Hydrodynamics of core-collapse supernovae and their progenitors

Abstract

Multi-dimensional fluid flow plays a paramount role in the explosions of massive stars as core-collapse supernovae. In recent years, three-dimensional (3D) simulations of these phenomena have matured significantly. Considerable progress has been made towards identifying the ingredients for shock revival by the neutrino-driven mechanism, and successful explosions have already been obtained in a number of self-consistent 3D models. These advances also bring new challenges, however. Prompted by a need for increased physical realism and meaningful model validation, supernova theory is now moving towards a more integrated view that connects multi-dimensional phenomena in the late convective burning stages prior to collapse, the explosion engine, and mixing instabilities in the supernova envelope. Here we review our current understanding of multi-D fluid flow in core-collapse supernovae and their progenitors. We start by outlining specific challenges faced by hydrodynamic simulations of core-collapse supernovae and of the late convective burning stages. We then discuss recent advances and open questions in theory and simulations.

arXiv commentInvited review article for Living Reviews in Computational Astrophysics. 100 pages, 15 figures

References in corpus (340)

• Modules for Experiments in Stellar Astrophysics (MESA)
• E pur si muove: Galiliean-invariant cosmological hydrodynamical simulations on a moving mesh
• Modules for Experiments in Stellar Astrophysics (MESA): Convective Boundaries, Element Diffusion, and Massive Star Explosions
• The Supernova -- Gamma-Ray Burst Connection
• A statistical study of 233 pulsar proper motions
• Masses, Radii, and Equation of State of Neutron Stars
• Explosion Mechanisms of Core-Collapse Supernovae
• Equations of state for supernovae and compact stars
• Core-Collapse Supernovae from 9 to 120 Solar Masses Based on Neutrino-powered Explosions
• The Progenitor Stars of Gamma-Ray Bursts
• The Nuclear Equation of State and Neutron Star Masses
• Presupernova Evolution of Differentially Rotating Massive Stars Including Magnetic Fields
• The death of massive stars - I. Observational constraints on the progenitors of type II-P supernovae
• Birth and Evolution of Isolated Radio Pulsars
• Nucleosynthesis Yields of Core-Collapse Supernovae and Hypernovae, and Galactic Chemical Evolution
• Nucleosynthesis and Remnants in Massive Stars of Solar Metallicity
• Smoothed Particle Hydrodynamics and Magnetohydrodynamics
• Nucleosynthesis and Evolution of Massive Metal-Free Stars
• Stability of Standing Accretion Shocks, With an Eye Toward Core Collapse Supernovae
• On the Nature of Core Collapse Supernova Explosions
• Evolutions in 3D numerical relativity using fixed mesh refinement
• Inside the Supernova: A Powerful Convective Engine
• Observational constraints on the progenitors of core-collapse supernovae : the case for missing high mass stars
• Evolution of Protoneutron Stars
• Explosions of O-Ne-Mg Cores, the Crab Supernova, and Subluminous Type II-P Supernovae
• The Expulsion of Stellar Envelopes in Core-Collapse Supernovae
• Magnetorotationally driven Supernovae as the origin of early galaxy $r$-process elements?
