Explosion Mechanisms of Core-Collapse Supernovae

Abstract

Supernova theory, numerical and analytic, has made remarkable progress in the past decade. This progress was made possible by more sophisticated simulation tools, especially for neutrino transport, improved microphysics, and deeper insights into the role of hydrodynamic instabilities. Violent, large-scale nonradial mass motions are generic in supernova cores. The neutrino-heating mechanism, aided by nonradial flows, drives explosions, albeit low-energy ones, of ONeMg-core and some Fe-core progenitors. The characteristics of the neutrino emission from new-born neutron stars were revised, new features of the gravitational-wave signals were discovered, our notion of supernova nucleosynthesis was shattered, and our understanding of pulsar kicks and explosion asymmetries was significantly improved. But simulations also suggest that neutrino-powered explosions might not explain the most energetic supernovae and hypernovae, which seem to demand magnetorotational driving. Now that modeling is being advanced from two to three dimensions, more realism, new perspectives, and hopefully answers to long-standing questions are coming into reach.

35 pages, 11 figures (29 eps files; high-quality versions can be obtained upon request); accepted by Annual Review of Nuclear and Particle Science

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• Neutrino halo effect on collective neutrino oscillation in iron core-collapse supernova model of a 9.6 $M_{\odot }$ star
• J0453+1559: a neutron star-white dwarf binary from a thermonuclear electron-capture supernova?
• An Observationally-Derived Kick Distribution for Neutron Stars in Binary Systems
• Identifying rotation in SASI-dominated core-collapse supernovae with a neutrino gyroscope
• Solar r-process-constrained actinide production in neutrino-driven winds of supernovae
• Robust measurement of supernova ${\nu }_e$ spectra with future neutrino detectors
• The Role of the Hadron-Quark Phase Transition in Core-Collapse Supernovae
• Three-Dimensional Kinematic Reconstruction of the Optically-Emitting, High-Velocity, Oxygen-Rich Ejecta of Supernova Remnant N132D
• Classifying the Equation of State from Rotating Core Collapse Gravitational Waves with Deep Learning
• Gravitational Waves from Core-Collapse Supernovae
• Influence of density dependence of symmetry energy in hot and dense matter for supernova simulations
• Supernova Constraints on Dark Flavored Sectors
• Spectropolarimetry of the Type Ib Supernova iPTF 13bvn: Revealing the complex explosion geometry of a stripped-envelope core-collapse supernova
• Low-energy Population III supernovae and the origin of extremely metal-poor stars
• Formation Timescales for High-Mass X-ray Binaries in M33
• EDGE: The sensitivity of ultra-faint dwarfs to a metallicity-dependent initial mass function
• Failure of a neutrino-driven explosion after core-collapse may lead to a thermonuclear supernova
• Calibration of neutron star natal kick velocities to isolated pulsar observations
• Matter mixing in aspherical core-collapse supernovae: a search for possible conditions for conveying ${}^{56}$Ni into high velocity regions
• Two-dimensional numerical study for magnetic field dependence of neutrino-driven core-collapse supernova models
• An Integral Condition for Core-Collapse Supernova Explosions
• Multi-Frequency General Relativistic Radiation-Hydrodynamics with ${\mathbf{M}}_1$ Closure
• Quantum Simulations of Nuclei and Nuclear Pasta with the Multi-resolution Adaptive Numerical Environment for Scientific Simulations
• Impact of systematic nuclear uncertainties on composition and decay heat of dynamical and disk ejecta in compact binary mergers
• Opportunities for Neutrino Physics at the Spallation Neutron Source: A White Paper
• Thermal evolution of neo-neutron stars. I: envelopes, Eddington luminosity phase and implications for GW170817
• A Critical Assessment of Turbulence Models for 1D Core-Collapse Supernova Simulations
• Asymmetric core collapse of rapidly rotating massive star
