Magnetorotational core collapse of possible GRB progenitors. II. Formation of protomagnetars and collapsars

Abstract

We assess the variance of the post-collapse evolution remnants of compact, massive, low-metallicity stars, under small changes in the degrees of rotation and magnetic field of selected pre-supernova cores. These stellar models are commonly considered progenitors of long gamma-ray bursts. The fate of the proto-neutron star (PNS) formed after collapse, whose mass may continuously grow due to accretion, critically depends on the poloidal magnetic field strength at bounce. Should the poloidal magnetic field be sufficiently weak, the PNS collapses to a black hole (BH) within a few seconds. Models on this evolutionary track contain promising collapsar engines. Poloidal magnetic fields smooth over large radial scales (e.g. dipolar fields) or slightly augmented with respect to the original pre-supernova core yield long-lasting PNSs. In these models, BH formation is avoided or staved off for a long time, hence, they may produce proto-magnetars (PMs). Some of our PM candidates have been run for $\lesssim 10$s after core bounce, but they have not entered the Kelvin-Helmholtz phase yet. Among these models, some display episodic events of spin-down during which we find properties broadly compatible with the theoretical expectations for PMs ($M_{PNS}\approx 1.85M_{\odot }-2.5M_{\odot }$, ${\bar{P}}_{PNS}\approx 1.5-4$ms, and $b_{PNS}^{\mathrm{surf}}\lesssim 10^{15}$G) and their very collimated supernova ejecta has nearly reached the stellar surface with (still growing) explosion energies $\gtrsim 2\times 10^{51}$erg.

arXiv comment33 pages, 23 figures, accepted by MNRAS

References in corpus (124)