• Progenitor-Explosion Connection and Remnant Birth Masses for Neutrino-Driven Supernovae of Iron-Core Progenitors
• Physics of Core-Collapse Supernovae in Three Dimensions: a Sneak Preview
• Simulations of Magnetically-Driven Supernova and Hypernova Explosions in the Context of Rapid Rotation
• The Magnetorotational Instability in Core Collapse Supernova Explosions
• Perspectives on Core-Collapse Supernova Theory
• Two-dimensional hydrodynamic core-collapse supernova simulations with spectral neutrino transport. I. Numerical method and results for a 15 M_sun star
• First-generation black-hole-forming supernovae and the metal abundance pattern of a very iron-poor star
• Neutrino Signal of Electron-Capture Supernovae from Core Collapse to Cooling
• Delayed neutrino-driven supernova explosions aided by the standing accretion-shock instability
• Radiation hydrodynamics with neutrinos: Variable Eddington factor method for core-collapse supernova simulations
• A two-parameter criterion for classifying the explodability of massive stars by the neutrino-driven mechanism
• Spectropolarimetry of Supernovae
• A single low-energy, iron-poor supernova as the source of metals in the star SMSS J 031300.36-670839.3
• Turbulent Convection in Stellar Interiors. I. Hydrodynamic Simulation
• The "Yin-Yang Grid": An Overset Grid in Spherical Geometry
• Multidimensional Supernova Simulations with Approximative Neutrino Transport I. Neutron Star Kicks and the Anisotropy of Neutrino-Driven Explosions in Two Spatial Dimensions
• Type II Supernovae: Model Light Curves and Standard Candle Relationships
• Pulsar Recoil and Gravitational Radiation due to Asymmetrical Stellar Collapse and Explosion
• Probing the gravitational well: No supernova explosion in spherical symmetry with general relativistic Boltzmann neutrino transport
• Supernova Simulations with Boltzmann Neutrino Transport: A Comparison of Methods
• Non-spherical Core Collapse Supernovae I. Neutrino-Driven Convection, Rayleigh-Taylor Instabilities, and the Formation and Propagation of Metal Clumps
• Explosion Mechanism, Neutrino Burst, and Gravitational Wave in Core-Collapse Supernovae
• The Remarkable Deaths of 9 - 11 Solar Mass Stars
• A Finite Difference Representation of Neutrino Radiation Hydrodynamics in Spherically Symmetric General Relativistic Space-Time
• On the formation history of Galactic double neutron stars
• A New Multi-Dimensional General Relativistic Neutrino Hydrodynamics Code of Core-Collapse Supernovae III. Gravitational Wave Signals from Supernova Explosion Models
• Three-dimensional neutrino-driven supernovae: Neutron star kicks, spins, and asymmetric ejection of nucleosynthesis products
• Two-Dimensional Hydrodynamic Core-Collapse Supernova Simulations with Spectral Neutrino Transport II. Models for Different Progenitor Stars
• The Compactness of Presupernova Stellar Cores
• Why pulsars rotate and move: kicks at birth
• The solar magnetic field
• Three-dimensional core-collapse supernova simulated using a 15 $M_{\odot }$ progenitor
• Spherically Symmetric Simulation with Boltzmann Neutrino Transport of Core Collapse and Post-Bounce Evolution of a 15 Solar Mass Star
• Magnetorotational Core-Collapse Supernovae in Three Dimensions
• The Overarching Framework of Core-Collapse Supernova Explosions as Revealed by 3D Fornax Simulations
• Pulsar Jets: Implications for Neutron Star Kicks and Initial Spins
• Electron-capture supernovae as the origin of elements beyond iron
• Conditions for Shock Revival by Neutrino Heating in Core-Collapse Supernovae
• Asymmetries in core-collapse supernovae from maps of radioactive ${}^{44}$Ti in CassiopeiaA
• Supernova Simulations from a 3D Progenitor Model -- Impact of Perturbations and Evolution of Explosion Properties
• Three-Dimensional Simulations of Core-Collapse Supernovae: From Shock Revival to Shock Breakout
• Bipolar Supernova Explosions: Nucleosynthesis & Implication on Abundances in Extremely Metal-Poor Stars
• 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
• Pulsar spins from an instability in the accretion shock of supernovae
• 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
• The Landscape of the Neutrino Mechanism of Core-Collapse Supernovae: Neutron Star and Black Hole Mass Functions, Explosion Energies and Nickel Yields
• A Simple Approach to the Supernova Progenitor-Explosion Connection
• Dimension as a Key to the Neutrino Mechanism of Core-Collapse Supernova Explosions
• Three-Dimensional Simulations of Mixing Instabilities in Supernova Explosions
• SASI Activity in Three-Dimensional Neutrino-Hydrodynamics Simulations of Supernova Cores
• Investigating stellar-mass black hole kicks
• Exploring Fundamentally Three-dimensional Phenomena in High-fidelity Simulations of Core-collapse Supernovae
• Non-Radial Instabilities and Progenitor Asphericities in Core-Collapse Supernovae
• On the nature of supernovae Ib and Ic
• Evidence for alignment of the rotation and velocity vectors in pulsars
• An HLLC Riemann Solver for Relativistic Flows: I. Hydrodynamics
• Is Strong SASI Activity the Key to Successful Neutrino-Driven Supernova Explosions?
