Supernova Simulations from a 3D Progenitor Model -- Impact of Perturbations and Evolution of Explosion Properties

Abstract

We study the impact of large-scale perturbations from convective shell burning on the core-collapse supernova explosion mechanism using three-dimensional (3D) multi-group neutrino hydrodynamics simulations of an 18 solar mass progenitor. Seed asphericities in the O shell, obtained from a recent 3D model of O shell burning, help trigger a neutrino-driven explosion 330ms after bounce whereas the shock is not revived in a model based on a spherically symmetric progenitor for at least another 300ms. We tentatively infer a reduction of the critical luminosity for shock revival by ~20% due to pre-collapse perturbations. This indicates that convective seed perturbations play an important role in the explosion mechanism in some progenitors. We follow the evolution of the 18 solar mass model into the explosion phase for more than 2s and find that the cycle of accretion and mass ejection is still ongoing at this stage. With a preliminary value of 0.77 Bethe for the diagnostic explosion energy, a baryonic neutron star mass of 1.85 solar masses, a neutron star kick of ~600km/s and a neutron star spin period of ~20ms at the end of the simulation, the explosion and remnant properties are slightly atypical, but still lie comfortably within the observed distribution. Although more refined simulations and a larger survey of progenitors are still called for, this suggests that a solution to the problem of shock revival and explosion energies in the ballpark of observations are within reach for neutrino-driven explosions in 3D.

23 pages, 22 figures, accepted for publication in MNRAS

References in corpus (22)

• Delayed neutrino-driven supernova explosions aided by the standing accretion-shock instability
• Three-dimensional core-collapse supernova simulated using a 15 $M_{\odot }$ progenitor
• Instability of a stalled accretion shock: evidence for the advective-acoustic cycle
• The Role of Turbulence in Neutrino-Driven Core-Collapse Supernova Explosions
• The Status of Multi-Dimensional Core-Collapse Supernova Models
• Neutrino-driven supernova of a low-mass iron-core progenitor boosted by three-dimensional turbulent convection
• Criteria for Core-Collapse Supernova Explosions by the Neutrino Mechanism
• Multidimensional supernova simulations with approximative neutrino transport. II. Convection and the advective-acoustic cycle in the supernova core
• Nucleosynthesis in the Innermost Ejecta of Neutrino-Drive Supernova Explosions in Two Dimensions
• Getting Its Kicks: A VLBA Parallax for the Hyperfast Pulsar B1508+55
• Neutron star kicks by the gravitational tug-boat mechanism in asymmetric supernova explosions: progenitor and explosion dependence
• The Dynamics of Neutrino-Driven Supernova Explosions after Shock Revival in 2D and 3D
• Improved constrained scheme for the Einstein equations: An approach to the uniqueness issue
• Dynamics of shock propagation and nucleosynthesis conditions in O-Ne-Mg core supernovae
• Hydrodynamical Neutron Star Kicks in Three Dimensions
• Neutrino-nucleon scattering in supernova matter from the virial expansion
• A Global Model of The Light Curves and Expansion Velocities of Type II-Plateau Supernovae
• How rapidly do neutron stars spin at birth? Constraints from archival X-ray observations of extragalactic supernovae
• Spin-Kick Correlation in Neutron Stars: Alignment Conditions and Implications
• Linear analysis on the growth of non-spherical perturbations in supersonic accretion flows
• Toward an Empirical Theory of Pulsar Emission XI. Understanding the Orientations of Pulsar Radiation and Supernova "Kicks"
• Does energy of type IIP supernovae depends on stellar mass?

