Long-term Simulations of Multi-Dimensional Core-collapse Supernovae: Implications for Neutron Star Kicks

Abstract

Core-collapse supernovae (CCSNe) are the final stage of massive stars, marking the birth of neutron stars (NSs). The aspherical mass ejection drives a natal kick of the forming NS. In this work we study the properties of the NS kick based on our long-term hydrodynamics CCSN simulations. We perform two-dimensional (2D) simulations for ten progenitors from a 10.8 to 20 $M_{\odot }$ star covering a wide range of the progenitor's compactness parameter, and two three-dimensional (3D) simulations for an 11.2 $M_{\odot }$ star. Our 2D models present a variety of explosion energies between $\sim 1.3\times 10^{50}$ erg and $\sim 1.2\times 10^{51}$ erg, and NS kick velocities between $\sim 100$ km s${}^{-1}$ and $\sim 1500$ km s${}^{-1}$. For the 2D exploding models, we find that the kick velocities tend to become higher with the progenitor's compactness. This is because the high progenitor compactness results in high neutrino luminosity from the proto-neutron star (PNS), leading to more energetic explosions. Since high-compactness progenitors produce massive PNSs, we point out that the NS masses and the kick velocities can be correlated, which is moderately supported by observation. Comparing 2D and 3D models of the 11.2 $M_{\odot }$ star, the diagnostic explosion energy in 3D is, as previously identified, higher than that in 2D, whereas the 3D model results in a smaller asymmetry in the ejecta distribution and a smaller kick velocity than in 2D. Our results confirm the importance of self-consistent CCSN modeling covering a long-term postbounce evolution in 3D for a quantitative prediction of the NS kicks.

arXiv comment13 pages, 10 figures, accepted for publication in PASJ

References in corpus (87)

