Nucleosynthesis Yields of Core-Collapse Supernovae and Hypernovae, and Galactic Chemical Evolution

Abstract

We present new nucleosynthesis yields as functions of the stellar mass, metallicity, and explosion energy (corresponding to normal supernovae and Hypernovae). We apply the results to the chemical evolution of the solar neighborhood. Our new yields are based on the new developments in the observational/theoretical studies of supernovae (SNe) and extremely metal-poor (EMP) stars in the halo, which have provided excellent opportunities to test the explosion models and their nucleosynthesis. We use the light curve and spectra fitting of individual SN to estimate the mass of the progenitor, explosion energy, and produced 56Ni mass. Comparison with the abundance patterns of EMP stars has made it possible to determine the model parameters of core-collapse SNe, such as mixing-fallback parameters. More specifically, we take into account the two distinct new classes of massive SNe: 1) very energetic Hypernovae, whose kinetic energy (KE) is more than 10 times the KE of normal core-collapse SNe, and 2) very faint and low energy SNe (Faint SNe). These two new classes of SNe are likely to be ``black-hole-forming'' SNe with rotating or non-rotating black holes. Nucleosynthesis in Hypernovae is characterized by larger abundance ratios (Zn,Co,V,Ti)/Fe and smaller (Mn,Cr)/Fe than normal SNe, which can explain the observed trends of these ratios in EMP stars. Nucleosynthesis in Faint SNe is characterized by a large amount of fall-back, which explains the abundance pattern of the most Fe-poor stars. These comparisons suggest that black-hole-forming SNe made important contributions to the early Galactic (and cosmic) chemical evolution.

To appear in Nuclear Physics A (Special Issue on Nuclear Astrophysics) eds. K. Langanke, F.-K. Thielemann, & M. Wiescher (2006), 36 pages