• Collapsars - Gamma-Ray Bursts and Explosions in "Failed Supernovae"
• Grids of stellar models with rotation - I. Models from 0.8 to 120 Msun at solar metallicity (Z = 0.014)
• Neutron Star Structure and the Equation of State
• Masses, Radii, and Equation of State of Neutron Stars
• Explosion Mechanisms of Core-Collapse Supernovae
• Core-Collapse Supernovae from 9 to 120 Solar Masses Based on Neutrino-powered Explosions
• Presupernova Evolution of Rotating Massive Stars I: Numerical Method and Evolution of the Internal Stellar Structure
• Dynamo action by differential rotation in a stably stratified stellar interior
• The Progenitor Stars of Gamma-Ray Bursts
• The Physics of Gamma-Ray Bursts and Relativistic Jets
• Presupernova Evolution of Differentially Rotating Massive Stars Including Magnetic Fields
• Supernovae, Jets, and Collapsars
• Black Hole Formation in Failing Core-Collapse Supernovae
• Gamma-ray Burst Afterglow with Continuous Energy Injection: Signature of a Highly-Magnetized Millisecond Pulsar
• Nucleosynthesis in neutrino-driven winds: I. The physical conditions
• The Proto-Magnetar Model for Gamma-Ray Bursts
• Evolution of rapidly rotating metal-poor massive stars towards gamma-ray bursts
• Evolution of Protoneutron Stars
• Magnetorotationally driven Supernovae as the origin of early galaxy $r$-process elements?
• Single star progenitors of long gamma-ray bursts I: Model grids and redshift dependent GRB rate
• Progenitor-Explosion Connection and Remnant Birth Masses for Neutrino-Driven Supernovae of Iron-Core Progenitors
• Simulations of Magnetically-Driven Supernova and Hypernova Explosions in the Context of Rapid Rotation
• Relativistic Jets in Collapsars
• The Magnetorotational Instability in Core Collapse Supernova Explosions
• Neutrino Signal of Electron-Capture Supernovae from Core Collapse to Cooling
• Constraining the Equation of State with Moment of Inertia Measurements
• Magnetar Spindown, Hyper-Energetic Supernovae, and Gamma Ray Bursts
• Asymmetric Supernovae, Pulsars, Magnetars, and Gamma-Ray Bursts
• Peering into the dark side: magnesium lines establish a massive neutron star in PSR J2215+5135
• Relativistic Jets from Collapsars
• A large scale dynamo and magnetoturbulence in rapidly rotating core-collapse supernovae
• A new population of ultra-long duration gamma-ray bursts
• Evidence for a Massive Neutron Star from a Radial-Velocity Study of the Companion to the Black Widow Pulsar PSR B1957+20
• Magnetorotational Core-Collapse Supernovae in Three Dimensions
• Core-Collapse Simulations of Rotating Stars
• Exploring the relativistic regime with Newtonian hydrodynamics: An improved effective gravitational potential for supernova simulations
• The Diversity of Transients from Magnetar Birth
• The Propagation and Eruption of Relativistic Jets from the Stellar Progenitors of GRBs
• Gamma-ray burst early afterglows: reverse shock emission from an arbitrarily magnetized ejecta
• Short GRBs with Extended Emission from Magnetar Birth: Jet Formation and Collimation
• Gravitational waves from instabilities in relativistic stars
• Relativistic MHD simulations of core-collapse GRB jets: 3D instabilities and magnetic dissipation
• Temporal and Angular Properties of GRB Jets Emerging from Massive Stars
• Viscosity and Rotation in Core-Collapse Supernovae
• The ultra-long Gamma-Ray Burst 111209A: the collapse of a blue supergiant?
• The Spin Periods and Rotational Profiles of Neutron Stars at Birth
• SN 2004aw: Confirming Diversity of Type Ic Supernovae
• 3-Dimensional Core-Collapse
• The Development of Explosions in Axisymmetric Ab Initio Core-Collapse Supernova Simulations of 12-25 $M_{\odot }$ Stars
• The Explosion of Helium Stars Evolved With Mass Loss
• Semi-global simulations of the magneto-rotational instability in core collapse supernovae
• Magnetized Relativistic Jets and Long-Duration GRBs from Magnetar Spindown during Core-Collapse Supernovae
• The bar-mode instability in differentially rotating neutron stars: Simulations in full general relativity
• Proto-Neutron Star Winds with Magnetic Fields and Rotation
• The Propeller Regime of Disk Accretion to a Rapidly Rotating Magnetized Star
• Axisymmetric simulations of magneto--rotational core collapse: dynamics and gravitational wave signal
• Core-collapse supernova explosions triggered by a quark-hadron phase transition during the early post-bounce phase
• A new multidimensional, energy-dependent two-moment transport code for neutrino-hydrodynamics
• Dynamical Rotational Instability at Low $T/W$
• Discovery of a strong magnetic field on the O star HD 191612: new clues to the future of theta1 Orionis C?
• Axisymmetric MHD simulations of the collapsar model for gamma-ray bursts
• Relativistic Jets and Long-Duration Gamma-ray Bursts from the Birth of Magnetars
• Systematic Features of Axisymmetric Neutrino-Driven Core-Collapse Supernova Models in Multiple Progenitors
• The Proto-neutron Star Phase of the Collapsar Model and the Route to Long-soft Gamma-ray Bursts and Hypernovae
• Effects of Fall-Back Accretion on Proto-Magnetar Outflows in Gamma-Ray Bursts and Superluminous Supernovae
