Neutrino-driven Core-collapse Supernova Yields in Galactic Chemical Evolution

Abstract

We provide yields from 189 neutrino-driven core-collapse supernova (CCSN) simulations covering zero-age main sequence masses between 11 and 75 solar masses and three different metallicities. Our CCSN simulations have two main advantages compared to previous methods used for applications in Galactic chemical evolution (GCE). Firstly, the mass cut between remnant and ejecta evolves naturally. Secondly, the neutrino luminosities and thus the electron fraction are not modified. Both is key to obtain an accurate nucleosynthesis. We follow the composition with an in-situ nuclear reaction network including the 16 most abundant isotopes and use the yields as input in a GCE model of the Milky Way. We adopt a GCE which takes into account infall of gas as well as nucleosynthesis from a large variety of stellar sources. The GCE model is calibrated to reproduce the main features of the solar vicinity. For the CCSN models, we use different calibrations and propagate the uncertainty. We find a big impact of the CCSN yields on our GCE predictions. We compare the abundance ratios of C, O, Ne, Mg, Si, S, Ar, Ca, Ti, and Cr with respect to Fe to an observational data set as homogeneous as possible. From this, we conclude that at least half of the massive stars have to explode to match the observed abundance ratios. If the explosions are too energetic, the high amount of iron will suppress the abundance ratios. With this, we demonstrate how GCE models can be used to constrain the evolution and deaths of massive stars.

13 pages, 11 figures, published in MNRAS

References in corpus (101)