• Towards Realistic Progenitors of Core-Collapse Supernovae
• Three-dimensional Hydrodynamic Core-Collapse Supernova Simulations for an $11.2M_{\odot }$ Star with Spectral Neutrino Transport
• 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
• Viscosity and Rotation in Core-Collapse Supernovae
• Revival of The Stalled Core-Collapse Supernova Shock Triggered by Precollapse Asphericity in the Progenitor Star
• 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
• The Spherical Accretion Shock Instability in the Linear Regime
• Criteria for Core-Collapse Supernova Explosions by the Neutrino Mechanism
• Advanced burning stages and fate of 8-10 Mo stars
• Neutrino-driven convection versus advection in core collapse supernovae
• Characterizing the Gravitational Wave Signal from Core-Collapse Supernovae
• Multidimensional supernova simulations with approximative neutrino transport. II. Convection and the advective-acoustic cycle in the supernova core
• 3-Dimensional Core-Collapse
• Multiple physical elements to determine the gravitational-wave signatures of core-collapse supernovae
• A new multi-dimensional general relativistic neutrino hydrodynamics code for core-collapse supernovae. I. Method and code tests in spherical symmetry
• Axisymmetric Ab Initio Core-Collapse Supernova Simulations of 12-25 M_sol Stars
• The Development of Explosions in Axisymmetric Ab Initio Core-Collapse Supernova Simulations of 12-25 $M_{\odot }$ Stars
• Relativistic simulations of rotational core collapse. I. Methods, initial models, and code tests
• Muon Creation in Supernova Matter Facilitates Neutrino-driven Explosions
• A Successful 3D Core-Collapse Supernova Explosion Model
• Equation-of-State Dependent Features in Shock-Oscillation Modulated Neutrino and Gravitational-Wave Signals from Supernovae
• The gravitational wave signal from core-collapse supernovae
• Anomalously Weak Solar Convection
• Gravitational Wave Signals from 3D Neutrino Hydrodynamics Simulations of Core-Collapse Supernovae
• How much H and He is "hidden" in SNe Ib/c? I. - low-mass objects
• 3D Collapse of Rotating Stellar Iron Cores in General Relativity including Deleptonization and a Nuclear Equation of State
• New Two-Dimensional Models of Supernova Explosions by the Neutrino-Heating Mechanism: Evidence for Different Instability Regimes in Collapsing Stellar Cores
• Self-sustained asymmetry of lepton-number emission: A new phenomenon during the supernova shock-accretion phase in three dimensions
• Neutron star kicks by the gravitational tug-boat mechanism in asymmetric supernova explosions: progenitor and explosion dependence
• Modeling Core-Collapse Supernovae in 3-Dimensions
• Nucleosynthesis and Clump Formation in a Core Collapse Supernova
• Modelling of isolated radio pulsars and magnetars on the fossil field hypothesis
• R-process Nucleosynthesis from Three-Dimensional Magnetorotational Core-Collapse Supernovae
• A constrained scheme for Einstein equations based on Dirac gauge and spherical coordinates
• Features of the Acoustic Mechanism of Core-Collapse Supernova Explosions
• Ledoux-Convection in Protoneutron Stars --- a Clue to Supernova Nucleosynthesis?