• A statistical study of 233 pulsar proper motions
• Core-Collapse Supernovae from 9 to 120 Solar Masses Based on Neutrino-powered Explosions
• Black Hole Formation in Failing Core-Collapse Supernovae
• Stability of Standing Accretion Shocks, With an Eye Toward Core Collapse Supernovae
• The Velocity Distribution of Isolated Radio Pulsars
• Progenitor-Explosion Connection and Remnant Birth Masses for Neutrino-Driven Supernovae of Iron-Core Progenitors
• High-precision timing of 42 millisecond pulsars with the European Pulsar Timing Array
• Physics of Core-Collapse Supernovae in Three Dimensions: a Sneak Preview
• Delayed neutrino-driven supernova explosions aided by the standing accretion-shock instability
• A two-parameter criterion for classifying the explodability of massive stars by the neutrino-driven mechanism
• Multidimensional Supernova Simulations with Approximative Neutrino Transport I. Neutron Star Kicks and the Anisotropy of Neutrino-Driven Explosions in Two Spatial Dimensions
• Pulsar Recoil and Gravitational Radiation due to Asymmetrical Stellar Collapse and Explosion
• Three-dimensional neutrino-driven supernovae: Neutron star kicks, spins, and asymmetric ejection of nucleosynthesis products
• Three-dimensional core-collapse supernova simulated using a 15 $M_{\odot }$ progenitor
• Magnetorotational Core-Collapse Supernovae in Three Dimensions
• Pulsar Jets: Implications for Neutron Star Kicks and Initial Spins
• Supernova Simulations from a 3D Progenitor Model -- Impact of Perturbations and Evolution of Explosion Properties
• Instability of a stalled accretion shock: evidence for the advective-acoustic cycle
• Neutrino-driven explosion of a 20 solar-mass star in three dimensions enabled by strange-quark contributions to neutrino-nucleon scattering
• A New Multi-Dimensional General Relativistic Neutrino Hydrodynamics Code for Core-Collapse Supernovae II. Relativistic Explosion Models of Core-Collapse Supernovae
• Pulsar Recoil by Large-Scale Anisotropies in Supernova Explosions
• A Comparison of Two- and Three-dimensional Neutrino-hydrodynamics simulations of Core-collapse Supernovae
• Exploring Fundamentally Three-dimensional Phenomena in High-fidelity Simulations of Core-collapse Supernovae
• SASI Activity in Three-Dimensional Neutrino-Hydrodynamics Simulations of Supernova Cores
• Non-Radial Instabilities and Progenitor Asphericities in Core-Collapse Supernovae
• The Role of Turbulence in Neutrino-Driven Core-Collapse Supernova Explosions
• Three-Dimensional Simulations of Neutrino-Driven Core-Collapse Supernovae from Low-Mass Single and Binary Star Progenitors
• Revival of The Stalled Core-Collapse Supernova Shock Triggered by Precollapse Asphericity in the Progenitor Star
• The isotropic diffusion source approximation for supernova neutrino transport
• Neutrino-driven convection versus advection in core collapse supernovae
• General-Relativistic Simulations of Three-Dimensional Core-Collapse Supernovae
• Axisymmetric Ab Initio Core-Collapse Supernova Simulations of 12-25 M_sol Stars
• Muon Creation in Supernova Matter Facilitates Neutrino-driven Explosions
• A Successful 3D Core-Collapse Supernova Explosion Model
• Neutron star kicks by the gravitational tug-boat mechanism in asymmetric supernova explosions: progenitor and explosion dependence
• The Progenitor Dependence of the Preexplosion Neutrino Emission in Core-Collapse Supernovae
• Three-dimensional simulations of rapidly rotating core-collapse supernovae: finding a neutrino-powered explosion aided by non-axisymmetric flows
• Three-Dimensional Supernova Explosion Simulations of 9-, 10-, 11-, 12-, and 13-M${}_{\odot }$ Stars
• The Dynamics of Neutrino-Driven Supernova Explosions after Shock Revival in 2D and 3D
• General Relativistic Three-Dimensional Multi-Group Neutrino Radiation-Hydrodynamics Simulations of Core-Collapse Supernovae
• Rotation-supported Neutrino-driven Supernova Explosions in Three Dimensions and the Critical Luminosity Condition
• Quark deconfinement as supernova explosion engine for massive blue-supergiant stars
• The Progenitor Dependence of Three-Dimensional Core-Collapse Supernovae
• Explosion geometry of a rotating 13 $M_{\odot }$ star driven by the SASI-aided neutrino-heating supernova mechanism
• Effects of neutrino-driven kicks on the supernova explosion mechanism
• Systematic Features of Axisymmetric Neutrino-Driven Core-Collapse Supernova Models in Multiple Progenitors
• Multi-messenger signals of long-term core-collapse supernova simulations : synergetic observation strategies
• Progenitor-dependent Explosion Dynamics in Self-consistent, Axisymmetric Simulations of Neutrino-driven Core-collapse Supernovae
• Crucial Physical Dependencies of the Core-Collapse Supernova Mechanism
• Neutrino Transfer in Three Dimensions for Core-Collapse Supernovae. I. Static Configurations
• A New Multi-Energy Neutrino Radiation-Hydrodynamics Code in Full General Relativity and Its Application to Gravitational Collapse of Massive Stars
• Fully General Relativistic Simulations of Core-Collapse Supernovae with An Approximate Neutrino Transport
• Two Dimensional Core-Collapse Supernova Explosions Aided by General Relativity with Multidimensional Neutrino Transport
• Correlated Signatures of Gravitational-Wave and Neutrino Emission in Three-Dimensional General-Relativistic Core-Collapse Supernova Simulations
• Axisymmetric simulations of magnetorotational core collapse: Approximate inclusion of general relativistic effects
• Simulations of core-collapse supernovae in spatial axisymmetry with full Boltzmann neutrino transport
• Hydrodynamical Neutron-star Kicks in Electron-capture Supernovae and Implications for the CRAB Supernova
• Neutron Star Kicks and their Relationship to Supernovae Ejecta Mass
• Protomagnetar and black hole formation in high-mass stars
• Revival of the Fittest: Exploding Core-Collapse Supernovae from 12 to 25 M${}_{\odot }$
• Anisotropic emission of neutrino and gravitational-wave signals from rapidly rotating core-collapse supernovae
• Three-Dimensional Core-Collapse Supernova Simulations with Multi-Dimensional Neutrino Transport Compared to the Ray-by-Ray-plus Approximation
• One-, Two-, and Three-dimensional Simulations of Oxygen Shell Burning Just Before the Core-Collapse of Massive Stars
• Core-collapse supernova simulations in one and two dimensions: comparison of codes and approximations
• The Hydrodynamic Origin of Neutron Star Kicks
• Comparing Neutron Star Kicks to Supernova Remnant Asymmetries
• Asymmetric neutrino emision and formation of rapidly moving pulsars
• Neutrino-driven Turbulent Convection and Standing Accretion Shock Instability in Three-Dimensional Core-Collapse Supernovae
• Intermediate-Mass-Elements in Young Supernova Remnants Reveal Neutron Star Kicks by Asymmetric Explosions
• Theoretical Support for the Hydrodynamic Mechanism of Pulsar Kicks
• Impact of Neutrino Opacities on Core-Collapse Supernova Simulations
• Characterizing SASI- and Convection-Dominated Core-Collapse Supernova Explosions in Two Dimensions
• The NANOGrav Nine-year Data Set: Astrometric Measurements of 37 Millisecond Pulsars
• A Detailed Comparison of Multi-Dimensional Boltzmann Neutrino Transport Methods in Core-Collapse Supernovae
• Three-dimensional Boltzmann-Hydro code for core-collapse in massive stars II. The Implementation of moving-mesh for neutron star kicks
• Two-Dimensional Core-Collapse Supernova Simulations with the Isotropic Diffusion Source Approximation for Neutrino Transport
• Diffuse Supernova Neutrino Background from extensive core-collapse simulations of $8$-$100{\mathrm{M}}_{\odot }$ progenitors
• Neutron Star Kicks II: Revision and further testing of the conservation of momentum "kick" model
• Numerical simulations of the magnetorotational instability in protoneutron stars: I. Influence of buoyancy
• On the Neutrino Distributions in Phase Space for the Rotating Core-collapse Supernova Simulated with a Boltzmann-neutrino-radiation-hydrodynamics Code
• Pulsar kicks by anisotropic neutrino emission from quark matter in strong magnetic fields
• Magnetohydrodynamic Turbulence Powered by Magnetorotational Instability in Nascent Proto-Neutron Stars
• Delayed pulsar kicks from the emission of sterile neutrinos
• North-South Neutrino Heating Asymmetry in Strongly Magnetized and Rotating Stellar Cores
• Revisiting Impacts of Nuclear Burning for Reviving Weak Shocks in Neutrino-Driven Supernovae
• Neutron star natal kick and jets in core collapse supernovae
• Estimating the core compactness of massive stars with Galactic supernova neutrinos