• SN 2012ca: a stripped envelope core-collapse SN interacting with dense circumstellar medium
• Revisiting Impacts of Nuclear Burning for Reviving Weak Shocks in Neutrino-Driven Supernovae
• Nothing to see here: Failed supernovae are faint or rare
• Spectrum of Supernova Neutrinos in Ultra-pure Scintillators
• Stochasticity and efficiency of simplified core-collapse supernova explosions
• A 3D Simulation of a Type II-P Supernova: from Core Bounce to Beyond Shock Breakout
• Nucleosynthesis Constraints on the Energy Growth Timescale of a Core-collapse Supernova Explosion
• The Zwicky Transient Facility phase I sample of hydrogen-rich superluminous supernovae without strong narrow emission lines
• The Energy Sources of Superluminous Supernovae
• Effect of the Nuclear Equation of State on Relativistic-Turbulence Induced Core-Collapse Supernovae
• The Role of Nucleon Strangeness in Supernova Explosions
• Impact of sterile neutrino dark matter on core-collapse supernovae
• On the effects of the Initial Mass Function on Galactic chemical enrichment
• Non-thermal radio supernova remnants of exiled Wolf-Rayet stars
• The Supernova -- Supernova Remnant Connection
• Detecting extra-galactic supernova neutrinos in the Antarctic ice
• 2D radiaition-hydrodynamic simulations of supernova shock breakout in bipolar explosions of a blue supergiant progenitor
• Gravitational waves and neutrino oscillations in Chern-Simons axion gravity
• The Impact of Progenitor Mass Loss on the Dynamical and Spectral Evolution of Supernova Remnants
• Active-sterile Neutrino Oscillations in Neutrino-driven Winds: Implications for Nucleosynthesis
• Expected impact from weak reactions with light nuclei in core-collapse supernova simulations
• On the energy source of ultra-stripped supernovae
• A Novel Multi-Dimensional Boltzmann Neutrino Transport Scheme for Core-Collapse Supernovae
• Probing nonlinear electrodynamics in slowly rotating spacetimes through neutrino astrophysics
• MODA: a new algorithm to compute optical depths in multi-dimensional hydrodynamic simulations
• Starburst and post-starburst high-redshift protogalaxies: The feedback impact of high energy cosmic rays
• Medium modifications for light and heavy nuclear clusters in simulations of core collapse supernovae -- Impact on equation of state and weak interactions
• OGLE-2014-SN-073 as a fallback accretion powered supernova
• Progenitors of low-mass binary black-hole mergers in the isolated binary evolution scenario
• General-relativistic radiation transport scheme in $\text{Gmunu}$ I: Implementation of two-moment based multi-frequency radiative transfer and code tests
• Is the Birth of PSR J0538+2817 Accompanied by a Gamma-ray Burst?
• A Comparison of 2D Magnetohydrodynamic Supernova Simulations with the CoCoNuT-FMT and Aenus-Alcar Codes
• Robust integration of fast flavor conversions in classical neutrino transport
• Unified nuclear matter EOSs constrained by the in-medium balance in density-dependent covariant density functionals
• Application of the nuclear equation of state obtained by the variational method to core-collapse supernovae
• Nuclear pasta structures and symmetry energy
• Multidimensional Boltzmann Neutrino Transport Code in Full General Relativity for Core-collapse Simulations
• Revisiting the Triangulation Method for Pointing to Supernova and Failed Supernova with Neutrinos
• Boosting jittering jets by neutrino heating in core collapse supernovae
• SIMBA-C: An updated chemical enrichment model for galactic chemical evolution in the SIMBA simulation
• SN2020qlb: A hydrogen-poor superluminous supernova with well-characterized light curve undulations
• Large-scale expansion of OB stars in Cygnus
• A Deep Near-Infrared [Fe II]+[Si I] Emission Line Image of the Supernova Remnant Cassiopeia A
• Interactions between Ultra-High-Energy Particles and Protogalactic Environments
• Supernova Limits on Muonic Dark Forces
• Remnant masses of core collapse supernovae in the jittering jets explosion mechanism
• Post-explosion evolution of core-collapse supernovae
