Three-dimensional core-collapse supernova simulated using a 15 $M_{\odot }$ progenitor

Abstract

We have performed ab initio neutrino radiation hydrodynamics simulations in three and two spatial dimensions (3D and 2D) of core-collapse supernovae from the same 15 $M_{\odot }$ progenitor through 440 ms after core bounce. Both 3D and 2D models achieve explosions, however, the onset of explosion (shock revival) is delayed by $\sim$100 ms in 3D relative to the 2D counterpart and the growth of the diagnostic explosion energy is slower. This is consistent with previously reported 3D simulations utilizing iron-core progenitors with dense mantles. In the $\sim$100 ms before the onset of explosion, diagnostics of neutrino heating and turbulent kinetic energy favor earlier explosion in 2D. During the delay, the angular scale of convective plumes reaching the shock surface grows and explosion in 3D is ultimately lead by a single, large-angle plume, giving the expanding shock a directional orientation not dissimilar from those imposed by axial symmetry in 2D simulations. We posit that shock revival and explosion in the 3D simulation may be delayed until sufficiently large plumes form, whereas such plumes form more rapidly in 2D, permitting earlier explosions.

7 pages, accepted for publication in ApJ Letters, animation available at ChimeraSN.org

References in corpus (25)

• Progenitors of core-collapse supernovae
• Explosion Mechanisms of Core-Collapse Supernovae
• Nucleosynthesis and Remnants in Massive Stars of Solar Metallicity
• Stability of Standing Accretion Shocks, With an Eye Toward Core Collapse Supernovae
• Inside the Supernova: A Powerful Convective Engine
• Two-Dimensional Hydrodynamic Core-Collapse Supernova Simulations with Spectral Neutrino Transport II. Models for Different Progenitor Stars
• Pulsar spins from an instability in the accretion shock of supernovae
• A Comparison of Two- and Three-dimensional Neutrino-hydrodynamics simulations of Core-collapse Supernovae
• Dimension as a Key to the Neutrino Mechanism of Core-Collapse Supernova Explosions
• SASI Activity in Three-Dimensional Neutrino-Hydrodynamics Simulations of Supernova Cores
• Is Strong SASI Activity the Key to Successful Neutrino-Driven Supernova Explosions?
• Three-dimensional Hydrodynamic Core-Collapse Supernova Simulations for an $11.2M_{\odot }$ Star with Spectral Neutrino Transport
• The Role of Turbulence in Neutrino-Driven Core-Collapse Supernova Explosions
• Neutrino-driven supernova of a low-mass iron-core progenitor boosted by three-dimensional turbulent convection
• 3-Dimensional Core-Collapse
• Axisymmetric Ab Initio Core-Collapse Supernova Simulations of 12-25 M_sol Stars
• Self-sustained asymmetry of lepton-number emission: A new phenomenon during the supernova shock-accretion phase in three dimensions
• Modeling Core-Collapse Supernovae in 3-Dimensions
• High-Resolution Three-Dimensional Simulations of Core-Collapse Supernovae in Multiple Progenitors
• Electron Neutrino Pair Annihilation: A New Source for Muon and Tau Neutrinos in Supernovae
• Dimensional Dependence of the Hydrodynamics of Core-Collapse Supernovae
• Interplay of Neutrino Opacities in Core-collapse Supernova Simulations
• On the Impact of Three Dimensions in Simulations of Neutrino-Driven Core-Collapse Supernova Explosions
• A Global Turbulence Model for Neutrino-Driven Convection in Core-Collapse Supernovae
• Toward connecting core-collapse supernova theory with observations: I. Shock revival in a 15 Msun blue supergiant progenitor with SN 1987A energetics

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