• Numerical Analysis on Standing Accretion Shock Instability with Neutrino Heating in the Supernova Cores
• Super-AGB Stars and their role as Electron Capture Supernova progenitors
• Magnetorotational collapse of massive stellar cores to neutron stars: Simulations in full general relativity
• Fornax: a Flexible Code for Multiphysics Astrophysical Simulations
• Axisymmetric simulations of magneto--rotational core collapse: dynamics and gravitational wave signal
• Gravitational Waves from Core Collapse Supernovae
• Long Gamma-Ray Transients from Collapsars
• Investigation of Neutrino-Driven Convection and the Core Collapse Supernova Mechanism Using Multigroup Neutrino Transport
• A new multidimensional, energy-dependent two-moment transport code for neutrino-hydrodynamics
• Neutrino emission characteristics and detection opportunities based on three-dimensional supernova simulations
• Production and Distribution of ${}^{44}$Ti and ${}^{56}$Ni in a Three-dimensional Supernova Model Resembling Cassiopeia A
• GRHydro: A new open source general-relativistic magnetohydrodynamics code for the Einstein Toolkit
• Proto-Neutron Star Cooling with Convection: The Effect of the Symmetry Energy
• Three-dimensional simulations of rapidly rotating core-collapse supernovae: finding a neutrino-powered explosion aided by non-axisymmetric flows
• The Dynamics of Neutrino-Driven Supernova Explosions after Shock Revival in 2D and 3D
• Three-Dimensional Supernova Explosion Simulations of 9-, 10-, 11-, 12-, and 13-M${}_{\odot }$ Stars
• 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
• The Dominance of Neutrino-Driven Convection in Core-Collapse Supernovae
• The Three Dimensional Evolution to Core Collapse of a Massive Star
• Low Mach Number Modeling of Type Ia Supernovae
• Improved constrained scheme for the Einstein equations: An approach to the uniqueness issue
• Magnetorotational supernovae
• Multi-Dimensional Radiation/Hydrodynamic Simulations of Protoneutron Star Convection
• The Progenitor Dependence of Three-Dimensional Core-Collapse Supernovae
• Three-Dimensional Simulations of Standing Accretion Shock Instability in Core-Collapse Supernovae
• A New Gravitational-Wave Signature from Standing Accretion Shock Instabilities in Supernovae
• Explosion geometry of a rotating 13 $M_{\odot }$ star driven by the SASI-aided neutrino-heating supernova mechanism
• Systematic Features of Axisymmetric Neutrino-Driven Core-Collapse Supernova Models in Multiple Progenitors
• High-Resolution Three-Dimensional Simulations of Core-Collapse Supernovae in Multiple Progenitors
• TESS: A Relativistic Hydrodynamics Code on a Moving Voronoi Mesh
• Do electron-capture supernovae make neutron stars? First multidimensional hydrodynamic simulations of the oxygen deflagration
• Numerical Relativity and Astrophysics
• The Last Minutes of Oxygen Shell Burning in a Massive Star
• Gravitational Wave Emission from 3D Explosion Models of Core-Collapse Supernovae with Low and Normal Explosion Energies
• Progenitor-dependent Explosion Dynamics in Self-consistent, Axisymmetric Simulations of Neutrino-driven Core-collapse Supernovae
• Active Carbon and Oxygen Shell Burning Hydrodynamics
• Hydrodynamical Neutron Star Kicks in Three Dimensions
• Crucial Physical Dependencies of the Core-Collapse Supernova Mechanism
• Magnetorotational core collapse of possible GRB progenitors. I. Explosion mechanisms
• Two-Dimensional Hydrodynamics of Pre-Core Collapse: Oxygen Shell Burning
• A New Multi-Energy Neutrino Radiation-Hydrodynamics Code in Full General Relativity and Its Application to Gravitational Collapse of Massive Stars
• Pulsar Spin-Velocity Alignment: Kinematic Ages, Birth Periods and Braking Indices
• Turbulent Convection in Stellar Interiors. II. The Velocity Field
• The Nucleosynthetic Imprint of 15-40 Solar Mass Primordial Supernovae on Metal-Poor Stars
• Neutrino signature of supernova hydrodynamical instabilities in three dimensions
• "Mariage des Maillages": A new numerical approach for 3D relativistic core collapse simulations
• The Fast and Furious Decay of the Peculiar Type Ic Supernova 2005ek
• Refined numerical models for multidimensional Type Ia supernova simulations
• Black hole formation and fallback during the supernova explosion of a $40{\mathrm{M}}_{\odot }$ star
• Late Spectral Evolution of SN 1987A: II. Line Emission
• On The Intrinsic Diversity of Type II-Plateau Supernovae
• A hot and fast ultra-stripped supernova that likely formed a compact neutron star binary
• Fully General Relativistic Simulations of Core-Collapse Supernovae with An Approximate Neutrino Transport
• Mapping Initial Hydrostatic Models in Godunov Codes