• The chemical composition of the Sun
• The Apache Point Observatory Galactic Evolution Experiment (APOGEE)
• Grids of stellar models with rotation - I. Models from 0.8 to 120 Msun at solar metallicity (Z = 0.014)
• Nucleosynthesis in Chandrasekhar Mass Models for Type Ia Supernovae and Constraints on Progenitor Systems and Burning-Front Propagation
• Core-Collapse Supernovae from 9 to 120 Solar Masses Based on Neutrino-powered Explosions
• Exploring the Milky Way stellar disk. A detailed elemental abundance study of 714 F and G dwarf stars in the Solar neighbourhood
• Galactic chemical evolution: Carbon through Zinc
• Black Hole Formation in Failing Core-Collapse Supernovae
• Core-collapse supernova equations of state based on neutron star observations
• Nucleosynthesis and Remnants in Massive Stars of Solar Metallicity
• Abundance Gradients and the Formation of the Milky Way
• Chemical Cartography with APOGEE: Metallicity Distribution Functions and the Chemical Structure of the Milky Way Disk
• The GALAH+ Survey: Third Data Release
• 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
• Observed and Physical Properties of Core-Collapse Supernovae
• Physics of Core-Collapse Supernovae in Three Dimensions: a Sneak Preview
• Chemodynamical evolution of the Milky Way disk I: The solar vicinity
• Evolution, nucleosynthesis and yields of low mass AGB stars
• Evolution, nucleosynthesis and yields of low mass AGB stars at different metallicities (II): the FRUITY database
• Quantifying the uncertainties of chemical evolution studies. II. Stellar yields
• A two-parameter criterion for classifying the explodability of massive stars by the neutrino-driven mechanism
• Chemical evolution with rotating massive star yields: I. The solar neighbourhood and the s-process elements
• Evolution, nucleosynthesis and yields of AGB stars at different metallicities (III): intermediate mass models, revised low mass models and the ph-FRUITY interface
• Variations in the Abundance Pattern of Extremely Metal-poor Stars and Nucleosynthesis in Population III Supernovae
• Radiation hydrodynamics of SN 1987A: I. Global analysis of the light curve for the first 4 months
• A New Open-Source Code for Spherically-Symmetric Stellar Collapse to Neutron Stars and Black Holes
• The Overarching Framework of Core-Collapse Supernova Explosions as Revealed by 3D Fornax Simulations
• Supernova Simulations from a 3D Progenitor Model -- Impact of Perturbations and Evolution of Explosion Properties
• Bipolar Supernova Explosions: Nucleosynthesis & Implication on Abundances in Extremely Metal-Poor Stars
• The evolution of the Milky Way from its earliest phases : constraints on stellar nucleosynthesis
• The Landscape of the Neutrino Mechanism of Core-Collapse Supernovae: Neutron Star and Black Hole Mass Functions, Explosion Energies and Nickel Yields
• The Gaia-ESO Survey: the Galactic Thick to Thin Disc transition
• A Simple Approach to the Supernova Progenitor-Explosion Connection
• NuGrid stellar data set I. Stellar yields from H to Bi for stars with metallicities Z = 0.02 and Z = 0.01
• Exploring Fundamentally Three-dimensional Phenomena in High-fidelity Simulations of Core-collapse Supernovae
• Galactic Archaeology with asteroseismic ages: evidence for delayed gas infall in the formation of the Milky Way disc
• Super and Massive AGB Stars: II - Nucleosynthesis and Yields - Z=0.02, 0.008 and 0.004
• The Development of Explosions in Axisymmetric Ab Initio Core-Collapse Supernova Simulations of 12-25 $M_{\odot }$ Stars
• Chemical Cartography with APOGEE: Large-scale Mean Metallicity Maps of the Milky Way
• Carbon, oxygen, and iron abundances in disk and halo stars. Implications of 3D non-LTE spectral line formation
• The evolution of CNO isotopes: a new window on cosmic star-formation history and the stellar IMF in the age of ALMA
• A new multidimensional, energy-dependent two-moment transport code for neutrino-hydrodynamics
• The Progenitor Dependence of Three-Dimensional Core-Collapse Supernovae
• Carbon and oxygen abundances in stellar populations
• The Gaia-ESO Survey: the chemical structure of the Galactic discs from the first internal data release
• Progenitor-dependent Explosion Dynamics in Self-consistent, Axisymmetric Simulations of Neutrino-driven Core-collapse Supernovae
• The s-process in the Galactic halo: the fifth signature of spinstars in the early Universe?
• Super and massive AGB stars - III. Nucleosynthesis in metal-poor and very metal-poor stars - Z=0.001 and 0.0001
• PUSHing Core-Collapse Supernovae to Explosions in Spherical Symmetry III: Nucleosynthesis Yields
• Pushing 1D CCSNe to explosions: model and SN 1987A
• Magnetorotational Explosion of A Massive Star Supported by Neutrino Heating in General Relativistic Three Dimensional Simulations
• The evolution of CNO isotopes: the impact of massive stellar rotators
• The Nickel Mass Distribution of Normal Type II Supernovae
• Simulating Turbulence-aided Neutrino-driven Core-collapse Supernova Explosions in One Dimension
• APOGEE DR16: a multi-zone chemical evolution model for the Galactic disc based on MCMC methods
• Equation of state effects in core-collapse supernovae
• An inhomogeneous model for the Galactic halo: a possible explanation for the spread observed in s- and r-process elements
• Explaining the Ba, Y, Sr, and Eu abundance scatter in metal-poor halo stars: constraints to the r-process
• Neutron-Capture Nucleosynthesis in the First Stars
• PUSHing Core-Collapse Supernovae to Explosions in Spherical Symmetry II: Explodability and Global Properties
• Equation of state effects in the core collapse of a $20$-$M_{\odot }$ star
• 3D Hydrodynamic Simulations of Carbon Burning in Massive Stars
• The light curve of SN 1987A revisited: constraining production masses of radioactive nuclides
• Nova nucleosynthesis and Galactic evolution of the CNO isotopes
• Stellar migrations and metal flows -- Chemical evolution of the thin disc of a simulated Milky Way analogous galaxy
• Sulphur abundance in Galactic stars
• Chemical evolution of the Milky Way: constraints on the formation of the thick and thin discs
• The search for failed supernovae with the Large Binocular Telescope: a new candidate and the failed SN fraction with 11 yr of data
• Hydrodynamical simulations of Galactic fountains II: evolution of multiple fountains
• The Collapse and Three-Dimensional Explosion of Three-Dimensional, vis à vis One-Dimensional, Massive-star Supernova Progenitor Models
• Implications for Post-Processing Nucleosynthesis of Core-Collapse Supernova Models with Lagrangian Particles
• Abundance gradients along the Galactic disc from chemical evolution models
• The effect of stellar migration on Galactic chemical evolution: a heuristic approach
• Three Dimensional Core-Collapse Supernova Simulations with 160 Isotopic Species Evolved to Shock Breakout
• PUSHing core-collapse supernovae to explosions in spherical symmetry IV: Explodability, remnant properties and nucleosynthesis yields of low metallicity stars
• Uncertainties in Supernova Yields I: 1D Explosions
• The Essential Character of the Neutrino Mechanism of Core-Collapse Supernova Explosions
• The AMBRE project: Iron-peak elements in the solar neighbourhood
• Proto-neutron star evolution with improved charged-current neutrino-nucleon interactions
• The Galactic evolution of phosphorus
• Three-dimensional simulation of a core-collapse supernova for a binary star progenitor of SN 1987A
• Explosion mechanism of core-collapse supernovae: role of the Si/O interface
• Origin of neutron capture elements with the Gaia-ESO survey: the evolution of s- and r-process elements across the Milky Way
• Magnetorotational core collapse of possible GRB progenitors. IV. A wider range of progenitors
• Three-Dimensional Hydrodynamic Simulations of Convective Nuclear Burning In Massive Stars Near Iron Core Collapse
• Simulations of the Early Post-Bounce Phase of Core-Collapse Supernovae in Three-Dimensional Space with Full Boltzmann Neutrino Transport
• 3D Simulations of Strongly Magnetised Non-Rotating Supernovae: Explosion Dynamics and Remnant Properties
• Post-shock-revival evolutions in the neutrino-heating mechanism of core-collapse supernovae
• Milky Way's Thick and Thin disk: Is there distinct thick disk?
• Connecting the Light Curves of Type IIP Supernovae to the Properties of their Progenitors
• Gravitational Wave Signals from Two-Dimensional Core-Collapse Supernova Models with Rotation and Magnetic Fields
• Three-dimensional Hydrodynamics Simulations of Precollapse Shell Burning in the Si- and O-rich Layers
• The contribution from rotating massive stars to the enrichment in Sr and Ba of the Milky Way
• Post-explosion evolution of core-collapse supernovae
• Core-collapse supernova simulations with reduced nucleosynthesis networks
• Tracer particles for core-collapse supernova nucleosynthesis: The advantages of moving backward
• A Force Explosion Condition for Spherically Symmetric Core-collapse Supernovae
• Parameterisations of thermal bomb explosions for core-collapse supernovae and 56Ni production
• Effects of Different Closure Choices in Core-Collapse Supernova Simulations
• The effects of rotation, metallicity and magnetic field on the islands of failed supernovae

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