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Title: The Explosion Mechanism of Core-Collapse Supernovae: Progress in Supernova Theory and Experiments

Abstract

The explosion of core-collapse supernova depends on a sequence of events taking place in less than a second in a region of a few hundred kilometers at the center of a supergiant star, after the stellar core approaches the Chandrasekhar mass and collapses into a proto-neutron star, and before a shock wave is launched across the stellar envelope. Theoretical efforts to understand stellar death focus on the mechanism which transforms the collapse into an explosion. Progress in understanding this mechanism is reviewed with particular attention to its asymmetric character. We highlight a series of successful studies connecting observations of supernova remnants and pulsars properties to the theory of core-collapse using numerical simulations. The encouraging results from first principles models in axisymmetric simulations is tempered by new puzzles in 3D. The diversity of explosion paths and the dependence on the pre-collapse stellar structure is stressed, as well as the need to gain a better understanding of hydrodynamical and MHD instabilities such as SASI and neutrino-driven convection. The shallow water analogy of shock dynamics is presented as a comparative system where buoyancy effects are absent. This dynamical system can be studied numerically and also experimentally with a water fountain. Lastly, we analysemore » the potential of this complementary research tool for supernova theory. We also review its potential for public outreach in science museums.« less

Authors:
 [1];  [1];  [2];  [3];  [1];  [1];  [4];  [4];  [5];  [1];  [6];  [7];  [8];  [1]
+ Show Author Affiliations
  1. Univ. Paris Diderot, Gif sur Yvette, Cedex (France)
  2. Max Planck Inst. for Astrophysics, Garching (Germany)
  3. National Autonomous Univ. of Mexico, Morelos (Mexico)
  4. CNRS/Observatoire de Paris. Univ. Paris (France). Laboratory Universe and Theories (LUTh)
  5. Univ. Claude Bernard Lyon, Villeurbanne (France). Inst. de Physique Nucleaire de Lyon
  6. Inst. de Physique Nucleaire (IPN), Orsay (France)
  7. Alternative Energies and Atomic Energy Commission (CEA), Arpajon (France)
  8. Univ. de Valencia, Valencia (Spain)
Publication Date:
Research Org.:
Los Alamos National Laboratory (LANL), Los Alamos, NM (United States)
Sponsoring Org.:
USDOE
OSTI Identifier:
1248610
Report Number(s):
LA-UR-14-29636
Journal ID: ISSN 1323-3580
Grant/Contract Number:  
AC52-06NA25396
Resource Type:
Accepted Manuscript
Journal Name:
Publications of the Astronomical Society of Australia
Additional Journal Information:
Journal Volume: 32; Journal ID: ISSN 1323-3580
Country of Publication:
United States
Language:
English
Subject:
79 ASTRONOMY AND ASTROPHYSICS; Astronomy and Astrophysics