Cited by in corpus (174)

• Science Case for the Einstein Telescope
• Core-Collapse Supernova Explosion Theory
• On the formation history of Galactic double neutron stars
• The Overarching Framework of Core-Collapse Supernova Explosions as Revealed by 3D Fornax Simulations
• Exploring Fundamentally Three-dimensional Phenomena in High-fidelity Simulations of Core-collapse Supernovae
• Three-Dimensional Simulations of Neutrino-Driven Core-Collapse Supernovae from Low-Mass Single and Binary Star Progenitors
• Characterizing the Gravitational Wave Signal from Core-Collapse Supernovae
• Hydrodynamics of core-collapse supernovae and their progenitors
• The Explosion of Helium Stars Evolved With Mass Loss
• Muon Creation in Supernova Matter Facilitates Neutrino-driven Explosions
• Self-consistent 3D Supernova Models From -7 Minutes to +7 Seconds: a 1-bethe Explosion of a ~19 Solar-mass Progenitor
• A Successful 3D Core-Collapse Supernova Explosion Model
• The gravitational wave signal from core-collapse supernovae
• Nucleosynthesis in the Innermost Ejecta of Neutrino-Drive Supernova Explosions in Two Dimensions
• Dipole portal to heavy neutral leptons
• Three-Dimensional Supernova Explosion Simulations of 9-, 10-, 11-, 12-, and 13-M${}_{\odot }$ Stars
• Rotation-supported Neutrino-driven Supernova Explosions in Three Dimensions and the Critical Luminosity Condition
• Three-dimensional Models of Core-collapse Supernovae From Low-mass Progenitors With Implications for Crab
• The Progenitor Dependence of Three-Dimensional Core-Collapse Supernovae
• Gravitational Wave Emission from 3D Explosion Models of Core-Collapse Supernovae with Low and Normal Explosion Energies
• Three-dimensional core-collapse supernova simulations of massive and rotating progenitors
• Black hole formation and fallback during the supernova explosion of a $40{\mathrm{M}}_{\odot }$ star
• Gravitational waves from three-dimensional core-collapse supernova models: The impact of moderate progenitor rotation
• Magnetorotational Explosion of A Massive Star Supported by Neutrino Heating in General Relativistic Three Dimensional Simulations
• Temporal and Angular Variations of 3D Core-Collapse Supernova Emissions and their Physical Correlations
• Simulating Turbulence-aided Neutrino-driven Core-collapse Supernova Explosions in One Dimension
• Simulations of core-collapse supernovae in spatial axisymmetry with full Boltzmann neutrino transport
• Gravitational-wave signal of a core-collapse supernova explosion of a 15 Solar mass star
• Hydrodynamical Neutron-star Kicks in Electron-capture Supernovae and Implications for the CRAB Supernova
• Fast-pairwise collective neutrino oscillations associated with asymmetric neutrino emissions in core-collapse supernova
• Anisotropic emission of neutrino and gravitational-wave signals from rapidly rotating core-collapse supernovae
• Revival of the Fittest: Exploding Core-Collapse Supernovae from 12 to 25 M${}_{\odot }$
• Three-Dimensional Core-Collapse Supernova Simulations with Multi-Dimensional Neutrino Transport Compared to the Ray-by-Ray-plus Approximation
• Be X-ray binaries in the SMC as indicators of mass transfer efficiency
• One-, Two-, and Three-dimensional Simulations of Oxygen Shell Burning Just Before the Core-Collapse of Massive Stars
• Fast Neutrino Flavor Conversions can Help and Hinder Neutrino-Driven Explosions
• Heavy axion-like particles and core-collapse supernovae: constraints and impact on the explosion mechanism
• Equation of state effects in the core collapse of a $20$-$M_{\odot }$ star
• Core-collapse supernova simulations in one and two dimensions: comparison of codes and approximations
• Supernova Fallback as Origin of Neutron Star Spins and Spin-kick Alignment
• The impact of fallback on the compact remnants and chemical yields of core-collapse supernovae
• Multi-D Simulations of Ultra-Stripped Supernovae to Shock Breakout
