Ultra-delayed neutrino-driven explosion of rotating massive-star collapse

Abstract

Long-term neutrino-radiation hydrodynamics simulations in full general relativity are performed for the collapse of rotating massive stars that are evolved from He-stars with their initial mass of $20$ and $32M_{\odot }$. It is shown that if the collapsing stellar core has sufficient angular momentum, the rotationally-supported proto-neutron star (PNS) survives for seconds accompanying the formation of a massive torus of mass larger than $1M_{\odot }$. Subsequent mass accretion onto the central region produces a massive and compact central object, and eventually enhances the neutrino luminosity beyond $10^{53}$\,erg/s, resulting in a very delayed neutrino-driven explosion in particular toward the polar direction. The kinetic energy of the explosion can be appreciably higher than $10^{52}$ erg for a massive progenitor star and compatible with that of energetic supernovae like broad-line type-Ic supernovae. By the subsequent accretion, the massive PNS collapses eventually into a rapidly spinning black hole, which could be a central engine for gamma-ray bursts if a massive torus surrounds it.

arXiv comment12 pages, 5 figures, accepted for publication in ApJ

References in corpus (56)

• Collapsars - Gamma-Ray Bursts and Explosions in "Failed Supernovae"
• The Physics of Gamma-Ray Bursts
• The Supernova -- Gamma-Ray Burst Connection
• On the Numerical Integration of Einstein's Field Equations
• Exploring the Sensitivity of Next Generation Gravitational Wave Detectors
• The Progenitor Stars of Gamma-Ray Bursts
• Supernovae, Jets, and Collapsars
• Core-collapse supernova equations of state based on neutron star observations
• Evolution of rapidly rotating metal-poor massive stars towards gamma-ray bursts
• The Observer's Guide to the Gamma-Ray Burst-Supernova Connection
• Magnetorotational Core-Collapse Supernovae in Three Dimensions
• Conditions for Shock Revival by Neutrino Heating in Core-Collapse Supernovae
• Bipolar Supernova Explosions: Nucleosynthesis & Implication on Abundances in Extremely Metal-Poor Stars
• A New Multi-Dimensional General Relativistic Neutrino Hydrodynamics Code for Core-Collapse Supernovae II. Relativistic Explosion Models of Core-Collapse Supernovae
• New Hyperon Equations of State for Supernovae and Neutron Stars in Density-dependent Hadron Field Theory
• Mass Ejection from the Remnant of a Binary Neutron Star Merger: Viscous-Radiation Hydrodynamics Study
• Asphericity in Supernova Explosions from Late-Time Spectroscopy
• Truncated Moment Formalism for Radiation Hydrodynamics in Numerical Relativity
• An Asymmetric, Energetic Type Ic Supernova Viewed Off-Axis, and a Link to Gamma-Ray Bursts
• Compact binary evolutions with the Z4c formulation
• Hydrodynamics of core-collapse supernovae and their progenitors
• Self-consistent 3D Supernova Models From -7 Minutes to +7 Seconds: a 1-bethe Explosion of a ~19 Solar-mass Progenitor
• High-spin binary black hole mergers
• Impact of an improved neutrino energy estimate on outflows in neutron star merger simulations
• A unified picture for low-luminosity and long gamma-ray bursts based on the extended progenitor of llgrb 060218/SN 2006aj
• Symmetry without Symmetry: Numerical Simulation of Axisymmetric Systems using Cartesian Grids
• Three-Dimensional Supernova Explosion Simulations of 9-, 10-, 11-, 12-, and 13-M${}_{\odot }$ Stars
• Three-dimensional Models of Core-collapse Supernovae From Low-mass Progenitors With Implications for Crab
• Binary Merger Progenitors for Gamma-Ray Bursts and Hypernovae
• Relativistic supernovae have shorter-lived central engines or more extended progenitors: the case of SN\,2012ap
• Properties of Neutrino-driven Ejecta from the Remnant of Binary Neutron Star Merger : Purely Radiation Hydrodynamics Case
• Stellar Yields of Rotating First Stars. II. Pair Instability Supernovae and Comparison with Observations
• Three-dimensional simulations of stellar core collapse in full general relativity: Nonaxisymmetric dynamical instabilities
• Unifying the Zoo of Jet-Driven Stellar Explosions
• The Connection between Gamma-Ray Bursts and Extremely Metal-Poor Stars: Black Hole-forming Supernovae with Relativistic Jets
• Magnetorotational core collapse of possible GRB progenitors. I. Explosion mechanisms
• Magnetorotational Explosion of A Massive Star Supported by Neutrino Heating in General Relativistic Three Dimensional Simulations
• Mass ejection from disks surrounding a low-mass black hole: Viscous neutrino-radiation hydrodynamics simulation in full general relativity
• Related progenitor models for long-duration gamma ray bursts and Type Ic superluminous supernovae
• Gravitational-wave signal of a core-collapse supernova explosion of a 15 Solar mass star
• Magnetorotational core collapse of possible GRB progenitors. III. Three-dimensional models
• Post-merger Mass Ejection of Low-mass Binary Neutron Stars
• Protomagnetar and black hole formation in high-mass stars
• Magnetorotational core collapse of possible GRB progenitors. II. Formation of protomagnetars and collapsars
• Formation of black hole and accretion disk in a massive high-entropy stellar core collapse
• Monte-Carlo neutrino transport in neutron star merger simulations
• Axisymmetric Simulations of Rotating Stellar Collapse in Full General Relativity --- Criteria for Prompt Collapse to Black Holes
• The Neutrino Signal in Stellar Core Collapse and Postbounce Evolution
• Long-term Simulations of Multi-Dimensional Core-collapse Supernovae: Implications for Neutron Star Kicks
• A New Gravitational Wave Signature of Low-$T/|W|$ Instability in Rapidly Rotating Stellar Core Collapse
• Stellar core collapse in full general relativity with microphysics - Formulation and Spherical collapse test -
• Long-term evolution of a merger-remnant neutron star in general relativistic magnetohydrodynamics I: Effect of magnetic winding
• The Boltzmann-radiation-hydrodynamics Simulations of Core-collapse Supernovae with Different Equations of State: the Role of Nuclear Composition and the Behavior of Neutrinos
• Post-shock-revival evolutions in the neutrino-heating mechanism of core-collapse supernovae
• Alternative possibility of GW190521: Gravitational waves from high-mass black hole-disk systems
• Properties of neutrino transfer in a deformed remnant of neutron star merger

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