• Dimensional Dependence of the Hydrodynamics of Core-Collapse Supernovae
• Two Dimensional Core-Collapse Supernova Explosions Aided by General Relativity with Multidimensional Neutrino Transport
• Non-radial instabilities of isothermal Bondi accretion with a shock: vortical-acoustic cycle vs post-shock acceleration
• Two-dimensional, Time-dependent, Multi-group, Multi-angle Radiation Hydrodynamics Test Simulation in the Core-Collapse Supernova Context
• Beyond Mixing-length Theory: a step toward 321D
• Temporal and Angular Variations of 3D Core-Collapse Supernova Emissions and their Physical Correlations
• The Spiral Modes of the Standing Accretion Shock Instability
• Simulating Self-gravitating Hydrodynamic Flows
• The Nickel Mass Distribution of Normal Type II Supernovae
• Turbulent convection in stellar interiors. III. Mean-field analysis and stratification effects
• Magnetic field amplification and magnetically supported explosions of collapsing, non-rotating stellar cores
• Mixing in Zero and Solar Metallicity Supernovae
• On the Impact of Three Dimensions in Simulations of Neutrino-Driven Core-Collapse Supernova Explosions
• The First Second of a Type-II Supernova: Convection, Accretion, and Shock Propagation
• SNSPH: A Parallel 3-D Smoothed Particle Radiation Hydrodynamics Code
• Radiative-transfer models for supernovae IIb/Ib/Ic from binary-star progenitors
• Magnetically-driven explosions of rapidly-rotating white dwarfs following Accretion-Induced Collapse
• Hydrodynamical Neutron-star Kicks in Electron-capture Supernovae and Implications for the CRAB Supernova
• A full general relativistic neutrino radiation-hydrodynamics simulation of a collapsing very massive star and the formation of a black hole
• Correlated Gravitational Wave and Neutrino Signals from General-Relativistic Rapidly Rotating Iron Core Collapse
• Neutron Star Kicks and their Relationship to Supernovae Ejecta Mass
• MAESTRO: An Adaptive Low Mach Number Hydrodynamics Algorithm for Stellar Flows
• Protomagnetar and black hole formation in high-mass stars
• Growth of Perturbation in Gravitational Collapse and Accretion
• Neutrino-driven explosions of ultra-stripped type Ic supernovae generating binary neutron stars
• Birth Kick Distributions and the Spin-Kick Correlation of Young Pulsars
• One-, Two-, and Three-dimensional Simulations of Oxygen Shell Burning Just Before the Core-Collapse of Massive Stars
• Turbulent Magnetic Field Amplification from Spiral SASI Modes: Implications for Core-Collapse Supernovae and Proto-Neutron Star Magnetization
• Idealised hydrodynamic simulations of turbulent oxygen-burning shell convection in 4π geometry
• Anisotropies in the Neutrino Fluxes and Heating Profiles in Two-dimensional, Time-dependent, Multi-group Radiation Hydrodynamics Simulations of Rotating Core-Collapse Supernovae
• Turbulent Cells in Stars: I. Fluctuations in Kinetic Energy and Luminosity
• A Global Turbulence Model for Neutrino-Driven Convection in Core-Collapse Supernovae
• 3D hydrodynamical simulations of a proton ingestion episode in a low-metallicity asymptotic giant branch star
• Initial spin periods of neutron stars in supernova remnants
• 3D Numerical Experimentation on the Core Helium Flash of low-mass Red Giants
• Numerical Relativity in Spherical Polar Coordinates: Evolution Calculations with the BSSN Formulation
• Core-collapse supernova simulations in one and two dimensions: comparison of codes and approximations
• Three Dimensional MHD Simulations of Accretion to an Inclined Rotator: The "Cubed Sphere" Method
• On the Importance of the Equation of State for the Neutrino-Driven Supernova Explosion Mechanism
• Fast time variations of supernova neutrino fluxes and their detectability
• 3D Hydrodynamic Simulations of Carbon Burning in Massive Stars
• The Physics of the Neutrino Mechanism of Core-Collapse Supernovae
• A New Multi-Dimensional General Relativistic Neutrino Hydrodynamics Code for Core-Collapse Supernovae IV. The Neutrino Signal
• The Hydrodynamic Origin of Neutron Star Kicks
• The impact of fallback on the compact remnants and chemical yields of core-collapse supernovae
• Equation of State Dependent Dynamics and Multimessenger Signals from Stellar-mass Black Hole Formation
• Multi-D Simulations of Ultra-Stripped Supernovae to Shock Breakout
• New numerical solver for flows at various Mach numbers
• On the Requirements for Realistic Modeling of Neutrino Transport in Simulations of Core-Collapse Supernovae
• Large-Scale Mixing in a Violent Oxygen-Neon Shell Merger Prior to a Core-Collapse Supernova
• Entropic-acoustic instability of shocked Bondi accretion I. What does perturbed Bondi accretion sound like ?