• Confirming NGC 6231 as the parent cluster of the runaway high-mass X-ray binary HD 153919/4U 1700-37 with Gaia DR2
• SN2017jgh - A high-cadence complete shock cooling lightcurve of a SN IIb with the Kepler telescope
• Comprehensive Analyses of the Neutrino-Process in the Core-collapsing Supernova
• Chemical stratification in a long gamma-ray burst cocoon and early-time spectral signatures of supernovae associated with gamma-ray bursts
• Classification of the core-collapse supernova explosion mechanism with learned dictionaries
• Properties of neutrino transfer in a deformed remnant of neutron star merger
• Wave heating from proto-neutron star convection and the core-collapse supernova explosion mechanism
• Impact of electron capture rates on nuclei far from stability on core-collapse supernovae
• Direct anthropic bound on the weak scale from supernovae explosions
• SU(3) Polyakov Linear-Sigma Model With Finite Isospin Asymmetry: QCD Phase Diagram
• NADA-FLD: A General Relativistic, Multi-dimensional Neutrino-hydrodynamics Code Employing Flux-limited Diffusion
• The Temperature and Ionization of Unshocked Ejecta in Cas A
• Dynamics of supernova bounce in laboratory
• 3D evolution of neutron star magnetic-fields from a realistic core-collapse turbulent topology
• Origin of metals in old Milky Way halo stars based on GALAH and Gaia
• The implications of large binding energies of massive stripped core collapse supernova progenitors on the explosion mechanism
• Powering luminous core collapse supernovae with jets
• Spectroscopic observations of progenitor activity 100 days before a Type Ibn supernova
• The 50-100pc scale parent stellar populations of type II supernovae and limitations of single star evolution models
• Recent results in nuclear astrophysics
• Bound-Preserving Discontinuous Galerkin Methods for Conservative Phase Space Advection in Curvilinear Coordinates
• A Black Hole Kicked At Birth: MAXI J1305-704
• Strongly Bipolar Inner Ejecta of the Normal Type IIP Supernova ASASSN-16at
• Core-collapse supernova simulations with reduced nucleosynthesis networks
• A DG-IMEX method for two-moment neutrino transport: Nonlinear solvers for neutrino-matter coupling
• The resonance triplet at E_alpha = 4.5 MeV in the 40Ca(alpha,gamma)44Ti reaction
• Reconstructing Gravitational Wave Core-Collapse Supernova Signals with Dynamic Time Warping
• Neutrino flavor mixing with moments
• Tracer particles for core-collapse supernova nucleosynthesis: The advantages of moving backward
• Nuclear pasta in hot dense matter and its implications for neutrino scattering
• Hadron-Quark Crossover and Hot Neutron Stars at Birth
• Amplifying magnetic fields of a newly born neutron star by stochastic angular momentum accretion in core collapse supernovae
• Long-term gravitational wave asteroseismology of supernova: from core collapse to 20 seconds postbounce
• SN 2020ank: a bright and fast-evolving H-deficient superluminous supernova
• Signatures of Neutrino Cooling in the SN1987A Scenario
• The Galactic Underworld: The spatial distribution of compact remnants
• The 3D shape of Type IIb SN 2011hs
• Introduction to multi-messenger astronomy
• Binary Pulsar J0737-3039: Evidence for a new core collapse and neutron star formation mechanism
• Spectropolarimetry of Type II supernovae (II) Intrinsic supernova polarization and its relations with the photometric/spectroscopic properties
• Measuring the properties of $f-$mode oscillations of a protoneutron star by third generation gravitational-wave detectors
• Characterising the signatures of star-forming galaxies in the extra-galactic $\gamma$-ray background
• X-Ray and Gamma-Ray Emission From Core-collapse Supernovae: Comparison of Three-dimensional Neutrino-driven Explosions With SN 1987A
• Nuclei in Core-Collapse Supernovae Engine
• Prompt directional detection of galactic supernova by combining large liquid scintillator neutrino detectors
• Neutrino transport with Monte Carlo method: I. Towards fully consistent implementation of nucleon recoils in core-collapse supernova simulations
• Signs of Higher Multipoles and Orbital Precession in GW151226