Citation Formats

Foglizzo, Thierry, Kazeroni, Rémi, Guilet, Jérôme, Masset, Frédéric, González, Matthias, Krueger, Brendan K., Novak, Jérôme, Oertel, Micaela, Margueron, Jérôme, Faure, Julien, Martin, Noël, Blottiau, Patrick, Peres, Bruno, and Durand, Gilles. The Explosion Mechanism of Core-Collapse Supernovae: Progress in Supernova Theory and Experiments. United States: N. p., 2015. Web. doi:10.1017/pasa.2015.9.
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Foglizzo, Thierry, Kazeroni, Rémi, Guilet, Jérôme, Masset, Frédéric, González, Matthias, Krueger, Brendan K., Novak, Jérôme, Oertel, Micaela, Margueron, Jérôme, Faure, Julien, Martin, Noël, Blottiau, Patrick, Peres, Bruno, & Durand, Gilles. The Explosion Mechanism of Core-Collapse Supernovae: Progress in Supernova Theory and Experiments. United States. https://doi.org/10.1017/pasa.2015.9
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Foglizzo, Thierry, Kazeroni, Rémi, Guilet, Jérôme, Masset, Frédéric, González, Matthias, Krueger, Brendan K., Novak, Jérôme, Oertel, Micaela, Margueron, Jérôme, Faure, Julien, Martin, Noël, Blottiau, Patrick, Peres, Bruno, and Durand, Gilles. Thu . "The Explosion Mechanism of Core-Collapse Supernovae: Progress in Supernova Theory and Experiments". United States. https://doi.org/10.1017/pasa.2015.9. https://www.osti.gov/servlets/purl/1248610.
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@article{osti_1248610,
title = {The Explosion Mechanism of Core-Collapse Supernovae: Progress in Supernova Theory and Experiments},
author = {Foglizzo, Thierry and Kazeroni, Rémi and Guilet, Jérôme and Masset, Frédéric and González, Matthias and Krueger, Brendan K. and Novak, Jérôme and Oertel, Micaela and Margueron, Jérôme and Faure, Julien and Martin, Noël and Blottiau, Patrick and Peres, Bruno and Durand, Gilles},
abstractNote = {The explosion of core-collapse supernova depends on a sequence of events taking place in less than a second in a region of a few hundred kilometers at the center of a supergiant star, after the stellar core approaches the Chandrasekhar mass and collapses into a proto-neutron star, and before a shock wave is launched across the stellar envelope. Theoretical efforts to understand stellar death focus on the mechanism which transforms the collapse into an explosion. Progress in understanding this mechanism is reviewed with particular attention to its asymmetric character. We highlight a series of successful studies connecting observations of supernova remnants and pulsars properties to the theory of core-collapse using numerical simulations. The encouraging results from first principles models in axisymmetric simulations is tempered by new puzzles in 3D. The diversity of explosion paths and the dependence on the pre-collapse stellar structure is stressed, as well as the need to gain a better understanding of hydrodynamical and MHD instabilities such as SASI and neutrino-driven convection. The shallow water analogy of shock dynamics is presented as a comparative system where buoyancy effects are absent. This dynamical system can be studied numerically and also experimentally with a water fountain. Lastly, we analyse the potential of this complementary research tool for supernova theory. We also review its potential for public outreach in science museums.},
doi = {10.1017/pasa.2015.9},
journal = {Publications of the Astronomical Society of Australia},
number = ,
volume = 32,
place = {United States},
year = {Thu Jan 01 00:00:00 EST 2015},
month = {Thu Jan 01 00:00:00 EST 2015}
}
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Pulsar Spin-Velocity Alignment: Kinematic Ages, Birth Periods and Braking Indices
text, January 2013

A Massive Pulsar in a Compact Relativistic Binary
text, January 2013

Parametric Study of Flow Patterns behind the Standing Accretion Shock Wave for Core-Collapse Supernovae
text, January 2013

Magnetorotational Core-Collapse Supernovae in Three Dimensions
text, January 2014

Asymmetries in core-collapse supernovae from maps of radioactive $^{44}$Ti in CassiopeiaA
text, January 2014

The Role of Turbulence in Neutrino-Driven Core-Collapse Supernova Explosions
text, January 2014

Neutrino viscosity and drag: impact on the magnetorotational instability in protoneutron stars
text, January 2014

The Magnetorotational Instability in Core Collapse Supernova Explosions
text, January 2002

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

Fitting Pulsar Wind Tori
text, January 2003

A statistical study of 233 pulsar proper motions
text, January 2005

A non-spherical core in the explosion of supernova SN 2004dj
text, January 2006

The Effect of Neutrino Radiation on Magnetorotational Instability in Proto-Neutron Stars
text, January 2006

56Ni dredge-up in Supernova 1987A
text, January 1998

Production of exotic hypernuclei and hyper-matter
preprint, January 2013

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    Structure of the hydraulic jump in convergent radial flows
    journal, December 2018

    Core-collapse supernovae in the hall of mirrors: A three-dimensional code-comparison project
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    Ultra-stripped supernovae: progenitors and fate
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    • Tauris, Thomas M.; Langer, Norbert; Podsiadlowski, Philipp
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    • DOI: 10.1093/mnras/stv990

    Shock–turbulence interaction in core-collapse supernovae
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    • Abdikamalov, Ernazar; Zhaksylykov, Azamat; Radice, David
    • Monthly Notices of the Royal Astronomical Society, Vol. 461, Issue 4
    • DOI: 10.1093/mnras/stw1604

    Diffuse supernova neutrino background from extensive core-collapse simulations of 8–100 M⊙ progenitors
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    • Horiuchi, Shunsaku; Sumiyoshi, Kohsuke; Nakamura, Ko
    • Monthly Notices of the Royal Astronomical Society, Vol. 475, Issue 1
    • DOI: 10.1093/mnras/stx3271

