Black Hole Formation in Failing Core-Collapse Supernovae
arXiv:1010.5550 · doi:10.1088/0004-637X/730/2/70
Abstract
We present results of a systematic study of failing core-collapse supernovae and the formation of stellar-mass black holes (BHs). Using our open-source general-relativistic 1.5D code GR1D equipped with a three-species neutrino leakage/heating scheme and over 100 presupernova models, we study the effects of the choice of nuclear equation of state (EOS), zero-age main sequence (ZAMS) mass and metallicity, rotation, and mass-loss prescription on BH formation. We find that the outcome, for a given EOS, can be estimated, to first order, by a single parameter, the compactness of the stellar core at bounce. By comparing protoneutron star (PNS) structure at the onset of gravitational instability with solutions of the Tolman-Oppenheimer-Volkof equations, we find that thermal pressure support in the outer PNS core is responsible for raising the maximum PNS mass by up to 25% above the cold NS value. By artificially increasing neutrino heating, we find the critical neutrino heating efficiency required for exploding a given progenitor structure and connect these findings with ZAMS conditions, establishing, albeit approximately, for the first time based on actual collapse simulations, the mapping between ZAMS parameters and the outcome of core collapse. We also study the effect of progenitor rotation and find that the dimensionless spin of nascent BHs may be robustly limited below a^* = Jc/GM^2 = 1 by the appearance of nonaxisymmetric rotational instabilities.
20 emulateapj pages, 13 figures, published in the Astrophysical Journal, minor revisions
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- The Vanishing & Appearing Sources during a Century of Observations project: I. USNO objects missing in modern sky surveys and follow-up observations of a "missing star"
- Effect of the Nuclear Equation of State on Relativistic-Turbulence Induced Core-Collapse Supernovae
- Dropping Anchor: Understanding the Populations of Binary Black Holes with Random and Aligned Spin Orientations
- On the effects of the Initial Mass Function on Galactic chemical enrichment
- General Relativistic Neutrino-Driven Turbulence in One-Dimensional Core-Collapse Supernovae
- The Status and Future of Direct Nuclear Reaction Measurements for Stellar Burning
- The initial mass-final luminosity relation of type II supernova progenitors. Hints of new physics?
- The Progenitor Age and Mass of the Black-Hole-Formation Candidate N6946-BH1
- Explodability criteria for the neutrino-driven supernova mechanism
- Role of supergiants in the formation of globular clusters
- Equation of state and composition of proto-neutron stars and merger remnants with hyperons
- Forming merging double compact objects with stable mass transfer
- The impact of vorticity waves on the shock dynamics in core-collapse supernovae
- The magneto-rotational instability in massive stars
- Progenitor Dependence of Hadron-quark Phase Transition in Failing Core-collapse Supernovae
- Phase transition towards strange matter
- The effect of mass loss in models of red supergiants in the Small Magellanic Cloud
- Mass-transferring binary stars as progenitors of interacting hydrogen-free supernovae
- Monte Carlo population synthesis on massive star binaries: Astrophysical implications for gravitational wave sources
- Supernovae from massive stars
- Properties of High-Redshift GRBs
- Numerical studies on core collapse supernova in self-interacting massive scalar-tensor gravity
- Realistic 3D hydrodynamics simulations find significant turbulent entrainment in massive stars
- Monotonicity of the cores of massive stars
- Gravitational Wave Signatures of Hyperaccreting Collapsar Disks
- Post-explosion evolution of core-collapse supernovae
- Carbon monoxide formation and cooling in supernovae
- Potential signature of Population III pair-instability supernova ejecta in the BLR gas of the most distant quasar at z = 7.54
- Astrophysical explosions revisited: collisionless coupling of debris to magnetized plasma
- Remnant masses from 1D+ core-collapse supernovae simulations: bimodal neutron star mass distribution and black holes in the low-mass gap
- Direct anthropic bound on the weak scale from supernovae explosions
- Dynamics of supernova bounce in laboratory