• Combining neutrino experimental light-curves for pointing to the next Galactic Core-Collapse Supernova
• Chiral effective field theory description of neutrino nucleon-nucleon Bremsstrahlung in supernova matter
• Comparison of the Core-Collapse Evolution of Two Nearly Equal Mass Progenitors
• Long-duration Gamma-ray Burst Progenitors and Magnetar Formation
• On the existence of a luminosity threshold of GRB jets in massive stars
• Supernova Neutrino Detection in LZ
• Constraining the final fates of massive stars by oxygen and iron enrichment history in the Galaxy
• SN 2021adxl: A luminous nearby interacting supernova in an extremely low metallicity environment
• Supernova neutrino fluxes in HALO-1kT, Super-Kamiokande, and JUNO
• Exploring Supernova Gravitational Waves with Machine Learning
• Turbulence Fingerprint on Collective Oscillations of Supernova Neutrinos
• Probing the Soft X-ray Properties and Multi-Wavelength Variability of SN2023ixf and its Progenitor
• Supernova Equation of State with an extended SU(3) Quark-Meson Model
• A systematic study of magnetar-powered hydrogen-rich supernovae
• Machine Learning for Conservative-to-Primitive in Relativistic Hydrodynamics
• SN 2023ixf -- an average-energy explosion with circumstellar medium and a precursor
• Magnetorotational Mechanism of the Explosion of Core-Collapse Supernovae
• Synthetic spectra of energetic core-collapse supernovae and the early spectra of SN 2007bi and SN 1999as
• Possible binary neutron star merger history of the primary of GW230529
• Search for gravitational waves emitted from SN 2023ixf
• Gravitational waves and core-collapse supernovae
• Neutrino scattering in supernovae and spin correlations of a unitary gas
• The jittering jets explosion mechanism (JJEM) in electron capture supernovae
• Supernovae Shock Breakout/Emergence Detection Predictions for a Wide-Field X-ray Survey
• Jetted and Turbulent Stellar Deaths: New LVK-Detectable Gravitational Wave Sources
• Knudsen number dependence of 2D single-mode Rayleigh-Taylor fluid instabilities
• Populations of evolved massive binary stars in the Small Magellanic Cloud I: Predictions from detailed evolution models
• Inferring physical properties of stellar collapse by third-generation gravitational-wave detectors
• General-relativistic radiation transport scheme in Gmunu II: Implementation of novel microphysical library for neutrino radiation -- Weakhub
• Finite-temperature linear response theory based on relativistic Hartree Bogoliubov model with point-coupling interaction
• The velocity distribution of outflows driven by choked jets in stellar envelopes
• Modeling of Cosmic-Ray Production and Transport and Estimation of Gamma-Ray and Neutrino Emissions in Starburst Galaxies
• Warm unstable asymmetric nuclear matter: critical properties and the density dependence of the symmetry energy
• Fast neutrino-flavor swap in high-energy astrophysical environments
• A Consistent Modeling of Neutrino-driven Wind with Accretion Flow onto a Protoneutron Star and its Implications for ${}^{56}$Ni Production
• On the importance of progenitor asymmetry to shock revival in core-collapse supernovae
• Towards generating a new supernova equation of state: A systematic analysis of cold hybrid stars
• Deceleration of kicked objects due to the Galactic potential
• On the synthesis of heavy nuclei in protomagnetar outflows and implications for ultra-high energy cosmic rays
• The radio pulsar population of the Small Magellanic Cloud
• Light Curves and Spectra from a Unimodal Core-Collapse SuperNova
• Collective Oscillations of Majorana Neutrinos in Strong Magnetic Fields and Self-induced Flavor Equilibrium
• Tracking the footprints of the radio pulsar B1727$-$47: proper motion, host supernova remnant, and the glitches
• Neutron stars formation and Core Collapse Supernovae
• Spectropolarimetry of the Type IIb SN 2008aq
• Self consistent calculation of the nuclear composition in hot and dense stellar matter
• Effects of nuclear matter and composition in core-collapse supernovae and long-term proto-neutron star cooling
