PUSHing core-collapse supernovae to explosions in spherical symmetry IV: Explodability, remnant properties and nucleosynthesis yields of low metallicity stars

Abstract

In this fourth paper of the series, we use the parametrized, spherically symmetric explosion method PUSH to perform a systematic study of two sets of non-rotating stellar progenitor models. Our study includes pre-explosion models with metallicities Z=0 and Z=Z${}_{\odot }\times 10^{-4}$ and covers a progenitor mass range from 11 up to 75 M${}_{\odot }$. We present and discuss the explosion properties of all models and predict remnant (neutron star or black hole) mass distributions within this approach. We also perform systematic nucleosynthesis studies and predict detailed isotopic yields as function of the progenitor mass and metallicity. We present a comparison of our nucleosynthesis results with observationally derived ${}^{56}$Ni ejecta from normal core-collapse supernovae and with iron-group abundances for metal-poor star HD~84937. Overall, our results for explosion energies, remnant mass distribution, ${}^{56}$Ni mass, and iron group yields are consistent with observations of normal CCSNe. We find that stellar progenitors at low and zero metallicity are more prone to BH formation than those at solar metallicity, which allows for the formation of BHs in the mass range observed by LIGO/VIRGO.

arXiv comment22 pages, 16 figures, 6 tables. Accepted to ApJ

References in corpus (48)

• Nuclear Ground-State Masses and Deformations
• GWTC-1: A Gravitational-Wave Transient Catalog of Compact Binary Mergers Observed by LIGO and Virgo during the First and Second Observing Runs
• Core-Collapse Supernovae from 9 to 120 Solar Masses Based on Neutrino-powered Explosions
• Properties of the Binary Black Hole Merger GW150914
• Nucleosynthesis in Massive Stars With Improved Nuclear and Stellar Physics
• Astrophysical Reaction Rates From Statistical Model Calculations
• Black Hole Formation in Failing Core-Collapse Supernovae
• Nucleosynthesis Yields of Core-Collapse Supernovae and Hypernovae, and Galactic Chemical Evolution
• Nucleosynthesis and Remnants in Massive Stars of Solar Metallicity
• Nucleosynthesis and Evolution of Massive Metal-Free Stars
• Statistical Model for a Complete Supernova Equation of State
• Neutrino-induced nucleosynthesis of A>64 nuclei: The nu p-process
• Presupernova evolution and explosive nucleosynthesis of rotating massive stars in the metallicity range -3 <=[Fe/H]<= 0
• Progenitor-Explosion Connection and Remnant Birth Masses for Neutrino-Driven Supernovae of Iron-Core Progenitors
• The nucleosynthesis of Al26 and Fe60 in solar metallicity stars extending in mass from 11 to 120 Msun: the hydrostatic and explosive contributions
• A two-parameter criterion for classifying the explodability of massive stars by the neutrino-driven mechanism
• On the Mass Distribution and Birth Masses of Neutron Stars
• The Compactness of Presupernova Stellar Cores
• The Overarching Framework of Core-Collapse Supernova Explosions as Revealed by 3D Fornax Simulations
• Very Low Energy Supernovae from Neutrino Mass Loss
• High Resolution Study of Presupernova Compactness
• The Landscape of the Neutrino Mechanism of Core-Collapse Supernovae: Neutron Star and Black Hole Mass Functions, Explosion Energies and Nickel Yields
• A Simple Approach to the Supernova Progenitor-Explosion Connection
• Composition of the Innermost Core Collapse Supernova Ejecta
• Charged-Particle and Neutron-Capture Processes in the High-Entropy Wind of Core-Collapse Supernovae
• The isotropic diffusion source approximation for supernova neutrino transport
• How much 56Ni can be produced in Core-Collapse Supernovae? : Evolution and Explosions of 30 - 100 Msun Stars
• Nucleosynthesis in the Innermost Ejecta of Neutrino-Drive Supernova Explosions in Two Dimensions
• Super-AGB Stars and their role as Electron Capture Supernova progenitors
• PUSHing Core-Collapse Supernovae to Explosions in Spherical Symmetry III: Nucleosynthesis Yields
• The Search for Failed Supernovae with the Large Binocular Telescope: Constraints from 7 Years of Data
• Pushing 1D CCSNe to explosions: model and SN 1987A
• Presupernova evolution and explosive nucleosynthesis of zero metal massive stars
• Conservative General Relativistic Radiation Hydrodynamics in Spherical Symmetry and Comoving Coordinates
• Iron-Group Abundances in the Metal-Poor Main Sequence Turnoff Star HD~84937
• The Nickel Mass Distribution of Normal Type II Supernovae
• Simulating Turbulence-aided Neutrino-driven Core-collapse Supernova Explosions in One Dimension
• PUSHing Core-Collapse Supernovae to Explosions in Spherical Symmetry II: Explodability and Global Properties
• The light curve of SN 1987A revisited: constraining production masses of radioactive nuclides
• Implications for Post-Processing Nucleosynthesis of Core-Collapse Supernova Models with Lagrangian Particles
• An advanced leakage scheme for neutrino treatment in astrophysical simulations
• Radioactivities and nucleosynthesis in SN 1987A
• Confronting Models of Massive Star Evolution and Explosions with Remnant Mass Measurements
• Nucleosynthesis in 2D Core-Collapse Supernovae of 11.2 and 17.0 M${}_{\odot }$ Progenitors: Implications for Mo and Ru Production
• A high-entropy wind r-process study based on nuclear-structure quantities from the new finite-range droplet model FRDM(2012)
• Explosive nucleosynthesis of ultra-stripped Type Ic supernovae: application to light trans-iron elements
• Convection-Aided Explosions in One-Dimensional Core-Collapse Supernova Simulations I: Technique and Validation
• The synthesis of Ti44 and Ni56 in massive stars

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• Neutrino-driven Core-collapse Supernova Yields in Galactic Chemical Evolution
• Empirical Constraints on Core Collapse Supernova Yields using Very Metal Poor Damped Lyman Alpha Absorbers
• A New Constraint on the Nuclear Equation of State from Statistical Distributions of Compact Remnants of Supernovae
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