Type Ia Supernova Nucleosynthesis: Metallicity-Dependent Yields

Abstract

Type Ia supernova explosions (SNIa) are fundamental sources of elements for the chemical evolution of galaxies. They efficiently produce intermediate-mass (with Z between 11 and 20) and iron group elements - for example, about 70% of the solar iron is expected to be made by SNIa. In this work, we calculate complete abundance yields for 39 models of SNIa explosions, based on three progenitors - a 1.4M deflagration detonation model, a 1.0 double detonation model and a 0.8 M double detonation model - and 13 metallicities, with 22Ne mass fractions of 0, 1x10-7, 1x10-6, 1x10-5, 1x10-4, 1x10-3, 2x10-3, 5x10-3, 1x10-2, 1.4x10-2, 5x10-2, and 0.1 respectively. Nucleosynthesis calculations are done using the NuGrid suite of codes, using a consistent nuclear reaction network between the models. Complete tables with yields and production factors are provided online at Zenodo: Yields. We discuss the main properties of our yields in the light of the present understanding of SNIa nucleosynthesis, depending on different progenitor mass and composition. Finally, we compare our results with a number of relevant models from the literature.

arXiv comment42 pages, 21 figures. Accepted for publication in ApJS 21-06-23

References in corpus (62)

• Modules for Experiments in Stellar Astrophysics (MESA)
• Type Ia Supernova Explosion Models
• Observational clues to the progenitors of Type-Ia supernovae
• Nucleosynthesis in Massive Stars With Improved Nuclear and Stellar Physics
• Astrophysical Reaction Rates From Statistical Model Calculations
• Shell-model calculations of stellar weak interaction rates: II. Weak rates for nuclei in the mass range A=45-65 in supernovae environment
• Three-dimensional delayed-detonation models with nucleosynthesis for Type Ia supernovae
• Double-detonation sub-Chandrasekhar supernovae: can minimum helium shell masses detonate the core?
• Sub-luminous type Ia supernovae from the mergers of equal-mass white dwarfs with M~0.9 M_sun
• Type Iax Supernovae: A New Class of Stellar Explosion
• Detonations in Sub-Chandrasekhar Mass C+O White Dwarfs
• Chemical evolution with rotating massive star yields: I. The solar neighbourhood and the s-process elements
• On Variations in the Peak Luminosity of Type Ia Supernovae
• Nucleosynthesis in Type Ia Supernovae
• Type-Ia supernova rates and the progenitor problem, a review
• Double-detonation sub-Chandrasekhar supernovae: synthetic observables for minimum helium shell mass models
• Sub-Chandrasekhar-mass white dwarf detonations revisited
• Nucleosynthesis in multi-dimensional SNIa explosions
• NuGrid stellar data set I. Stellar yields from H to Bi for stars with metallicities Z = 0.02 and Z = 0.01
• NLTE abundances of Mn in a sample of metal-poor stars
• Type Ia Supernovae: Their Origin and Possible Applications in Cosmology
• Type Ia Supernovae as Sites of p-process: Two-Dimensional Models Coupled to Nucleosynthesis
• Coulomb tunneling for fusion reactions in dense matter: Path integral Monte Carlo versus mean field
• NuGrid Stellar Data Set. II. Stellar Yields from H to Bi for Stellar Models with Mzams = 1 to 25Msun and Z = 0.0001 to 0.02
• The Role of Electron Captures in Chandrasekhar Mass Models for Type Ia Supernovae
• s-Process Nucleosynthesis in Advanced Burning Phases of Massive Stars
• Explosive Nucleosynthesis in Near-Chandrasekhar Mass White Dwarf Models for Type Ia Supernovae: Dependence on Model Parameters
• Solar abundance of manganese: a case for the existence of near Chandrasekhar-mass Type Ia supernova progenitors
• Early Blue Excess from the Type Ia Supernova 2017cbv and Implications for Its Progenitor
• New Type Ia supernova Yields and the Manganese and Nickel Problems in the Milky Way and Dwarf Spheroidal Galaxies
• The ejected mass distribution of type Ia supernovae: A significant rate of non-Chandrasekhar-mass progenitors
