Pushing 1D CCSNe to explosions: model and SN 1987A

Abstract

We report on a method, PUSH, for triggering core-collapse supernova explosions of massive stars in spherical symmetry. We explore basic explosion properties and calibrate PUSH such that the observables of SN1987A are reproduced. Our simulations are based on the general relativistic hydrodynamics code AGILE combined with the detailed neutrino transport scheme IDSA for electron neutrinos and ALS for the muon and tau neutrinos. To trigger explosions in the otherwise non-exploding simulations, we rely on the neutrino-driven mechanism. The PUSH method locally increases the energy deposition in the gain region through energy deposition by the heavy neutrino flavors. Our setup allows us to model the explosion for several seconds after core bounce. We explore the progenitor range 18-21M${}_{\odot }$. Our studies reveal a distinction between high compactness (HC) and low compactness (LC) progenitor models, where LC models tend to explore earlier, with a lower explosion energy, and with a lower remnant mass. HC models are needed to obtain explosion energies around 1 Bethe, as observed for SN1987A. However, all the models with sufficiently high explosion energy overproduce ${}^{56}$Ni. We conclude that fallback is needed to reproduce the observed nucleosynthesis yields. The nucleosynthesis yields of ${}^{57-58}$Ni depend sensitively on the electron fraction and on the location of the mass cut with respect to the initial shell structure of the progenitor star. We identify a progenitor and a suitable set of PUSH parameters that fit the explosion properties of SN1987A when assuming 0.1M${}_{\odot }$ of fallback. We predict a neutron star with a gravitational mass of 1.50M${}_{\odot }$. We find correlations between explosion properties and the compactness of the progenitor model in the explored progenitors. However, a more complete analysis will require the exploration of a larger set of progenitors with PUSH.

revised version as accepted by ApJ (results unchanged, text modified for clarification, a few references added); 26 pages, 20 figures

References in corpus (21)

• Shapiro delay measurement of a two solar mass neutron star
• A Massive Pulsar in a Compact Relativistic Binary
• Magnetorotationally driven Supernovae as the origin of early galaxy $r$-process elements?
• Neutrino-driven winds from neutron star merger remnants
• The nucleosynthesis of Al26 and Fe60 in solar metallicity stars extending in mass from 11 to 120 Msun: the hydrostatic and explosive contributions
• Delayed neutrino-driven supernova explosions aided by the standing accretion-shock instability
• Asymmetries in core-collapse supernovae from maps of radioactive ${}^{44}$Ti in CassiopeiaA
• Neutrino-driven supernova of a low-mass iron-core progenitor boosted by three-dimensional turbulent convection
• Criteria for Core-Collapse Supernova Explosions by the Neutrino Mechanism
• The isotropic diffusion source approximation for supernova neutrino transport
• Multidimensional supernova simulations with approximative neutrino transport. II. Convection and the advective-acoustic cycle in the supernova core
• How much 56Ni can be produced in Core-Collapse Supernovae? : Evolution and Explosions of 30 - 100 Msun Stars
• The Progenitor Dependence of the Preexplosion Neutrino Emission in Core-Collapse Supernovae
• Hard X-ray emission lines from the decay of Ti-44 in the remnant of supernova 1987A
• The light curve of SN 1987A revisited: constraining production masses of radioactive nuclides
• X-ray illumination of the ejecta of Supernova 1987A
• Effects of Rotation on Standing Accretion Shock Instability in Nonlinear Phase for Core-Collapse Supernovae
• Spectral and morphological analysis of the remnant of Supernova 1987A with ALMA & ATCA
• Comparative analysis of SN1987A antineutrino fluence
• High-resolution radio observations of SNR 1987A at high frequencies
• Nucleon self-energies for supernova equations of state

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