• Magnetorotational core collapse of possible GRB progenitors. I. Explosion mechanisms
• The origin and propagation of variability in the outflows of long duration gamma-ray bursts
• Photospheric emission as the dominant radiation mechanism in long-duration gamma-ray bursts
• Magnetorotational Explosion of A Massive Star Supported by Neutrino Heating in General Relativistic Three Dimensional Simulations
• Stellar explosions powered by the Blandford-Znajek mechanism
• Magnetar Driven Bubbles and the Origin of Collimated Outflows in Gamma-ray Bursts
• Deceleration of arbitrarily magnetized GRB ejecta: the complete evolution
• Jet propagations, breakouts and photospheric emissions in collapsing massive progenitors of long duration gamma ray bursts
• Magnetar formation through a convective dynamo in protoneutron stars
• Related progenitor models for long-duration gamma ray bursts and Type Ic superluminous supernovae
• Axisymmetric simulations of magnetorotational core collapse: Approximate inclusion of general relativistic effects
• Magnetic field amplification and magnetically supported explosions of collapsing, non-rotating stellar cores
• Angular Energy Distribution of Collapsar-Jets
• Three-dimensional AMR simulations of long-duration Gamma-Ray Burst jets inside massive progenitor stars
• The nature of low T/|W| dynamical instabilities in differentially rotating stars
• Magnetically-driven explosions of rapidly-rotating white dwarfs following Accretion-Induced Collapse
• Protomagnetar and black hole formation in high-mass stars
• Numerical Study on GRB-Jet Formation in Collapsars
• Constraining the GRB-magnetar model by means of the Galactic pulsar population
• Magnetar-Driven Magnetic Tower as a Model for Gamma-Ray Bursts and Asymmetric Supernovae
• Collimated Jet or Expanding Outflow: Possible Origins of GRBs and X-Ray Flashes
• The Birth Function for Black Holes and Neutron Stars in Close Binaries
• The GRB-SLSN Connection: mis-aligned magnetars, weak jet emergence, and observational signatures
• The effects of surface fossil magnetic fields on massive star evolution: I. Magnetic field evolution, mass-loss quenching and magnetic braking
• Accretion modes in collapsars - prospects for GRB production
• Rotating proto-neutron stars: spin evolution, maximum mass and I-Love-Q relations
• On the existence of a reverse shock in magnetized GRB ejecta
• Viscous, Resistive Magnetorotational Modes
• Low T/|W| dynamical instability in differentially rotating stars: Diagnosis with canonical angular momentum
• The impact of non-dipolar magnetic fields in core-collapse supernovae
• Photospheric Emission from Collapsar Jets in 3D Relativistic Hydrodynamics
• On the maximum magnetic field amplification by the magnetorotational instability in core-collapse supernovae
• Neutrino viscosity and drag: impact on the magnetorotational instability in protoneutron stars
• Global Simulations of Magnetorotational Instability in The Collapsed Core of A Massive Star
• Wind anisotropies and GRB progenitors
• Local Simulations of the Magneto-rotational Instability in Core-Collapse Supernovae
• Long-Term Evolution of Slowly Rotating Collapsar in Special Relativistic Magnetohydrodynamics
• Core collapse with magnetic fields and rotation
• Termination of the magnetorotational instability via parasitic instabilities in core-collapse supernovae
• Are pulsars born with a hidden magnetic field?
• Photospheric emission from long duration gamma-ray bursts powered by variable engines
• On the measurements of numerical viscosity and resistivity in Eulerian MHD codes
• Stability analysis of relativistic jets from collapsars and its implications on the short-term variability of gamma-ray bursts
• Striped Blandford/Znajek jets from advection of small scale magnetic field
• On MHD jet production in the collapsing and rotating envelope
• Dynamical bar-mode instability in rotating and magnetized relativistic stars
• Three-dimensional simulations of long duration gamma-ray burst jets: time scales from variable engines
• Magnetic effects on the low-T/|W| instability in differentially rotating neutron stars
• The Arduous Journey to Black-Hole Formation in Potential Gamma-Ray Burst Progenitors
• Neutron star collapse and gravitational waves with a non-convex equation of state
• Numerically solving the relativistic Grad-Shafranov equation in Kerr spacetimes: Numerical techniques
• Numerical models of blackbody-dominated gamma-ray bursts -- II. Emission properties
• Dynamical Bar-Mode Instability in Differentially Rotating Magnetized Neutron Stars
• Numerical models of blackbody-dominated gamma-ray bursts -- I. Hydrodynamics and the origin of the thermal emission
• On the existence of a luminosity threshold of GRB jets in massive stars
• Magnetized stars with differential rotation and a differential toroidal field
• The propagation of neutrino-driven jets in Wolf-Rayet stars
• Inner Engine Shutdown from Transitions in the Angular Momentum Distribution in Collapsars
• Termination of the MRI via parasitic instabilities in core-collapse supernovae: influence of numerical methods

