low-mass Iron-core-collapse Supernovae: New Neutrino-radiation-hydrodynamics Simulations. United States: N. p., 2017. Web. doi:10.3847/1538-4357/aa92c5.
Radice, David, Burrows, Adam, Vartanyan, David, Skinner, Michael Aaron, & Dolence, Joshua C. Electron-capture and Low-mass Iron-core-collapse Supernovae: New Neutrino-radiation-hydrodynamics Simulations. United States. https://doi.org/10.3847/1538-4357/aa92c5
Radice, David, Burrows, Adam, Vartanyan, David, Skinner, Michael Aaron, and Dolence, Joshua C. Wed . "Electron-capture and Low-mass Iron-core-collapse Supernovae: New Neutrino-radiation-hydrodynamics Simulations". United States. https://doi.org/10.3847/1538-4357/aa92c5. https://www.osti.gov/servlets/purl/1414138.
@article{osti_1414138,
title = {Electron-capture and Low-mass Iron-core-collapse Supernovae: New Neutrino-radiation-hydrodynamics Simulations},
author = {Radice, David and Burrows, Adam and Vartanyan, David and Skinner, Michael Aaron and Dolence, Joshua C.},
abstractNote = {We present new 1D (spherical) and 2D (axisymmetric) simulations of electron-capture (EC) and low-mass iron-core-collapse supernovae (SN). We consider six progenitor models: the ECSN progenitor from Nomoto; two ECSN-like low-mass low-metallicity iron-core progenitors from A. Heger (2016, private communication); and the 9, 10, and 11 ${M}_{\odot }$ (zero-age main-sequence) progenitors from Sukhbold et al. We confirm that the ECSN and ESCN-like progenitors explode easily even in 1D with explosion energies of up to a 0.15 Bethes ($1\ {\rm{B}}\equiv {10}^{51}\ \mathrm{erg}$), and are a viable mechanism for the production of very-low-mass neutron stars. However, the 9, 10, and 11 ${M}_{\odot }$ progenitors do not explode in 1D and are not even necessarily easier to explode than higher-mass progenitor stars in 2D. We study the effect of perturbations and of changes to the microphysics and we find that relatively small changes can result in qualitatively different outcomes, even in 1D, for models sufficiently close to the explosion threshold. Finally, we revisit the impact of convection below the protoneutron star (PNS) surface. We analyze 1D and 2D evolutions of PNSs subject to the same boundary conditions. Lastly, we find that the impact of PNS convection has been underestimated in previous studies and could result in an increase of the neutrino luminosity by up to factors of two.},
doi = {10.3847/1538-4357/aa92c5},
journal = {The Astrophysical Journal (Online)},
number = 1,
volume = 850,
place = {United States},
year = {Wed Nov 15 00:00:00 EST 2017},
month = {Wed Nov 15 00:00:00 EST 2017}
}

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Criteria for Core-Collapse Supernova Explosions by the Neutrino Mechanism
text, January 2008


Charged current neutrino interactions in core-collapse supernovae in a virial expansion
text, January 2012


General-Relativistic Simulations of Three-Dimensional Core-Collapse Supernovae
text, January 2012


Core-Collapse Supernovae: Reflections and Directions
preprint, January 2012


SASI Activity in Three-Dimensional Neutrino-Hydrodynamics Simulations of Supernova Cores
text, January 2013


Type IIP supernova 2008in: the explosion of a normal red supergiant
text, January 2013


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text, January 2014


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text, January 2015


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Three-dimensional core-collapse supernova simulated using a 15 $M_\odot$ progenitor
text, January 2015


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text, January 2015


The Last Minutes of Oxygen Shell Burning in a Massive Star
text, January 2016


Neutrino-nucleon scattering in supernova matter from the virial expansion
text, January 2016


Stability of Standing Accretion Shocks, With an Eye Toward Core Collapse Supernovae
text, January 2002


Shock Breakout in Core-Collapse Supernovae and its Neutrino Signature
text, January 2002