- Intermediate Luminosity Red Transients by Black Holes Born from Erupting Massive Stars
- Helium giant stars as progenitors of rapidly fading Type Ibc supernovae
- A systematic study of super-Eddington layers in the envelopes of massive stars
- Black Hole Accretion Disk Diffuse Neutrino Background
- Explodability fluctuations of massive stellar cores enable asymmetric compact object mergers such as GW190814
- An Exceptional Dimming Event for a Massive, Cool Supergiant in M51
- The Cosmic MeV Neutrino Background as a Laboratory for Black Hole Formation
- Effective Helium Burning Rates and the Production of the Neutrino Nuclei
- A population of Type Ibc supernovae with massive progenitors; broad lightcurves not uncommon in (i)PTF
- General relativistic neutrino transport using spectral methods
- Estimating the core compactness of massive stars with Galactic supernova neutrinos
- Probing the metastability of protoneutron star with hyperon in core-collapse supernova
- Stability of the protoneutron stars toward black hole formation
- Dissecting the microphysics behind the metallicity-dependence of massive stars radii
- Long-duration Gamma-ray Burst Progenitors and Magnetar Formation
- On the existence of a luminosity threshold of GRB jets in massive stars
- Comparison of the Core-Collapse Evolution of Two Nearly Equal Mass Progenitors
- Pre-Supernova Alert System for Super-Kamiokande
- Constraints on the Galactic Centre environment from Gaia hypervelocity stars II: The evolved population
- Reducing Uncertainties in the Production of the Gamma Emitting Nuclei 26Al, 44Ti, and 60Fe in Core Collapse Supernovae by Using Effective Helium Burning Rates
- Exploring Supernova Gravitational Waves with Machine Learning
- Density Profiles of Collapsed Rotating Massive Stars Favor Long Gamma-Ray Bursts
- Diffuse neutrino background from past core-collapse supernovae
- Enhanced low-energy supernova burst detection in large liquid argon time projection chambers enabled by Q-Pix
- Type IIP Supernova Progenitors and their explodability I: Convective Overshoot, Blue Loops and Surface Composition
- Neutrinos from explosive transients at the dawn of multi-messenger astronomy
- Dust Formation By Failed Supernovae
- Constraining the final fates of massive stars by oxygen and iron enrichment history in the Galaxy
- Possible binary neutron star merger history of the primary of GW230529
- Populations of evolved massive binary stars in the Small Magellanic Cloud I: Predictions from detailed evolution models
- Evolution and Nucleosynthesis of Very Massive Stars
- Impact of late-time neutrino emission on the diffuse supernova neutrino background
- The evolutions of the innermost stable circular orbits in dynamical spacetimes
- A metallicity dependence on the occurrence of core-collapse supernovae
- The non-linear onset of neutrino-driven convection in two and three-dimensional core-collapse supernovae
- Rotation and Magnetism of Massive Stellar Cores
- Non-thermal neutrinos created by shock acceleration in successful and failed core-collapse supernova
- Revealing local failed supernovae with neutrino telescopes
- Hot and dense matter beyond relativistic mean field theory
- Memory-triggered supernova neutrino detection
- Neutron stars formation and Core Collapse Supernovae
- Collective neutrino oscillations and detectabilities in failed supernovae
- Exploring the Fate of Stellar Core Collapse with Supernova Relic Neutrinos
- Mechanical feedback from black hole accretion as an energy source of core-collapse supernova explosions
- Simulations of the progenitors of black hole-neutron star gravitational wave sources
- Connecting stellar and galactic scales: Energetic feedback from stellar wind bubbles to supernova remnants
- Compactness peaks: An astrophysical interpretation of the mass distribution of merging binary black holes
- How many explosions does one need? -- Quantifying supernovae in globular clusters from iron abundance spreads
- Neutrino Echos following Black Hole Formation in Core-Collapse Supernovae
- A Force Explosion Condition for Spherically Symmetric Core-collapse Supernovae
- The Search for Failed Supernovae with the Large Binocular Telescope: N6946-BH1, Still No Star
- Black Hole Supernovae, their Equation of State Dependence and Ejecta Composition