• Large-Scale Mixing in a Violent Oxygen-Neon Shell Merger Prior to a Core-Collapse Supernova
• Particle-in-cell Simulation of the Neutrino Fast Flavor Instability
• Intermediate-Mass-Elements in Young Supernova Remnants Reveal Neutron Star Kicks by Asymmetric Explosions
• Impact of Neutrino Opacities on Core-Collapse Supernova Simulations
• Stellar Collapse Diversity and the Diffuse Supernova Neutrino Background
• Neutrino Emission as Diagnostics of Core-Collapse Supernovae
• Neutrino emission characteristics of black hole formation in three-dimensional simulations of stellar collapse
• The Collapse and Three-Dimensional Explosion of Three-Dimensional, vis à vis One-Dimensional, Massive-star Supernova Progenitor Models
• Supernova Simulations Confront SN 1987A Neutrinos
• Core Collapse Supernova Gravitational Wave Emission for Progenitors of 9.6, 15, and 25 Solar Masses
• Gravitational Waves from Neutrino Asymmetries in Core-Collapse Supernovae
• Turbulence in Core-Collapse Supernovae
• 3D hydrodynamic simulations of C ingestion into a convective O shell
• Towards an Understanding of the Resolution Dependence of Core-Collapse Supernova Simulations
• Matter Mixing in Aspherical Core-collapse Supernovae: Three-dimensional Simulations with Single Star and Binary Merger Progenitor Models for SN 1987A
• The presupernova core mass-radius relation of massive stars: understanding its formation and evolution
• The Essential Character of the Neutrino Mechanism of Core-Collapse Supernova Explosions
• How Turbulence Enables Core-Collapse Supernova Explosions
• The difficulty of inferring progenitor masses from Type II-Plateau supernova light curves
• Pulsational pair-instability supernovae: gravitational collapse, black-hole formation, and beyond
• Angular momentum transport in massive stars and natal neutron star rotation rates
• Simulations of light curves and spectra for superluminous Type Ic supernovae powered by magnetars
• Long-term Simulations of Multi-Dimensional Core-collapse Supernovae: Implications for Neutron Star Kicks
• The infancy of core-collapse supernova remnants
• Convective H-He Interactions in Massive Population III Stellar Evolution Models
• Kicks and Induced Spins of Neutron Stars at Birth
• Supernova neutrino signals based on long-term axisymmetric simulations
• Core collapse with magnetic fields and rotation
• Radiative-transfer modeling of nebular-phase type II supernovae. Dependencies on progenitor and explosion properties
• Properties of Convective Oxygen and Silicon Burning Shells in Supernova Progenitors
• Core-collapse supernovae in the hall of mirrors. A three-dimensional code-comparison project
• Three-Dimensional Hydrodynamic Simulations of Convective Nuclear Burning In Massive Stars Near Iron Core Collapse
• Interplay Between Neutrino Kicks and Hydrodynamic Kicks of Neutron Stars and Black Holes
• The chemical signature of jet-driven hypernovae
• Simulations of the Early Post-Bounce Phase of Core-Collapse Supernovae in Three-Dimensional Space with Full Boltzmann Neutrino Transport
• The impact of the new measurement of the ${}^{12}\mathrm{C}{+}^{12}\mathrm{C}$ fusion cross section on the final compactness of the massive stars
• The role of radioactive nickel in shaping the plateau phase of Type II supernovae
• Signatures of R-process Enrichment in Supernovae from Collapsars
• The Impact of Different Neutrino Transport Methods on Multidimensional Core-collapse Supernova Simulations
• Resolution Study for Three-dimensional Supernova Simulations with the Prometheus-Vertex Code
• ${}^{44}\mathrm{Ti}$ ejecta in young supernova remnants
• Three-Dimensional Boltzmann-Hydro Code for core-collapse in massive stars III. A New method for momentum feedback from neutrino to matter
• On The Development of Multidimensional Progenitor Models For Core-collapse Supernovae
• Effects of the standing accretion-shock instability and the lepton-emission self-sustained asymmetry in the neutrino emission of rotating supernovae
