Explosion geometry of a rotating 13 $M_{\odot }$ star driven by the SASI-aided neutrino-heating supernova mechanism

Abstract

By performing axisymmetric hydrodynamic simulations of core-collapse supernovae with spectral neutrino transport based on the isotropic diffusion source approximation scheme, we support the assumption that the neutrino-heating mechanism aided by the standing accretion shock instability and convection can initiate an explosion of a 13 $M_{\odot }$ star. Our results show that bipolar explosions are more likely to be associated with models which include rotation. We point out that models, which form a north-south symmetric bipolar explosion, can lead to larger explosion energies than for the corresponding unipolar explosions.

5 pages, 4 figures; accepted for publication in PASJ Letters

References in corpus (13)

• Delayed neutrino-driven supernova explosions aided by the standing accretion-shock instability
• Signals of the QCD phase transition in core-collapse supernovae
• Instability of a stalled accretion shock: evidence for the advective-acoustic cycle
• Criteria for Core-Collapse Supernova Explosions by the Neutrino Mechanism
• The isotropic diffusion source approximation for supernova neutrino transport
• Features of the Acoustic Mechanism of Core-Collapse Supernova Explosions
• Special Relativistic Simulations of Magnetically-dominated Jets in Collapsing Massive Stars
• Gravitational waves from 3D MHD core collapse simulations
• Effect of Rotation on the Stability of a Stalled Cylindrical Shock and its Consequences for Core-Collapse Supernovae
• Effects of Rotation on Standing Accretion Shock Instability in Nonlinear Phase for Core-Collapse Supernovae
• The saturation of SASI by parasitic instabilities
• Multi-Dimensional Simulations for Early Phase Spectra of Aspherical Hypernovae: SN 1998bw and Off-Axis Hypernovae
• Mechanisms of Core-Collapse Supernovae & Simulation Results from the CHIMERA Code

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