• Mechanical feedback from black hole accretion as an energy source of core-collapse supernova explosions
• Properties and applications of a predicted population of runaway He-sdO/B stars ejected from single degenerate He-donor SNe
• Gravitational instability caused by the weight of heat
• Long-duration transient, gravitational-wave search pipeline
• Hybrid method to resolve the neutrino mass hierarchy by supernova (anti)neutrino induced reactions
• Prospects for Distinguishing Supernova Models Using a Future Neutrino Signal
• Open issues in neutrino astrophysics
• Hadronic Interactions of Energetic Charged Particles in Protogalactic Outflow Environments and Implications for the Early Evolution of Galaxies
• Constraining neutrino-DM interactions with Milky Way dwarf spheroidals and supernova neutrinos
• Hydrodynamic Shock Wave Studies within a Kinetic Monte Carlo Approach
• Anisotropic neutrinos and gravitational waves from black hole neutrino-dominated accretion flows in fallback core-collapse supernovae
• Filamentary Ejecta Network in Cassiopeia~A Reveals Fingerprints of the Supernova Explosion Mechanism
• Stability of stagnation via an expanding accretion shock wave
• Modified Urca neutrino emissivity at finite temperature
• Visualizing convolutional neural network for classifying gravitational waves from core-collapse supernovae
• Parameterisations of thermal bomb explosions for core-collapse supernovae and 56Ni production
• Reducing cosmological small scale structure via a large dark matter-neutrino interaction: constraints and consequences
• Magnetorotational neutron star kicks
• The Gravothermal Instability at all scales: from Turnaround Radius to Supernovae
• Equation of State of Neutron-Rich Matter in $d$-Dimensions
• Neutrinos, supernovae, and the origin of the heavy elements
• Comparison of simulated neutrino emission models with data on Supernova 1987A
• Parametric initial conditions for core-collapse supernova simulations
• Discovery of Stable Titanium at the Northeastern Jet of Cassiopeia A: Need for a Weak Jet Mechanism?
• Compact Objects in close orbits as Gravitational Wave Sources: Formation Scenarios and Properties
• Probe and Prejudice: Classification of compact objects and model comparison using EOS knowledge
• Shock Revival in Core-Collapse Supernovae: A Phase-Diagram Analysis
• Galactic Population Synthesis of Radioactive Nucleosynthesis Ejecta
• Computational Techniques for Parameter Estimation of Gravitational Wave Signals
• Flavor Equilibration of Supernova Neutrinos: Exploring the Dynamics of Slow Modes
• Compact Object Formation and the Supernova Explosion Engine
• Light Curves of Type IIP Supernovae from Neutrino-driven Explosions of Red Supergiants Obtained by a Semi-analytic Approach
• Accretion-Induced Collapse of Dark Matter Admixed White Dwarfs -- II: Rotation and Gravitational-wave Signals
• Spatial distribution of radionuclides in 3D models of SN 1987A and Cas A
• Chaos in Inhomogeneous Neutrino Fast Flavor Instability
• Element formation in radiation-hydrodynamics simulations of kilonovae
• Diverse, massive-star-associated sources for elements heavier than Fe and the roles of neutrinos
• The effects of rotation, metallicity and magnetic field on the islands of failed supernovae
• Impact of Rotation on the Multimessenger Signatures of a Hadron-quark Phase Transition in Core-collapse Supernovae
• Supernova Neutrinos: flavour conversion mechanisms and new physics scenarios
• Constraining the supersaturation density equation of state from core-collapse supernova simulations - Excluded volume extension of the baryons
• PTF11rka: an interacting supernova at the crossroads of stripped-envelope and H-poor super-luminous stellar core collapses
• Impact of rotation on the evolution of convective vortices in collapsing stars
• Statistical tests of young radio pulsars with/without supernova remnants: implying two origins of neutron stars
• The Force Explosion Condition is Consistent with Spherically Symmetric CCSN Explosions