• Aspherical Core-Collapse Supernovae in Red Supergiants Powered by Nonrelativistic Jets
• Effect of Rotation on the Stability of a Stalled Cylindrical Shock and its Consequences for Core-Collapse Supernovae
• High-Resolution Simulations of Convection Preceding Ignition in Type Ia Supernovae Using Adaptive Mesh Refinement
• Three-Dimensional Simulations of SASI- and Convection-Dominated Core-Collapse Supernovae
• Three-Dimensional General-Relativistic Hydrodynamic Simulations of Binary Neutron Star Coalescence and Stellar Collapse with Multipatch Grids
• Effects of Rotation on Standing Accretion Shock Instability in Nonlinear Phase for Core-Collapse Supernovae
• Observational Tests and Predictive Stellar Evolution II: Non-standard Models
• An Improved Multipole Approximation for Self-Gravity and Its Importance for Core-Collapse Supernova Simulations
• Gamma-Ray Lines from Asymmetric Supernovae
• Neutrino-driven Turbulent Convection and Standing Accretion Shock Instability in Three-Dimensional Core-Collapse Supernovae
• Effects of Jet-like Explosion in SN 1987A
• Theoretical Support for the Hydrodynamic Mechanism of Pulsar Kicks
• Anelastic and Compressible Simulations of Stellar Oxygen Burning
• The core helium flash revisited: II. Two and three-dimensional hydrodynamic simulations
• Toward a consistent use of overshooting parametrizations in 1D stellar evolution codes
• Characterizing SASI- and Convection-Dominated Core-Collapse Supernova Explosions in Two Dimensions
• Neutrino Emission as Diagnostics of Core-Collapse Supernovae
• Thermonuclear Kinetics in Astrophysics
• Neutrino-Driven Convection in Core-Collapse Supernovae: High-Resolution Simulations
• Stability of a Spherical Accretion Shock with Nuclear Dissociation
• Rayleigh-Taylor Instability in a Relativistic Fireball on a Moving Computational Grid
• 3D simulations of Rayleigh-Taylor mixing in core-collapse SNe with CASTRO
• Convective-reactive nucleosynthesis of K, Sc, Cl and p-process isotopes in O-C shell mergers
• Application of the Cubed-Sphere Grid to Tilted Black-Hole Accretion Disks
• An axis-free overset grid in spherical polar coordinates for simulating 3D self-gravitating flows
• The Core-Collapse Supernova with "Non-Uniform" Magnetic Fields
• Generation of Magnetic Fields by the Stationary Accretion Shock Instability
• Dynamics of a Spherical Accretion Shock with Neutrino Heating and Alpha-Particle Recombination
• 3D hydrodynamic simulations of C ingestion into a convective O shell
• Supernova 1987A: neutrino-driven explosions in three dimensions and light curves
• Astrophysical hydrodynamics with a high-order discontinuous Galerkin scheme and adaptive mesh refinement
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• Towards a new generation of multi-dimensional stellar evolution models: development of an implicit hydrodynamic code
• Hydrodynamics of Core-Collapse Supernovae at the Transition to Explosion. I. Spherical Symmetry
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• Effects of LESA in Three-Dimensional Supernova Simulations with Multi-Dimensional and Ray-by-Ray-plus Neutrino Transport
• Further Adventures: Oxygen Burning in a Convective Shell
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• A 3D Simulation of a Neutrino-Driven Supernova Explosion Aided By Convection and Magnetic Fields
• The final core collapse of pulsational pair instability supernovae
• Inference of proto-neutron star properties from gravitational-wave data in core-collapse supernovae
• Three dimensional magnetorotational core-collapse supernova explosions of a 39 solar mass progenitor star
• Emission lines due to ionizing radiation from a compact object in the remnant of Supernova 1987A
• Evaluating Approximate Flavor Instability Metrics in Neutron Star Mergers
