Special Relativistic Simulations of Magnetically-dominated Jets in Collapsing Massive Stars

Abstract

We perform a series of two-dimensional magnetohydrodynamic core-collapse simulations of rapidly rotating and strongly magnetized massive stars. To study the properties of magnetic explosions for a longer time stretch of postbounce evolution, we develop a new code under the framework of special relativity including a realistic equation of state with a multiflavor neutrino leakage scheme. Our results show the generation of the magnetically-dominated jets in the two ways. One is launched just after the core-bounce in a prompt way and another is launched at $\sim 100$ ms after the stall of the prompt shock. We find that the shock-revival occurs when the magnetic pressure becomes strong, due to the field wrapping, enough to overwhelm the ram pressure of the accreting matter. The critical toroidal magnetic fields for the magnetic shock-revival are found to be universal of $\sim 10^{15}\mathrm{G}$ behind the jets. We point out that the time difference before the shock-revival has a strong correlation with the explosions energies. Our results suggest that the magnetically dominated jets are accompanied by the formation of the magnetars. Since the jets are mildly relativistic, we speculate that they might be the origin of some observed X-ray flashes.

arXiv comment50 pages, 14 figures, Accepted to ApJ, A paper with high-resolution figures available at http://www-utap.phys.s.u-tokyo.ac.jp/~takiwaki/res/index-j.html

References in corpus (77)

• Collapsars - Gamma-Ray Bursts and Explosions in "Failed Supernovae"
• Discovery of the peculiar supernova 1998bw in the error box of GRB980425
• Gamma-Ray Bursts and the Fireball Model
• Neutron Star Observations: Prognosis for Equation of State Constraints
• Spectroscopic Discovery of the Supernova 2003dh Associated with GRB 030329
• Gamma-Ray Bursts
• Are Gamma-Ray Bursts in Star Forming Regions?
• Dynamo action by differential rotation in a stably stratified stellar interior
• The Progenitor Stars of Gamma-Ray Bursts
• Relativistic Equation of State of Nuclear Matter for Supernova and Neutron Star
• Theory of Core-Collapse Supernovae
• Presupernova Evolution of Differentially Rotating Massive Stars Including Magnetic Fields
• Physics of Strongly Magnetized Neutron Stars
• Nucleosynthesis in neutrino-driven winds: I. The physical conditions
• Electrodynamics of Magnetars: Implications for the Persistent X-ray Emission and Spindown of the Soft Gamma Repeaters and Anomalous X-ray Pulsars
• Evolution of rapidly rotating metal-poor massive stars towards gamma-ray bursts
• General Relativistic Magnetohydrodynamic Simulations of Jet Formation and Large-Scale Propagation from Black Hole Accretion Systems
• Relativistic ejecta from XRF 060218 and the rate of cosmic explosions
• Presupernova Evolution of Rotating Massive Stars II: -- Evolution of the Surface Properties
• 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
• Discovery of Rapid X-ray Oscillations in the Tail of the SGR 1806-20 Hyperflare
• Magnetar Spindown, Hyper-Energetic Supernovae, and Gamma Ray Bursts
• Asymmetric Supernovae, Pulsars, Magnetars, and Gamma-Ray Bursts
• The Giant Flare of 1998 August 27 from SGR 1900+14: II. Radiative Mechanism and Physical Constraints on the Source
• Magnetically Driven Accretion Flows in the Kerr Metric I: Models and Overall Structure
• Magnetically Driven Jets in the Kerr Metric
• A neutron-star-driven X-ray flash associated with supernova SN 2006aj
• Explosion Mechanism, Neutrino Burst, and Gravitational Wave in Core-Collapse Supernovae
• Relativistic Jets from Collapsars
• High Resolution Calculations of Merging Neutron Stars II: Neutrino Emission
• Magnetically Driven Accretion in the Kerr Metric III: Unbound Outflows
• Magnetar-like X-ray Bursts from an Anomalous X-ray Pulsar
• The Unique Type Ib Supernova 2005bf at Nebular Phases: A Possible Birth Event of A Strongly Magnetized Neutron Star
• Proto-Neutron Star Winds with Magnetic Fields and Rotation
• Magnetorotational collapse of massive stellar cores to neutron stars: Simulations in full general relativity
• Magnetically Driven Accretion Flows in the Kerr Metric IV: Dynamical Properties of the Inner Disk
• Axisymmetric MHD simulations of the collapsar model for gamma-ray bursts
• Relativistic Jets and Long-Duration Gamma-ray Bursts from the Birth of Magnetars
• "Meissner effect" and Blandford-Znajek mechanism in conductive black hole magnetospheres
• R-Process Nucleosynthesis in MHD Jet Explosions of Core-Collapse Supernovae
• 3D Relativistic Magnetohydrodynamic Simulations of Magnetized Spine-Sheath Relativistic Jets
• Stellar explosions powered by the Blandford-Znajek mechanism
• Axisymmetric simulations of magnetorotational core collapse: Approximate inclusion of general relativistic effects
• New Evidence for Proton Cyclotron Resonance in a Magnetar Strength Field from SGR 1806-20
• Stellar Explosions by Magnetic Towers
• Disk-Jet Coupling in Black Hole Accretion Systems II: Force-Free Electrodynamical Models
• Magneto-driven Shock Waves in Core-Collapse Supernova
• Numerical Study on GRB-Jet Formation in Collapsars
• Low-Luminosity GRB 060218: A Collapsar Jet from a Neutron Star, Leaving a Magnetar as a Remnant?
• Magnetar-energized supernova explosions and GRB-jets
• Gravitational waves from 3D MHD core collapse simulations
• SN 2006aj Associated with XRF 060218 At Late Phases: Nucleosynthesis-Signature of A Neutron Star-Driven Explosion
• 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
• Magnetorotational Collapse of Population III Stars
• General Relativistic Augmentation of Neutrino Pair Annihilation Energy Deposition Near Neutron Stars
• General relativistic simulations of pasive-magneto-rotational core collapse with microphysics
• MHD Models of Axisymmetric Protostellar Jets
• Gravitational Radiation from Rotational Core Collapse: Effects of Magnetic Fields and Realistic Equation of States
• The Core-Collapse Supernova with "Non-Uniform" Magnetic Fields
• A General Relativistic Magnetohydrodynamics Simulation of Jet Formation
• Evidence of a cyclotron feature in the spectrum of the anomalous X-ray pulsar 1RXS J170849-400910
• Magnetohydrodynamic Simulations of A Rotating Massive Star Collapsing to A Black Hole
• High magnetic field pulsars and magnetars: a unified picture
• Relativistic Effects on Neutrino Pair Annihilation above a Kerr Black Hole with the Accretion Disk
• Neutrino Pair Annihilation in the Gravitation of Gamma Ray Burst Sources
• Did we observe the supernova shock breakout in GRB 060218?
• Astrophysical Explosions Driven by a Rotating, Magnetized, Gravitating Sphere
• Magnetically-dominated jets inside collapsing stars as a model for gamma-ray bursts and supernova explosions
• Nonaxisymmetric Magnetorotational Instability in Proto-Neutron Stars
• Numerical Simulations of Equatorially-Asymmetric Magnetized Supernovae: Formation of Magnetars and Their Kicks
• A Formation Mechanism of Collapsar Black Hole -- early evolution phase
• COSMOS: A Radiation-Chemo-Hydrodynamics Code for Astrophysical Problems
• GRB Host Studies (GHostS)
• Magnetars' Giant Flares: the case of SGR 1806-20

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