- From Galactic Chemical Evolution to Cosmic Supernova Rates Synchronized with Core-Collapse Supernovae Limited to the Narrow Progenitor Mass Range
- Parameterisations of thermal bomb explosions for core-collapse supernovae and 56Ni production
- Diffuse supernova neutrino background with up-to-date star formation rate measurements and long-term multidimensional supernova simulations
- The Explosion Mechanism of Core-Collapse Supernovae and Its Observational Signatures
- Gravitational Waves from Newborn Accreting Millisecond Magnetars
- Constraining the onset density for the QCD phase transition with the neutrino signal from core-collapse supernovae
- Radio Transients from Newborn Black Holes
- On the distribution of stellar-sized black hole spins
- Parametric initial conditions for core-collapse supernova simulations
- A deep near-infrared spectroscopic survey of the Scutum-Crux arm for Wolf-Rayet stars
- Constraining the supersaturation density equation of state from core-collapse supernova simulations - Excluded volume extension of the baryons
- Neutrino-driven Core-collapse Supernova Yields in Galactic Chemical Evolution
- Numerical relativity simulations of black hole and relativistic jet formation
- Light Curves of Type IIP Supernovae from Neutrino-driven Explosions of Red Supergiants Obtained by a Semi-analytic Approach
- No evidence for a dip in the binary black hole mass spectrum
- The Force Explosion Condition is Consistent with Spherically Symmetric CCSN Explosions
- The effects of rotation, metallicity and magnetic field on the islands of failed supernovae
- Outflow-Driven Transients from the Birth of Binary Black Holes I: Tidally-Locked Secondary Supernovae
- Supernovae from stellar mergers and accretors of binary mass transfer: Implications for Type IIP, 1987A-like and interacting supernovae
- Nebular C IV 1550 Imaging of the Metal-Poor Starburst Mrk 71: Direct Evidence of Catastrophic Cooling
- The Progenitor of the Vela Pulsar
- The Origin of the Possible Massive Black Hole in the Progenitor System of iPTF13bvn
- An excision scheme for black holes in constrained evolution formulations: spherically symmetric case
- Progenitors of Long-Duration Gamma-ray Bursts
- Progenitor Dependence of Neutrino-driven Supernova Explosions with the Aid of Heavy Axion-like Particles
- Hyperons during proto-neutron star deleptonization and the emission of dark flavoured particles
- Equation of state in neutron stars and supernovae
- Progenitor constraint with circumstellar material for the magnetar-hosting supernova remnant RCW 103
- The fate of rotating massive stars across cosmic times
- The initial mass-remnant mass relation for core collapse supernovae
- Weak Shock Propagation with Accretion. III. A Numerical Study On Shock Propagation & Stability
- Quantum Black Hole Seismology II: Applications to Astrophysical Black Holes
- Gravitational wave signals in the deci-Hz range from neutrinos during the proto-neutron star cooling phase
- Evolution of the surface magnetic field of rotating proto-neutron stars
- Evaluating Machine Learning Models for Supernova Gravitational Wave Signal Classification
- A Modified Initial Mass Function of the First Stars with Explodability Theory under Different Enrichment Scenarios
- The Antesonic Condition for the Explosion of Core-Collapse Supernovae II: Rotation and Turbulence
- Detecting and reconstructing gravitational waves from the next Galactic core-collapse supernova in the Advanced Detector Era
- Sensitivity of multi-PMT Optical Modules in Antarctic Ice to Supernova Neutrinos of MeV energy
- Neutron Stars: Laboratories for fundamental physics under extreme astrophysical conditions
- Variety of disk wind-driven explosions in massive rotating stars
- Failed Supernova Remnants
- Transition Elements in Supernova Presolar Grains: Condensation vs. Implantation
- Disappearance of a massive star in the Andromeda Galaxy due to formation of a black hole
- Comparison of Electron Capture Rates in the N=50 Region using 1D Simulations of Core-collapse Supernovae
- Abundance Pattern Fitting with Bayesian Inference: Constraining First Stars' Properties and Their Explosion Mechanism with Extremely Metal-poor Stars
- Stochastic Gravitational Wave Background from PBH-ABH Mergers
- Enforcing causality in nonrelativistic equations of state at finite temperature
- Upper Limit on Star Formation and Metal Enrichment in Minihalos
