Magnetorotational Explosion of A Massive Star Supported by Neutrino Heating in General Relativistic Three Dimensional Simulations

Abstract

We present results of three-dimensional (3D), radiation-magnetohydrodynamics (MHD) simulations of core-collapse supernovae in full general relativity (GR) with spectral neutrino transport. In order to study the effects of progenitor's rotation and magnetic fields, we compute three models, where the precollapse rotation rate and magnetic fields are included parametrically to a 20 M${}_{\odot }$ star. While we find no shock revival in our two non-magnetized models during our simulation times ($\sim 500$ ms after bounce), the magnetorotationally (MR) driven shock expansion immediately initiates after bounce in our rapidly rotating and strongly magnetized model. We show that the expansion of the MR-driven flows toward the polar directions is predominantly driven by the magnetic pressure, whereas the shock expansion toward the equatorial direction is supported by neutrino heating. Our detailed analysis indicates that the growth of the so-called kink instability may hinder the collimation of jets, resulting in the formation of broader outflows. Furthermore we find a dipole emission of lepton number, only in the MR explosion model, whose asymmetry is consistent with the explosion morphology. Although it is similar to the lepton-number emission self-sustained asymmetry (LESA), our analysis shows that the dipole emission occurs not from the protoneutron star convection zone but from above the neutrino sphere indicating that it is not associated with the LESA. We also report several unique neutrino signatures, which are significantly dependent on both the time and the viewing angle, if observed, possibly providing a rich information regarding the onset of the MR-driven explosion.

19 pages, 14 figures, accepted for publication in the ApJ

References in corpus (25)

• Nucleosynthesis and Remnants in Massive Stars of Solar Metallicity
• Magnetorotationally driven Supernovae as the origin of early galaxy $r$-process elements?
• Delayed neutrino-driven supernova explosions aided by the standing accretion-shock instability
• Three-dimensional core-collapse supernova simulated using a 15 $M_{\odot }$ progenitor
• Magnetorotational Core-Collapse Supernovae in Three Dimensions
• Pulsar spins from an instability in the accretion shock of supernovae
• Asphericity in Supernova Explosions from Late-Time Spectroscopy
• Truncated Moment Formalism for Radiation Hydrodynamics in Numerical Relativity
• The Role of Turbulence in Neutrino-Driven Core-Collapse Supernova Explosions
• The Status of Multi-Dimensional Core-Collapse Supernova Models
• Muon Creation in Supernova Matter Facilitates Neutrino-driven Explosions
• High-spin binary black hole mergers
• Semi-global simulations of the magneto-rotational instability in core collapse supernovae
• Special Relativistic Simulations of Magnetically-dominated Jets in Collapsing Massive Stars
• The explosion mechanism of core-collapse supernovae: progress in supernova theory and experiments
• Three-Dimensional Supernova Explosion Simulations of 9-, 10-, 11-, 12-, and 13-M${}_{\odot }$ Stars
• Rotation-supported Neutrino-driven Supernova Explosions in Three Dimensions and the Critical Luminosity Condition
• Magnetar formation through a convective dynamo in protoneutron stars
• Magnetic field amplification and magnetically supported explosions of collapsing, non-rotating stellar cores
• Neutrino-nucleon scattering in supernova matter from the virial expansion
• Anisotropic emission of neutrino and gravitational-wave signals from rapidly rotating core-collapse supernovae
• A systematic study of proto-neutron star convection in three-dimensional core-collapse supernova simulations
• Impacts of Rotation on Three-dimensional Hydrodynamics of Core-collapse Supernovae
• Magnetohydrodynamic Turbulence Powered by Magnetorotational Instability in Nascent Proto-Neutron Stars
• Three Dimensional Magnetohydrodynamical Simulations of Core Collapse Supernova

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