• Low-luminosity type IIP supernovae: SN 2005cs and SN 2020cxd as very low-energy iron core-collapse explosions
• 3D Simulations of Strongly Magnetised Non-Rotating Supernovae: Explosion Dynamics and Remnant Properties
• 3D Simulations of Oxygen Shell Burning with and without Magnetic Fields
• Gravitational-wave Signals From Three-dimensional Supernova Simulations With Different Neutrino-Transport Methods
• Supplying angular momentum to the jittering jets explosion mechanism using inner convection layers
• Identifying rotation in SASI-dominated core-collapse supernovae with a neutrino gyroscope
• A three-dimensional hydrodynamics simulation of oxygen-shell burning in the final evolution of a fast-rotating massive star
• Three-dimensional GRMHD Simulations of Rapidly Rotating Stellar Core-Collapse
• Three-dimensional Hydrodynamics Simulations of Precollapse Shell Burning in the Si- and O-rich Layers
• A Critical Assessment of Turbulence Models for 1D Core-Collapse Supernova Simulations
• Modeling the γ-ray Pulsar Wind Nebulae population in our Galaxy
• Reviving the stalled shock by jittering jets in core collapse supernovae: jets from the standing accretion shock instability
• Impact of magnetic field on neutrino-matter interactions in core-collapse supernova
• A 3D Simulation of a Type II-P Supernova: from Core Bounce to Beyond Shock Breakout
• Hydrodynamic Simulations of Electron-capture Supernovae: Progenitor and Dimension Dependence
• A Comparison of Explosion Energies for Simulated and Observed Core-Collapse Supernovae
• The Status and Future of Direct Nuclear Reaction Measurements for Stellar Burning
• The Morphologies and Kinematics of Supernova Remnants
• Neutron star natal kick and jets in core collapse supernovae
• The impact of vorticity waves on the shock dynamics in core-collapse supernovae
• Explodability criteria for the neutrino-driven supernova mechanism
• Measuring the neutron star compactness and binding energy with supernova neutrinos
• On Stellar Evolution In A Neutrino Hertzsprung-Russell Diagram
• 3D stellar evolution: hydrodynamic simulations of a complete burning phase in a massive star
• Monotonicity of the cores of massive stars
• Efficient estimation method for time evolution of proto-neutron star mass and radius from supernova neutrino signal
• Remnant masses of core collapse supernovae in the jittering jets explosion mechanism
• Post-explosion evolution of core-collapse supernovae
• Toward Realistic Models of Core Collapse Supernovae: A Brief Review
• Effects of rotation and magnetic field on the revival of a stalled shock in supernova explosions
• Wave heating from proto-neutron star convection and the core-collapse supernova explosion mechanism
• Neutrino flavor mixing with moments
• Shock Revival in Core-collapse Supernovae Assisted by Heavy Axion-like Particles
• Core-collapse supernova simulations with reduced nucleosynthesis networks
• Multimessenger Emission from the Accretion Induced Collapse of White Dwarfs
• Asymmetries of Heavy Elements in the Young Supernova Remnant Cassiopeia A
• The impact of progenitor asymmetries on the neutrino-driven convection in core-collapse supernovae
• Effect of stellar rotation on the development of post-shock instabilities during core-collapse supernovae
• Amplifying magnetic fields of a newly born neutron star by stochastic angular momentum accretion in core collapse supernovae
• Neutrino transport with Monte Carlo method: I. Towards fully consistent implementation of nucleon recoils in core-collapse supernova simulations
• Comparison of the Core-Collapse Evolution of Two Nearly Equal Mass Progenitors
• Supernova bounds on new scalars from resonant and soft emission
• Impact of medium modification of the nucleon weak and electromagnetic form factors on the neutrino mean free path in dense matter
• X-ray Absorption in Young Core-Collapse Supernova Remnants