• Neutrino-driven massive stellar explosions in 3D fostered by magnetic fields via turbulent $\alpha$-effect
• Dynamical trapping and relaxation of scalar gravitational fields
• Searching for ejected supernova companions in the era of precise proper motion and radial velocity measurements
• In-flight positron annihilation as a probe of feebly interacting particles
• X-ray Studies of the Inverted Ejecta Layers in the Southeast Area of Cassiopeia A
• The odd-isotope fractions of Barium in CEMP-r/s star HE 0338-3945 and r-II star CS 31082-001
• Solving the gamma-ray radiative transfer equation for supernovae
• Observing the earliest moments of supernovae using strong gravitational lenses
• Phase-transition-induced collapse of proto-compact stars and its implication for supernova explosions
• Nuclear pasta in hot and dense matter and its influence on the equation of state for astrophysical simulations
• The Formation of Electron-capture Supernovae: A Review
• Progenitor Dependence of Neutrino-driven Supernova Explosions with the Aid of Heavy Axion-like Particles
• Creation of electron-positron pairs at excited Landau levels by neutrino in a strong magnetic field
• SN 2020zbf: A fast-rising hydrogen-poor superluminous supernova with strong carbon lines
• The Core-Collapse Supernova Explosion Mechanism
• Thermal Regulation and the Star-Forming Main Sequence
• Uncertainty Quantification for Neutrino Opacities in Core-Collapse Supernovae and Neutron Star Mergers
• Impact of rotation on stellar models
• Linear response theory in asymmetric nuclear matter for Skyrme functionals including spin-orbit and tensor terms II: Charge Exchange
• Equation of state in neutron stars and supernovae
• Three-dimensional radiation hydrodynamics simulations of wandering intermediate-mass black holes considering the anisotropic radiation and dust sublimation
• Prospects for reconstructing the gravitational-wave signals from core-collapse supernovae with Advanced LIGO-Virgo and the BayesWave algorithm
• Equilibrium nuclear ensembles taking into account vaporization of hot nuclei in dense stellar matter
• Axion-photon conversion in transient compact stars: Systematics, constraints, and opportunities
• What can be learned from a proto-neutron star's mass and radius?
• Hyperons and $\Delta$'s in rotating protoneutron stars: Global properties
• Supernova Preshock Neutronization Burst as a Probe of Non-Standard Neutrino Interactions
• Diagnosing The Ejecta Properties of Engine-Driven Supernovae from Observables in Their Initial Phase
• Hidden shock powering the peak of SN 2020faa
• Astrophysics with the Laser Interferometer Space Antenna
• A two-phase model of galaxy formation: III. The formation of globular clusters
• Non-conservation of Lepton Numbers in the Neutrino Sector Could Change the Prospects for Core Collapse Supernova Explosions
• Cooling the Shock: New Supernova Constraints on Dark Photons
• Detecting and reconstructing gravitational waves from the next Galactic core-collapse supernova in the Advanced Detector Era
• Nuclear pasta structures at high temperatures
• An Exploration of X-ray Supernova Remnants in the Milky Way and Nearby Galaxies
• Many-Body Simulations of the Fast Flavor Instability
• On the mass-function of GWTC-2 binary black hole systems and their progenitors
• Proof of the Classical Soft Graviton Theorem in D=4
• Deep Learning of the Eddington Tensor in the Core-collapse Supernova Simulation
• Response of nuclear-dissociating shocks to vorticity perturbations
• Theoretical developments in supernova neutrino physics : mass corrections and pairing correlators
• The Red Supergiant Progenitor of the Type II Supernova 2024abfl
• Fast and Not-so-Furious: Case Study of the Fast and Faint Type IIb SN 2021bxu
• Parameter estimation of protoneutron stars from gravitational wave signals using the Hilbert-Huang transform
• Abundance Pattern Fitting with Bayesian Inference: Constraining First Stars' Properties and Their Explosion Mechanism with Extremely Metal-poor Stars
• Exploring GRBs and supernovae connection: does a superluminous hypernova population exist?