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• Metastable Helium Absorptions with 3D Hydrodynamics and Self-Consistent Photochemistry I: WASP-69b, Dimensionality, XUV Flux Level, Spectral Types, and Flares
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• Two-dimensional numerical study for magnetic field dependence of neutrino-driven core-collapse supernova models
• Impact of magnetic field on neutrino-matter interactions in core-collapse supernova
• Ultra-delayed neutrino-driven explosion of rotating massive-star collapse
• Studying magnetic fields and dust in M17 using polarized thermal dust emission observed by SOFIA/HAWC+
• Laboratory modeling of jets from young stars using plasma focus facilities
• Neutrino flavor mixing with moments
• Universality in supernova gravitational waves with proto-neutron star properties
• Three-flavor collective neutrino conversions with multi-azimuthal-angle instability in an electron-capture supernova model
• The Proper Motion of the Pulsar J1124-5916 in the Galactic Supernova Remnant G292.0+1.8
• The rocket effect mechanism in neutron stars in supernova remnants
• Observing Supernova Neutrino Light Curves with Super-Kamiokande. III. Extraction of Mass and Radius of Neutron Stars from Synthetic Data
• Progenitor Dependence of Neutrino-driven Supernova Explosions with the Aid of Heavy Axion-like Particles
• Natal kicks of compact objects
• On the Zeeman Effect in Magnetically-Arrested Disks
• Hunting isolated neutron stars with proper motions from wide-area optical surveys
• Modeling the Galactic Neutron Star Population for Use in Continuous Gravitational Wave Searches