Cited by in corpus (50)

• Magnetorotational core collapse of possible GRB progenitors. III. Three-dimensional models
• Neutrino absorption and other physics dependencies in neutrino-cooled black-hole accretion disks
• Magnetorotational supernovae: A nucleosynthetic analysis of sophisticated 3D models
• The spins of compact objects born from helium stars in binary systems
• Nucleosynthesis in magneto-rotational supernovae
• The Essential Character of the Neutrino Mechanism of Core-Collapse Supernova Explosions
• Pulsational pair-instability supernovae: gravitational collapse, black-hole formation, and beyond
• Three-dimensional core-collapse supernovae with complex magnetic structures: I. Explosion dynamics
• Magnetorotational core collapse of possible GRB progenitors. IV. A wider range of progenitors
• Three dimensional magnetorotational core-collapse supernova explosions of a 39 solar mass progenitor star
• R-process viable outflows are suppressed in global alpha-viscosity models of collapsar disks
• 3D Simulations of Oxygen Shell Burning with and without Magnetic Fields
• The double-peaked type Ic Supernova 2019cad: another SN 2005bf-like object
• Three-dimensional GRMHD Simulations of Rapidly Rotating Stellar Core-Collapse
• Collapsar Black Holes are Likely Born Slowly Spinning
• The effects of surface fossil magnetic fields on massive star evolution: IV. Grids of models at Solar, LMC, and SMC metallicities
• 3D code for MAgneto-Thermal evolution in Isolated Neutron Stars, MATINS: The Magnetic Field Formalism
• Ultra-delayed neutrino-driven explosion of rotating massive-star collapse
• A Stochastic Approach To Reconstruct Gamma Ray Burst Lightcurves
• The magneto-rotational instability in massive stars
• A Comparison of 2D Magnetohydrodynamic Supernova Simulations with the CoCoNuT-FMT and Aenus-Alcar Codes
• Magnetism in High-Mass Stars
• Chemical stratification in a long gamma-ray burst cocoon and early-time spectral signatures of supernovae associated with gamma-ray bursts
• 3D evolution of neutron star magnetic-fields from a realistic core-collapse turbulent topology
• Magnetically-Driven Neutron-Rich Ejecta Unleashed: Global 3D Neutrino-General Relativistic Magnetohydrodynamic Simulations of Collapsars Probe the Conditions for r-process Nucleosynthesis
• Long-duration Gamma-ray Burst Progenitors and Magnetar Formation
• The evolution of a newborn millisecond magnetar with a propeller-recycling disk
• Fast cooling and internal heating in hyperon stars
• Mixing of materials in magnetised core-collapse supernova remnants
• Neutrino Echos following Black Hole Formation in Core-Collapse Supernovae
• A Mechanical Model for Magnetized Relativistic Blastwaves
• GRB Optical and X-ray Plateau Properties Classifier Using Unsupervised Machine Learning
• Magnetar central engines in gamma-ray busts follow the universal relation of accreting magnetic stars
• Thermal luminosity degeneracy of magnetized neutron stars with and without hyperon cores
• Magnetorotational neutron star kicks
• Constraining the onset density for the QCD phase transition with the neutrino signal from core-collapse supernovae
• A Study of Primordial Very Massive Star Evolution. II. Stellar Rotation and Gamma-Ray Burst Progenitors
• Tracing the ejecta structure of SN 1987A: Insights and diagnostics from 3D MHD simulations
• Diffuse Neutrino Background from Magnetorotational Stellar Core Collapses
• Variety of disk wind-driven explosions in massive rotating stars
• Polarized radio emission unveils the structure of the pre-supernova circumstellar magnetic field and the radio emission in SN1987A
• Computational General Relativistic Force-Free Electrodynamics: I. Multi-Coordinate Implementation and Testing
• Magnetar field dynamics shaped by chiral anomalies and helicity
• Reality of inverse cascading in neutron star crusts
• Discovery and Analysis of Afterglows from Poorly Localised GRBs with the Gravitational-wave Optical Transient Observer (GOTO) All-sky Survey
• Small Progenitors, Large Couplings: Type Ic Supernova Constraints on Radiatively Decaying Particles
• Multi-Model Framework for Reconstructing Gamma-Ray Burst Light Curves
• MRI-driven $\alpha \Omega$ dynamo at high Pm numbers
• Evolution of Crab Pulsar: Magnetic Inclination Angle and Spin
• On the Origin of Pulsar and Magnetar Magnetic Fields