• Skyrme-RPA study of charged-current neutrino opacity in hot and dense supernova matter
• Explosive Nucleosynthesis: What we learned and what we still do not understand
• A Chandra X-ray Study of Supernova Remnant N63A in the Large Magellanic Cloud
• Neutrino induced reactions in core-collapse supernovae: effects on the electron fraction
• Influence of the effective mass on the properties of nuclear matter at finite density and temperature
• Equation of state and neutrino transfer in supernovae and neutron stars
• Nucleon Short-Range Correlations and High-Momentum Dynamics: Implications on the Equation of State of Dense Matter
• Estimate of the Detectability of the Circular Polarisation Signature of Supernova Gravitational Waves Using the Stokes Parameters
• Neutrino flavour as a test of the explosion mechanism of core-collapse supernovae
• Stellar evolution, SN explosion, and nucleosynthesis
• Investigating starburst-driven neutrino emission from galaxies in the Great Observatories All-Sky LIRG Survey
• A mixed helium-oxygen shell in some core-collapse supernova progenitors
• Simple fits for the neutrino luminosities from protoneutron star cooling
• Determining the minimal mass of a proto-neutron star with chirally constrained nuclear equations of state
• Strongly interacting matter in extreme magnetic fields
• Termination of the MRI via parasitic instabilities in core-collapse supernovae: influence of numerical methods
• Detecting Supernova Axions with IAXO
• An axisymmetric shock breakout indicated by prompt polarized emission from the type II supernova 2024ggi
• The Milky Way satellite galaxy Leo T: A perturbed cored dwarf
• Neutrino astrophysics : recent advances and open issues
• Post-explosion positive jet-feedback activity in inner ejecta of core collapse supernovae
• Massive Computation for Understanding Core-Collapse Supernova Explosions
• Anisotropic neutrino effect on magnetar spin: constraint on inner toroidal field
• Dark Matter Balls Help Supernovae to Explode
• Porting Large HPC Applications to GPU Clusters: The Codes GENE and VERTEX
• Chiral transport of neutrinos in supernovae
• Mass Distribution and "Mass Gap" of Compact Stellar Remnants in Binary Systems
• The spectra of a radiative reprocessing outflow model for fast blue optical transients
• Waveform Reconstruction of Core-Collapse Supernova Gravitational Waves with Improved Multisynchrosqueezing Transform
• Electron-neutrino lepton number crossings: Variations with the supernova core physics
• Constraints on Explosion Timescale of Core-Collapse Supernovae Based on Systematic Analysis of Light Curves
• The rotational shear in pre-collapse cores of massive stars
• Neutrino-pair bremsstrahlung from nucleon-$\alpha$ versus nucleon-nucleon scattering
• The $\gamma$-ray deposition histories of Calcium-rich supernovae
• Surprises from the spins: astrophysics and relativity with detections of spinning black-hole mergers
• Stellar energy loss rates in the pair-annihilation process beyond the standard model
• Preliminary EoS for core-collapse supernova simulations with the QMC model
• The Corona-Australis star-forming region: New insights on its formation history from detailed stellar and disk analysis
• Three-flavor, Full Momentum Space Neutrino Spin Oscillations in Neutron Star Mergers
• Core-Collapse Supernovae: From Neutrino-Driven 1D Explosions to Light Curves and Spectra
• Buoyancy instability of homologous implosions
• Star Formation for Predictive Primordial Galaxy Formation
• SN 2022ngb: A faint, slowly evolving Type IIb supernova with a low-mass envelope
• Two-beam Multiparticle Many-body simulations of Inhomogeneous FFI
• Light Neutral Clusters in Supernova Matter
• Gravitational waves from magnetorotational core-collapse supernovae using 3D GRMHD simulations: effect of rotation and magnetic fields
• Properties and microscopic structures of dense stellar matter in RMF models
• Dynamical ejecta of neutron star mergers with nucleonic weak processes I: Nucleosynthesis
• Supernova explosions of runaway stars and young neutron stars above the Galactic plane
• Spin Flavor Spectral Splits of Supernova Neutrino Flavor Conversions
• On the character of turbulence in self-consistent models of core-collapse supernovae
• Neutrino-Neutron Scattering Opacities in Supernova Matter
• In-Stabilities of massive white dwarfs in modified gravity
• Timing coincidence search for supernova neutrinos with optical transient surveys
• Uncovering the neutrino mass ordering with the next galactic core-collapse supernova neutrino burst using water Cherenkov detectors
• Hypothesis about Enrichment of Solar System