• The physics of Core-Collapse Supernovae: explosion mechanism and explosive nucleosynthesis
• Gmunu: Paralleled, grid-adaptive, general-relativistic magnetohydrodynamics in curvilinear geometries in dynamical spacetimes
• Magnetic support for neutrino-driven explosion of 3D non-rotating core-collapse supernova models
• New method for detecting fast neutrino flavor conversions in core-collapse supernova models with two-moment neutrino transport
• 3D Simulations of Oxygen Shell Burning with and without Magnetic Fields
• The Impact of Black Hole Formation on Population Averaged Supernova Yields
• PUSHing core-collapse supernovae to explosions in spherical symmetry V: Equation of state dependency of explosion properties, nucleosynthesis yields, and compact remnants
• An Observationally-Derived Kick Distribution for Neutron Stars in Binary Systems
• The Role of the Hadron-Quark Phase Transition in Core-Collapse Supernovae
• Gravitational Waves from Core-Collapse Supernovae
• Calibration of neutron star natal kick velocities to isolated pulsar observations
• Fast-rotating massive Population~III stars as possible sources of extreme N-enrichment in high-redshift galaxies
• Two-dimensional numerical study for magnetic field dependence of neutrino-driven core-collapse supernova models
• Effect of the Nuclear Equation of State on Relativistic-Turbulence Induced Core-Collapse Supernovae
• Ultra-delayed neutrino-driven explosion of rotating massive-star collapse
• Explodability criteria for the neutrino-driven supernova mechanism
• A Comparison of 2D Magnetohydrodynamic Supernova Simulations with the CoCoNuT-FMT and Aenus-Alcar Codes
• Multidimensional low-Mach number time-implicit hydrodynamic simulations of convective helium shell burning in a massive star
• A DG-IMEX method for two-moment neutrino transport: Nonlinear solvers for neutrino-matter coupling
• Microscopic nuclear equation of state at finite temperature and stellar stability
• Core-collapse supernova simulations with reduced nucleosynthesis networks
• Raising the observed metallicity floor with a 3D non-LTE analysis of SDSS J102915.14+172927.9
• Spontaneous Scalarization as a New Core-Collapse Supernova Mechanism and its Multi-Messenger Signals
• Modelling supernova nebular lines in 3D with $\text{ExTraSS}$
• Long-term gravitational wave asteroseismology of supernova: from core collapse to 20 seconds postbounce
• Differential Rotation in a 3D Simulation of Oxygen Shell Burning
• The Galactic Underworld: The spatial distribution of compact remnants
• A finite-volume scheme for modeling compressible magnetohydrodynamic flows at low Mach numbers in stellar interiors
• Effect of stellar rotation on the development of post-shock instabilities during core-collapse supernovae
• The stochastic enrichment of Population II stars
• Exploring Supernova Gravitational Waves with Machine Learning
• Middle aged $\gamma$-ray pulsar J1957+5033 in X-rays: pulsations, thermal emission and nebula
• Comparison between core-collapse supernova nucleosynthesis and meteoric stardust grains: investigating magnesium, aluminium, and chromium
• thornado-hydro: a discontinuous Galerkin method for supernova hydrodynamics with nuclear equations of state
• Standing Accretion Shock Instability in the Collapse of a Rotating Stellar Core
• Probing nuclear physics with supernova gravitational waves and machine learning
• Black Hole Supernovae, their Equation of State Dependence and Ejecta Composition
• Parameterisations of thermal bomb explosions for core-collapse supernovae and 56Ni production
• Inferring Type II-P Supernova Progenitor Masses from Plateau Luminosities
• Magnetorotational neutron star kicks
• Fallback onto Kicked Neutron Stars and its Effect on Spin-Kick Alignment
• Light Curves of Type IIP Supernovae from Neutrino-driven Explosions of Red Supergiants Obtained by a Semi-analytic Approach