• SN 2023ixf -- an average-energy explosion with circumstellar medium and a precursor
• Jet-shaped geometrically modified light curves of core collapse supernovae
• Rotation and Magnetism of Massive Stellar Cores
• The non-linear onset of neutrino-driven convection in two and three-dimensional core-collapse supernovae
• Vortical amplification of magnetic field at inward shock of supernova remnant Cassiopeia A
• Acoustic wave generation in collapsing massive stars with convective shells
• On the importance of progenitor asymmetry to shock revival in core-collapse supernovae
• A Force Explosion Condition for Spherically Symmetric Core-collapse Supernovae
• A Generalized Kompaneets Formalism for Inelastic Neutrino-Nucleon Scattering in Supernova Simulations
• Parameterisations of thermal bomb explosions for core-collapse supernovae and 56Ni production
• Black Hole Supernovae, their Equation of State Dependence and Ejecta Composition
• Stellar Neutrino Emission Across The Mass-Metallicity Plane
• Fallback onto Kicked Neutron Stars and its Effect on Spin-Kick Alignment
• A well-balanced scheme for the simulation tool-kit A-MaZe: implementation, tests, and first applications to stellar structure
• Neutrino-driven Core-collapse Supernova Yields in Galactic Chemical Evolution
• The Yet-Unobserved Multi-Messenger Gravitational-Wave Universe
• Impact of rotation on the evolution of convective vortices in collapsing stars
• Turbulent dynamo action and its effects on the mixing at the convective boundary of an idealized oxygen-burning shell
• Active Learning for Computationally Efficient Distribution of Binary Evolution Simulations
• Light Curves of Type IIP Supernovae from Neutrino-driven Explosions of Red Supergiants Obtained by a Semi-analytic Approach
• The Force Explosion Condition is Consistent with Spherically Symmetric CCSN Explosions
• Near-critical supernova outflows and their neutrino signatures
• Enhanced mass-loss rate evolution of stars with $\gtrsim 18M_{\odot }$ and missing optically-observed type II core-collapse supernovae
• Supernovae from stellar mergers and accretors of binary mass transfer: Implications for Type IIP, 1987A-like and interacting supernovae
• Natal kicks of compact objects
• Explosion Energies for Core-collapse Supernovae I: Analytic, Spherically Symmetric Solutions
• Response of nuclear-dissociating shocks to vorticity perturbations
• Parallelized Solution Method of the Three-dimensional Gravitational Potential on the Yin-Yang Grid
• Transition Elements in Supernova Presolar Grains: Condensation vs. Implantation
• Chlorine and Potassium Enrichment in the Cassiopeia A Supernova Remnant
• Constraints on Explosion Timescale of Core-Collapse Supernovae Based on Systematic Analysis of Light Curves
• A Parametric Study of the SASI Comparing General Relativistic and Nonrelativistic Treatments
• Dynamical ejecta of neutron star mergers with nucleonic weak processes I: Nucleosynthesis
• FRIB and the GW170817 Kilonova
• Turbulence Generation by Shock-Acoustic-Wave Interaction in Core-Collapse Supernovae
• Asymmetric emissions of neutrinos in the cooling of rotating proto-neutron stars
• The influence of rotation and metallicity on the explodability of massive stars
• 3D Synthetic Convective Velocity Fields to Initialise Core-Collapse Supernova Simulations from 1D Progenitors
• A Brief History of the Co-evolution of Supernova Theory with Neutrino Physics
• Linear Analysis of the Shock Instability in Core-collapse Supernovae: Influences of Acoustic Power and Fluctuations of Neutrino Luminosity
• Comprehensive neutrino light curves and spectra: from pre-supernova evolution to early supernova phase
• Assessing the Distance for Probing the Nuclear Equation of State with Supernova Gravitational Waves
• Constraining the Time of Gravitational Wave Emission from Core-Collapse Supernovae
• Stochastic Gravitational-Wave Background from Stellar Core-Collapse Events