• Non-Standard Neutrino Self-Interactions Can Cause Neutrino Flavor Equipartition Inside the Supernova Core
• Bridging the Gap: From Massive Stars to Supernovae
• Rapid decline in the lightcurves of luminous supernovae by jet-driven bipolar explosions
• GenASiS: General Astrophysical Simulation System. II. Nonrelativistic Hydrodynamics
• Kinetic Simulations of Rayleigh-Taylor Instabilities
• Accelerating Our Understanding of Supernova Explosion Mechanism via Simulations and Visualizations with GenASiS
• A Brief History of the Co-evolution of Supernova Theory with Neutrino Physics
• Neutrinos from Diffuse Supernova Background
• Matter- and magnetically-driven flavor conversion of neutrinos in magnetorotational collapses
• Equation of State in a Generalized Relativistic Density Functional Approach
• Neutrino transport with Monte Carlo method: II. Quantum Kinetic Equations
• Neutrino mixing in nuclear rapid neutron-capture processes
• A comprehensive search for high-velocity X-ray sources: New compact object binary candidates in the Gaia era
• Parametric instability in scalar gravitational fields
• Sensitivity Study of Supernova Neutrinos for Mass Hierarchy
• The Radio Remnant of Supernova 1987A - A Broader View
• Multimessenger Analysis Strategy for Core-Collapse Supernova Search: Gravitational Waves and Low-energy Neutrinos
• Th/Eu abundance ratio of red giants in the Kepler Field
• Discrete Self Similarity in Filled Type I Strong Explosions
• On Neutron Star Natal Kicks in High-Mass X-Ray Binaries: Insights from Population Synthesis
• Quasi-classical Gravity effect on neutrino oscillations in a gravitational field of an heavy astrophysical object
• The influence of rotation and metallicity on the explodability of massive stars
• Emission of neutrino-antineutrino pairs by hadronic bremsstrahlung processes
• New Skyrme parametrizations to describe finite nuclei and neutron star matter with realistic effective masses. II. Adjusting the spin-dependent terms
• Convection signatures in early-time gravitational waves from core-collapse supernovae
• Effects of Nontrivial Topology on Neutron Star Rotation and its Potential Observational Implications
• The Dark Photon: a 2026 Perspective
• Revisiting black hole hyperaccretion in the center of gamma-ray bursts for the lower mass gap
• Equilibrium constants of nuclear reactions in supernova explosions
• Observational signatures of stellar explosions driven by relativistic jets
• Constraining the Time of Gravitational Wave Emission from Core-Collapse Supernovae
• Three-dimensional equation of state extension of quark matter in Fermi-liquid theory
• Effects of spacetime geometry on neutrino oscillation inside a Core-Collapse Supernova
• Convective stability analysis of massive neutron stars formed in binary mergers
• Joint Analysis Method on Gravitational Waves and Low-Energy Neutrinos to Detect Core-Collapse Supernovae
• P-stars in the gravitational wave era
• Supernova Detection at SNOLAB
• From supernovae to neutron stars: crust formation time
• Forming Double Neutron Stars using Detailed Binary Evolution Models with POSYDON: Comparison to the Galactic Systems
• Constraining the gravitational-wave emission of core-collapse supernovae with ground-based detectors
• Residual neural networks to classify the high frequency emission in core-collapse supernova gravitational waves
• Quasi-Elastic Neutrino Reactions on Carbon and Lead Nuclei
• EDGE-INFERNO: How chemical enrichment assumptions impact the individual stars of a simulated ultra-faint dwarf galaxy
• Numerical modeling of core-collapse supernovae and compact objects
• The e-ASTROGAM space mission: a major step forward for supernova physics
• Using CSST and ejecta-wind interaction in type II-P supernovae to constrain the wind-mass loss of red supergiant stars
• Multimessenger Constraints on the Central Engine in SN 2023ixf: Neutron Star or Black Hole?
• Constraining the Pulsar 3D Velocity Distribution: The Impact of Spin-Velocity Alignment
• Stellar Instability from Parametric Resonance
• Gravitational wave interactions with a viscous fluid: Core collapse supernova, binary neutron star merger, and accretion around a black hole merger
• Impact of tides on non-coplanar orbits of progenitors of high-mass X-ray binaries
• Signatures of electromagnetic and sound radiation produced by gravitational waves in core-collapse supernovae
• The Strange Physics of Dark Baryons
• Stochastic Gravitational-Wave Background from Stellar Core-Collapse Events
• Hydrogen-rich supernovae beyond the neutrino-driven core-collapse paradigm
• Phenomenological QCD equations of state for neutron star mergers, a talk presented at CPOD17