    The impact of vorticity waves on the shock dynamics in core-collapse supernovae
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    • Huete, César; Abdikamalov, Ernazar; Radice, David
    • Monthly Notices of the Royal Astronomical Society, Vol. 475, Issue 3
    • DOI: 10.1093/mnras/stx3360

    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

    Merging black hole binaries with the SEVN code
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    • Spera, Mario; Mapelli, Michela; Giacobbo, Nicola
    • Monthly Notices of the Royal Astronomical Society, Vol. 485, Issue 1
    • DOI: 10.1093/mnras/stz359

    Charged-current scattering off the 16O nucleus as a detection channel for supernova neutrinos
    journal, December 2018

    • Nakazato, Ken’ichiro; Suzuki, Toshio; Sakuda, Makoto
    • Progress of Theoretical and Experimental Physics, Vol. 2018, Issue 12
    • DOI: 10.1093/ptep/pty134

    A new Multi-Energy Neutrino Radiation-Hydrodynamics code in full General Relativity and its Application to the Gravitational Collapse of Massive Stars
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    • Kuroda, Takami; Takiwaki, Tomoya; Kotake, Kei
    • The Astrophysical Journal Supplement Series, Vol. 222, Issue 2
    • DOI: 10.3847/0067-0049/222/2/20

    Formation of Double Neutron Star Systems
    journal, September 2017

    • Tauris, T. M.; Kramer, M.; Freire, P. C. C.
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    • DOI: 10.3847/1538-4357/aa7e89

    Impact of Neutrino Opacities on Core-collapse Supernova Simulations
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    • Kotake, Kei; Takiwaki, Tomoya; Fischer, Tobias
    • The Astrophysical Journal, Vol. 853, Issue 2
    • DOI: 10.3847/1538-4357/aaa716

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

    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

    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

    Cooling Timescale for Protoneutron Stars and Properties of Nuclear Matter: Effective Mass and Symmetry Energy at High Densities
    journal, June 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

    Possible Early Linear Acceleration of Proto-neutron Stars via Asymmetric Neutrino Emission in Core-collapse Supernovae
    journal, July 2019

    • Nagakura, Hiroki; Sumiyoshi, Kohsuke; Yamada, Shoichi
    • The Astrophysical Journal, Vol. 880, Issue 2
    • DOI: 10.3847/2041-8213/ab30ca

    Multimessenger signals of long-term core-collapse supernova simulations: synergetic observation strategies
    journal, June 2016

    • Nakamura, Ko; Horiuchi, Shunsaku; Tanaka, Masaomi
    • Monthly Notices of the Royal Astronomical Society, Vol. 461, Issue 3
    • DOI: 10.1093/mnras/stw1453

    A critical assessment of turbulence models for 1D core-collapse supernova simulations
    journal, June 2019

    • Müller, Bernhard
    • Monthly Notices of the Royal Astronomical Society, Vol. 487, Issue 4
    • DOI: 10.1093/mnras/stz1594

    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 simulations of rapidly rotating core-collapse supernovae: finding a neutrino-powered explosion aided by non-axisymmetric flows
    journal, May 2016

    • Takiwaki, Tomoya; Kotake, Kei; Suwa, Yudai
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    • DOI: 10.1093/mnrasl/slw105

    Systematic features of axisymmetric neutrino-driven core-collapse supernova models in multiple progenitors
    journal, October 2015

    • Nakamura, Ko; Takiwaki, Tomoya; Kuroda, Takami
    • Publications of the Astronomical Society of Japan, Vol. 67, Issue 6
    • DOI: 10.1093/pasj/psv073

    One-, Two-, and Three-dimensional Simulations of Oxygen-shell Burning Just before the Core Collapse of Massive Stars
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    • The Astrophysical Journal, Vol. 881, Issue 1
    • DOI: 10.3847/1538-4357/ab2b9d

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

    Gravitational wave asteroseismology with protoneutron stars
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    Impact of Neutrino Opacities on Core-Collapse Supernova Simulations
    text, January 2018

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

    Neutrino-driven Explosions
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    Supernovae from massive stars
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    Turbulence Generation by Shock-Acoustic-Wave Interaction in Core-Collapse Supernovae
    preprint, January 2018

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