• Thermodynamics of oscillating neutrinos
• Effective Chiral Magnetic Effect from Neutrino Radiation
• 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
• Hydrodynamics and Nucleosynthesis of Jet-Driven Supernovae II: Comparisons with Abundances of Extremely Metal-Poor Galaxies and Constraints on Supernova Progenitors
• Neutrino quantum kinetics in two spatial dimensions
• Phase-transition-induced collapse of proto-compact stars and its implication for supernova explosions
• A New Constraint on the Nuclear Equation of State from Statistical Distributions of Compact Remnants of Supernovae
• Tracing the ejecta structure of SN 1987A: Insights and diagnostics from 3D MHD simulations
• Modifications to the signal from a gravitational wave event due to a surrounding shell of matter
• Energy conserving and well-balanced discontinuous Galerkin methods for the Euler-Poisson equations in spherical symmetry
• A kinematically constrained kick distribution for isolated neutron stars
• Natal kicks of compact objects
• Detecting and reconstructing gravitational waves from the next Galactic core-collapse supernova in the Advanced Detector Era
• Evaluating Machine Learning Models for Supernova Gravitational Wave Signal Classification
• Magnetic Webs in Stellar Radiative Zones
• Core Collapse Supernova Gravitational Wave Sourcing and Characterization based on Three-Dimensional Models
• A Black-Hole Excision Scheme for General Relativistic Core-Collapse Supernova Simulations
• Advection Algorithms for Quantum Neutrino Moment Transport
• Comparison of Electron Capture Rates in the N=50 Region using 1D Simulations of Core-collapse Supernovae
• Performance of high-order Godunov-type methods in simulations of astrophysical low Mach number flows
• Binarity at LOw Metallicity (BLOeM): Bayesian inference of natal kicks from inert black hole binaries
• A Parametric Study of the SASI Comparing General Relativistic and Nonrelativistic Treatments
• Spherically Symmetric Accretion onto a Compact Object through a Standing Shock: The Effects of General Relativity in the Schwarzschild Geometry
• Plasma Instabilities Dominate Radioactive Transients Magnetic Fields: The self-confinement of leptons in Type Ia and Core-Collapse Supernovae, and Kilonovae
• Core-Collapse Supernovae: From Neutrino-Driven 1D Explosions to Light Curves and Spectra
• Fluid Dynamics in Curvilinear Coordinates without Fictitious Forces
• On the algebraic stretching dynamics of variable-density mixing in shock-bubble interaction
• Neutrino transport with Monte Carlo method: II. Quantum Kinetic Equations
• Constraints on Weak Supernova Kicks from Observed Pulsar Velocities
• Matter- and magnetically-driven flavor conversion of neutrinos in magnetorotational collapses
• Neutrino magnetohydrodynamic instabilities in presence of two-flavor oscillations
• On Neutron Star Natal Kicks in High-Mass X-Ray Binaries: Insights from Population Synthesis
• Convection signatures in early-time gravitational waves from core-collapse supernovae
• Time integration for neutrino radiation transport using minimally implicit Runge-Kutta methods
• 3D Synthetic Convective Velocity Fields to Initialise Core-Collapse Supernova Simulations from 1D Progenitors
• Proto-neutron star oscillations including accretion flows
• Neutrino flavor instabilities in neutron star mergers with moment transport: Slow, fast, and collisional modes
• Assessing the Distance for Probing the Nuclear Equation of State with Supernova Gravitational Waves
• Comprehensive neutrino light curves and spectra: from pre-supernova evolution to early supernova phase
• Revisiting the Perseus Cluster III: Role of Aspherical Explosions on its Chemical Composition and Extension to Metal-Poor Stars and Galaxies
• GenASiS: General Astrophysical Simulation System. II. Self-gravitating Baryonic Matter