• Trends in Ti44 and Ni56 from Core-Collapse Supernovae
• The Effect of Different Type Ia Supernova Progenitors on Galactic Chemical Evolution
• The delay time distribution of type Ia supernovae: a comparison between theory and observation
• Metallicity effect in multi-dimensional SNIa nucleosynthesis
• Spectra of Type Ia Supernovae from Double Degenerate Mergers
• 56Ni Production in Double Degenerate White Dwarf Collisions
• Explosive Nucleosynthesis in Sub-Chandrasekhar Mass White Dwarf Models for Type Ia Supernovae: Dependence on Model Parameters
• Single Degenerate Models for Type Ia Supernovae Progenitor's Evolution and Nucleosythesis Yields
• SNe Ia from double detonations: Impact of core-shell mixing on the carbon ignition mechanism
• Sensitivity study of explosive nucleosynthesis in Type Ia supernovae: I. Modification of individual thermonuclear reaction rates
• Multi-Dimensional Parameter Study of Double Detonation Type Ia Supernovae Originating from Thin-Helium-Shell White Dwarfs
• Nucleosynthesis imprints from different Type Ia Supernova explosion scenarios and implications for galactic chemical evolution
• Sub-Chandrasekhar progenitors favoured for type Ia supernovae: Evidence from late-time spectroscopy
• Testing the role of SNe Ia for Galactic chemical evolution of p-nuclei with 2D models and with s-process seeds at different metallicities
• Manganese Indicates a Transition from Sub- to Near-Chandrasekhar Type Ia Supernovae in Dwarf Galaxies
• Observational constraints on the origin of the elements. III. Evidence for the dominant role of sub-Chandrasekhar SN Ia in the chemical evolution of Mn and Fe in the Galaxy
• Metallicity-dependent nucleosynthetic yields of Type Ia supernovae originating from double detonations of sub-M${}_{\text{Ch}}$ white dwarfs
• A Tracer Method for Computing Type Ia Supernova Yields: Burning Model Calibration, Reconstruction of Thickened Flames, and Verification for Planar Detonations
• The Effects of Variations in Nuclear Interactions on Nucleosynthesis in Thermonuclear Supernovae
• Mn abundances in the stars of the Galactic disc with metallicities -1.0 < [Fe/H] < 0.3
• Observational evidence for high neutronization in supernova remnants: implications for Type Ia supernova progenitors
• A radio-detected Type Ia supernova with helium-rich circumstellar material
• ${}^{60}$Fe in core-collapse supernovae and prospects for X-ray and $\gamma$-ray detection in supernova remnants
• A New Model for Electron-Capture Supernovae in Galactic Chemical Evolution
• Observing the metal-poor solar neighbourhood: a comparison of galactic chemical evolution predictions
• Exploring the diversity of double detonation explosions for type Ia supernovae: Effects of the post-explosion helium shell composition
• Sensitivity of Type Ia supernovae to electron capture rates
• Radioactive nuclei in the early Solar System: analysis of the 15 isotopes produced by core-collapse supernovae
• Manganese spread in Ursa Minor as a proof of sub-classes of type Ia supernovae
• Heavy Elements Nucleosynthesis On Accreting White Dwarfs: building seeds for the p-process
• Quantifying How Density Gradients and Front Curvature Affect Carbon Detonation Strength During Type Ia Supernovae

Cited by in corpus (6)

• Ultraviolet spectroscopy of the supernova Ia hypervelocity runaway white dwarf J0927-6335
• Using chemical evolution models of the Milky Way disk to constrain Type Ia supernova progenitors
• Using Binary Population Synthesis to Calculate the Yields of Low- and Intermediate-Mass Binary Populations at Low Metallicity
• Revisiting the Perseus Cluster II: Metallicity-Dependence of Massive Stars and Chemical Enrichment History
• The Two-infall Model Revisited: Constraints on Milky Way Bulge Assembly from >30,000 Galactic Chemical Evolution Models and Machine Learning
• Trans-Fe elements from Type Ia Supernovae. I. Heavy element nucleosynthesis during the formation of near-Chandrasekhar white dwarfs