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Works referencing / citing this record:

Final evolution of super-AGB stars and supernovae triggered by electron capture
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What can be learned from a future supernova neutrino detection?
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Turbulence in core-collapse supernovae
journal, April 2018

  • Radice, David; Abdikamalov, Ernazar; Ott, Christian D.
  • Journal of Physics G: Nuclear and Particle Physics, Vol. 45, Issue 5
  • DOI: 10.1088/1361-6471/aab872

Global comparison of core-collapse supernova simulations in spherical symmetry
journal, September 2018

  • O’Connor, Evan; Bollig, Robert; Burrows, Adam
  • Journal of Physics G: Nuclear and Particle Physics, Vol. 45, Issue 10
  • DOI: 10.1088/1361-6471/aadeae

The impact of different neutrino transport methods on multidimensional core-collapse supernova simulations
journal, November 2018

  • Pan, Kuo-Chuan; Mattes, Carlos; O’Connor, Evan P.
  • Journal of Physics G: Nuclear and Particle Physics, Vol. 46, Issue 1
  • DOI: 10.1088/1361-6471/aaed51

The impact of vorticity waves on the shock dynamics in core-collapse supernovae
journal, January 2018

  • Huete, César; Abdikamalov, Ernazar; Radice, David
  • Monthly Notices of the Royal Astronomical Society, Vol. 475, Issue 3
  • DOI: 10.1093/mnras/stx3360

A successful 3D core-collapse supernova explosion model
journal, September 2018

  • Vartanyan, David; Burrows, Adam; Radice, David
  • Monthly Notices of the Royal Astronomical Society, Vol. 482, Issue 1
  • DOI: 10.1093/mnras/sty2585

Revival of the fittest: exploding core-collapse supernovae from 12 to 25 M⊙
journal, March 2018

  • Vartanyan, David; Burrows, Adam; Radice, David
  • Monthly Notices of the Royal Astronomical Society, Vol. 477, Issue 3
  • DOI: 10.1093/mnras/sty809

Temporal and angular variations of 3D core-collapse supernova emissions and their physical correlations
journal, August 2019

  • Vartanyan, David; Burrows, Adam; Radice, David
  • Monthly Notices of the Royal Astronomical Society, Vol. 489, Issue 2
  • DOI: 10.1093/mnras/stz2307

The overarching framework of core-collapse supernova explosions as revealed by 3D fornax simulations
journal, November 2019

  • Burrows, Adam; Radice, David; Vartanyan, David
  • Monthly Notices of the Royal Astronomical Society, Vol. 491, Issue 2
  • DOI: 10.1093/mnras/stz3223

Three-dimensional supernova explosion simulations of 9-, 10-, 11-, 12-, and 13-M⊙ stars
journal, February 2019

  • Burrows, Adam; Radice, David; Vartanyan, David
  • Monthly Notices of the Royal Astronomical Society, Vol. 485, Issue 3
  • DOI: 10.1093/mnras/stz543

Two-dimensional Core-collapse Supernova Explosions Aided by General Relativity with Multidimensional Neutrino Transport
journal, February 2018


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 for Core-collapse Supernova Remnants in M31 and M33
journal, July 2018

  • Díaz-Rodríguez, Mariangelly; Murphy, Jeremiah W.; Rubin, David A.
  • The Astrophysical Journal, Vol. 861, Issue 2
  • DOI: 10.3847/1538-4357/aac6e1

Hydrodynamical Neutron-star Kicks in Electron-capture Supernovae and Implications for the CRAB Supernova
journal, September 2018


Exploring Fundamentally Three-dimensional Phenomena in High-fidelity Simulations of Core-collapse Supernovae
journal, September 2018


The Evolution toward Electron Capture Supernovae: The Flame Propagation and the Pre-bounce Electron–Neutrino Radiation
journal, January 2019

  • Takahashi, Koh; Sumiyoshi, Kohsuke; Yamada, Shoichi
  • The Astrophysical Journal, Vol. 871, Issue 2
  • DOI: 10.3847/1538-4357/aaf8a8