- Triangulating Black Hole Forming Stellar Collapses through Neutrinos
- The impact of wind mass loss on nucleosynthesis and yields of very massive stars at low metallicity
- Estimate of the Detectability of the Circular Polarisation Signature of Supernova Gravitational Waves Using the Stokes Parameters
- Wolf-Rayet -- compact object binaries as progenitors of binary compact objects
- Formation of millisecond pulsar-helium star binaries
- Optical ultra-stable optical clock cavities as resonant mass gravitational wave detectors in search for new physics
- Neutrino flavour as a test of the explosion mechanism of core-collapse supernovae
- Scalar Gravitational Wave Signals from Core Collapse in Massive Scalar-Tensor Gravity with Triple-Scalar Interactions
- The structure and evolution of a high-mass stellar merger in the Hertzsprung gap
- The demographics of core-collapse supernovae. The role of binary evolution and CSM interaction
- Evolving massive stars to core collapse with GENEC: Extension of equation of state, opacities and effective nuclear network
- Strong Variability in AzV 493, an Extreme Oe-Type Star in the SMC
- Neutrino signals from Neutron Star implosions to Black Holes
- Constraints on Explosion Timescale of Core-Collapse Supernovae Based on Systematic Analysis of Light Curves
- The Type II-P Supernova 2019mhm and Constraints on Its Progenitor System
- Dependence of the Sr-to-Ba and Sr-to-Eu Ratio on the Nuclear Equation of State in Metal Poor Halo Stars
- Multimessenger signatures of a deformed magnetar in gamma-ray bursts
- Spherically Symmetric Accretion onto a Compact Object through a Standing Shock: The Effects of General Relativity in the Schwarzschild Geometry
- Fast Transients from Magnetic Disks Around Non-Spinning Collapsar Black Holes
- Production of heavy -elements and Ti in Cas A: comparison to abundances from 1D core-collapse supernova models and evidence for Carbon-Oxygen shell mergers
- New {\em ab initio} constrained extended Skyrme equations of state for simulations of neutron stars, supernovae and binary mergers: I. Subsaturation density domain
- Gravitational waves from magnetorotational core-collapse supernovae using 3D GRMHD simulations: effect of rotation and magnetic fields
- A Parametric Study of the SASI Comparing General Relativistic and Nonrelativistic Treatments
- Ultra-compact X-ray Binaries: A Review
- The influence of rotation and metallicity on the explodability of massive stars
- Circini: A massive hierarchical triple system with an eclipsing binary
- Neutrinos from Diffuse Supernova Background
- Power-law Emission-line Wings and Radiation-Driven Superwinds in Local Lyman Continuum Emitters
- Occurrence of fast neutrino flavor conversions in QCD phase-transition supernovae
- Multimessenger Analysis Strategy for Core-Collapse Supernova Search: Gravitational Waves and Low-energy Neutrinos
- An apparent positive relation between spin and orbital angular momentum in X-ray binaries
- New ab initio constrained extended Skyrme equations of state for simulations of neutron stars, supernovae and binary mergers: II. Thermal response in the suprasaturation density domain
- Numerical Simulations of the Random Angular Momentum in Convection: Implications for Supergiant Collapse to Form Black Holes
- Convection signatures in early-time gravitational waves from core-collapse supernovae
- Modeling the outcome of supernova explosions in binary population synthesis using the stellar compactness
- 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
- GenASiS: General Astrophysical Simulation System. II. Self-gravitating Baryonic Matter
- The Impact of the New Fe Decay Rates on Fe and Al Nucleosynthesis in Massive Stars
- Formation of black holes from He stars
- Progenitors of Core-Collapse Supernovae
- The Supernova Remnant G284.31.8 and Its Relation to the Gamma-ray Binary 1FGL J1018.65856
- Massive stars evolution: feedbacks in low-Z environment
- Progenitor and Close-In Circumstellar Medium of Type II Supernova 2020fqv from High-Cadence Photometry and Ultra-Rapid UV Spectroscopy
- Multimessenger Signatures of Tilted, Self-Gravitating, Black Hole Disks
- Photons from neutrinos: the gamma ray echo of a supernova neutrino burst
- A Black Hole is Born: 3D GRMHD Simulation of Black Hole Formation from Core-Collapse