Three-dimensional Core-collapse Supernova Simulations with Multidimensional Neutrino Transport Compared to the Ray-by-ray-plus Approximation
journal, March 2019

  • Glas, Robert; Just, Oliver; Janka, H. -Thomas
  • The Astrophysical Journal, Vol. 873, Issue 1
  • DOI: 10.3847/1538-4357/ab0423

Evolution of ONeMg Core in Super-AGB Stars toward Electron-capture Supernovae: Effects of Updated Electron-capture Rate
journal, November 2019

  • Zha, Shuai; Leung, Shing-Chi; Suzuki, Toshio
  • The Astrophysical Journal, Vol. 886, Issue 1
  • DOI: 10.3847/1538-4357/ab4b4b

Matter Mixing in Aspherical Core-collapse Supernovae: Three-dimensional Simulations with Single-star and Binary Merger Progenitor Models for SN 1987A
journal, January 2020

  • Ono, Masaomi; Nagataki, Shigehiro; Ferrand, Gilles
  • The Astrophysical Journal, Vol. 888, Issue 2
  • DOI: 10.3847/1538-4357/ab5dba

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

GW170817: Joint Constraint on the Neutron Star Equation of State from Multimessenger Observations
journal, January 2018

  • Radice, David; Perego, Albino; Zappa, Francesco
  • The Astrophysical Journal, Vol. 852, Issue 2
  • DOI: 10.3847/2041-8213/aaa402

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

Turbulent mixing and transition criteria of flows induced by hydrodynamic instabilities
journal, August 2019

  • Zhou, Ye; Clark, Timothy T.; Clark, Daniel S.
  • Physics of Plasmas, Vol. 26, Issue 8
  • DOI: 10.1063/1.5088745

Neutrino signals of core-collapse supernovae in underground detectors
journal, August 2018

  • Seadrow, Shaquann; Burrows, Adam; Vartanyan, David
  • Monthly Notices of the Royal Astronomical Society, Vol. 480, Issue 4
  • DOI: 10.1093/mnras/sty2164

Core-collapse supernova simulations in one and two dimensions: comparison of codes and approximations
journal, September 2018

  • Just, O.; Bollig, R.; Janka, H-Th
  • Monthly Notices of the Royal Astronomical Society, Vol. 481, Issue 4
  • DOI: 10.1093/mnras/sty2578

The mechanism(s) of core-collapse supernovae
journal, September 2017

  • Couch, Sean M.
  • Philosophical Transactions of the Royal Society A: Mathematical, Physical and Engineering Sciences, Vol. 375, Issue 2105
  • DOI: 10.1098/rsta.2016.0271

Three-dimensional Boltzmann-hydro Code for Core-collapse in Massive Stars. III. A New Method for Momentum Feedback from Neutrino to Matter
journal, June 2019

  • Nagakura, Hiroki; Sumiyoshi, Kohsuke; Yamada, Shoichi
  • The Astrophysical Journal, Vol. 878, Issue 2
  • DOI: 10.3847/1538-4357/ab2189

The Progenitor Dependence of Core-collapse Supernovae from Three-dimensional Simulations with Progenitor Models of 12–40 M
journal, February 2018

  • Ott, Christian D.; Roberts, Luke F.; da Silva Schneider, André
  • The Astrophysical Journal, Vol. 855, Issue 1
  • DOI: 10.3847/2041-8213/aaa967

On the minimum mass of neutron stars
journal, September 2018

  • Suwa, Yudai; Yoshida, Takashi; Shibata, Masaru
  • Monthly Notices of the Royal Astronomical Society, Vol. 481, Issue 3
  • DOI: 10.1093/mnras/sty2460

Progenitor Mass Distribution for Core-Collapse Supernova Remnants in M31 and M33
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


Three-Dimensional Supernova Explosion Simulations of 9-, 10-, 11-, 12-, and 13-M$_{\odot}$ Stars
text, January 2019