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• Massive Stars and their Supernovae
• Cosmological evolution of the Nitrogen abundance
• Nuclear Star Clusters in Cosmological Simulations
• The Mean Absorption Line Spectra of a Selection of Luminous z~6 Lyman Break Galaxies
• Progenitors and Explosion Properties of Supernova Remnants Hosting Central Compact Objects: I. RCW 103 Associated with the Peculiar Source 1E 161348-5055
• Mixing of Primordial Gas in Lyman Break Galaxies
• Elliptical Galaxy in the Making: The Dual Active Galactic Nuclei and Metal-enriched Halo of Mrk 273
• A Model for Clumpy Self-Enrichment in Globular Clusters
• The Hamburg/ESO R-process Enhanced Star survey (HERES) VI. The Galactic Chemical Evolution of Silicon
• Evolution of Neutral Oxygen During the Epoch of Reionization and its Use in Estimating the Neutral Hydrogen Fraction
• Extreme r-process enhanced stars at high metallicity in Fornax
• Observational constraints on the origin of the elements. V. Non-LTE abundance ratios of [Ni/Fe] in Galactic stars and enrichment by sub-Chandrasekhar mass SNe
• The GALAH survey: Chemical homogeneity of the Orion complex
• Enrichment by Extragalactic First Stars in the Large Magellanic Cloud
• Reaction Rate Sensitivity of the Production of $\gamma$-ray Emitting Isotopes in Core-Collapse Supernova
• On the radial profile of gas-phase Fe/α ratio around distant galaxies
• Diffraction-limited Subaru imaging of M82: sharp mid-infrared view of the starburst core
• Metallicity of the Fossil Group NGC 1550 Observed with Suzaku
• The Cosmic Evolution of Magnesium Isotopes
• Dust formation in embryonic pulsar-aided supernova remnants
• A New Chemical Evolution Model for Dwarf Spheroidal Galaxies based on Observed Long Star Formation Histories
• SIMBA-C: An updated chemical enrichment model for galactic chemical evolution in the SIMBA simulation
• Post-explosion evolution of core-collapse supernovae
• Evidences of extragalactic origin and planet engulfment in the metal-poor twin pair HD 134439/HD 134440
• Stellar Core Collapse with Hadron-Quark Phase Transition
• Chemical abundances in the metal-intermediate GC NGC 6723
• The g-mode Excitation in the Proto Neutron Star by the Standing Accretion Shock Instability
• The Expansion of the Forward Shock of 1E 0102.2-7219 in X-rays
• On the Number of Stars in the Sun's Birth Cluster
• SN 2015as: A low luminosity Type IIb supernova without an early light curve peak
• Aligned metal absorbers and the ultraviolet background at the end of reionization
• Nucleosynthesis in neutrino-driven winds in hypernovae
• Scientific Objectives of the Hot Universe Baryon Surveyor (HUBS) Mission
• Is the metallicity of their hosts a good measure of the metallicity of Type Ia supernovae?
• Hitomi Observations of the LMC SNR N132D: Highly Redshifted X-ray Emission from Iron Ejecta
• Analysis of XMM-Newton Observations of Supernova Remnant W49B and Clues to the Progenitor
• External Enrichment of Minihalos by the First Supernovae
• Spatially Resolved Chandra Spectroscopy of the Large Magellanic Cloud Supernova Remnant N132D
• An X-ray study of the galactic-scale starburst-driven outflow in NGC 253
• Exploring Simulated Early Star Formation in the Context of the Ultrafaint Dwarf Galaxies
• A Spallation Model for the Titanium-rich Supernova Remnant Cassiopeia A
• Massive High-Redshift Quiescent Galaxies With JWST
• Chromospheric Models and the Oxygen Abundance in Giant Stars
• Ideal Engine Durations For Gamma-Ray-Burst-Jet Launch
• GEMINI 3D spectroscopy of BAL+IR+Fe II QSOs: II. IRAS 04505-2958 an explosive QSO with hypershell and a new scenario for galaxy formation and galaxy end
• Broad-Lined Supernova 2016coi with Helium Envelope
• Direct-collapse black hole formation induced by internal radiation of host halos
• Chemical enrichment in the cool core of the Centaurus cluster of galaxies
• The Origin of the Young Pulsar PSR J0826+2637 and Its Possible Former Companion HIP 13962
• A high-precision abundance analysis of the nuclear benchmark star HD 20
• The Cosmic Ultraviolet Baryon Survey (CUBS) II: Discovery of an H${}_2$-Bearing DLA in the Vicinity of an Early-Type Galaxy at z = 0.576
• Inferring the velocity of early massive stars from the abundances of extremely metal-poor stars
• A Nucleosynthetic Origin for the Southwestern Fe-rich Structure in Kepler's Supernova Remnant
• A Detailed Archival CHANDRA Study of the Young Core-Collapse Supernova Remnant 1E 0102.2-7219 in the Small Magellanic Cloud
• Nucleosynthesis in Primordial Hypernovae
• Spatially Resolved X-ray Spectroscopy of Kepler's Supernova Remnant: Distinct Properties of the Circumstellar Medium and the Ejecta
• Chlorine Abundances in Cool Stars
• The chemical composition of red giants in 47 Tucanae. II. Magnesium isotopes and pollution scenarios
• The effects of local stellar radiation and dust depletion on non-equilibrium interstellar chemistry
• Constraining the final fates of massive stars by oxygen and iron enrichment history in the Galaxy
• Type IIP Supernova Progenitors and their explodability I: Convective Overshoot, Blue Loops and Surface Composition
• The Manhattan Suite: Accelerated galaxy evolution in the early Universe
• A strong neutron burst in jet-like supernovae of spinstars
• A Glimpse of the Stellar Populations and Elemental Abundances of Gravitationally Lensed, Quiescent Galaxies at $z\gtrsim 1$ with Keck Deep Spectroscopy
• An XMM-Newton X-ray View of Supernova Remnant W49B: Revisiting its Recombining Plasmas and Progenitor Type
• The metal contents of two groups of galaxies
• Suzaku X-ray observations of the mixed-morphology supernova remnant CTB 1
• The effects of binary stars on galaxies and metal-enriched gas during reionization
• Suzaku Observation of the Metallicity Distribution in the Elliptical Galaxy NGC 4636
• Abundance Patterns in the Interstellar Medium of the S0 Galaxy NGC 1316 (Fornax A) Revealed with Suzaku
• Spatially Resolved Gas-phase Metallicity in FIRE-2 Dwarfs: Late-Time Evolution of Metallicity Relations in Simulations with Feedback and Mergers
• A Dusty Dawn: Galactic Dust Buildup at $z\gtrsim 5$
• Neutron stars formation and Core Collapse Supernovae
• The Exceptional X-ray Evolution of SN1996cr in High Resolution
• Characterizing the Rapid Hydrogen Disappearance in SN2022crv: Evidence of a Continuum between Type Ib and IIb Supernova Properties
• Neutron Star Planets: Atmospheric processes and habitability
• Neutrino-dominated accretion flows: second nucleosynthesis factory in core-collapse supernovae and regulation of iron markets in galaxies
• Composite Stellar Populations and Element by Element Abundances in the Milky Way Bulge and Elliptical Galaxies
• The Physical Nature of Circumgalactic Medium Absorbers in Simba
• Progenitor-mass-dependent yields amplify intrinsic scatter in dwarf-galaxy elemental abundance ratios
• Distribution of Si, Fe, and Ni in the Intracluster Medium of the Coma Cluster
• Fe K and ejecta emission in SNR G15.9+0.2 with XMM-Newton
• A Deep Chandra Observation of Oxygen-Rich Supernova Remnant B0049-73.6 in the Small Magellanic Cloud
• Galactic vs. Extragalactic Origin of the Peculiar Transient SCP 06F6
• Chemical Cartography with APOGEE: Two-process Parameters and Residual Abundances for 288,789 Stars from Data Release 17
• Anisotropic neutrinos and gravitational waves from black hole neutrino-dominated accretion flows in fallback core-collapse supernovae
• Asymmetry in The Observed Metal-Rich Ejecta of Galactic Type Ia Supernova Remnant G299.2-2.9
• Four Metal-poor Stars in the Sagittarius Dwarf Spheroidal Galaxy
• Cosmic Sands: The Origin of Dusty, Star-forming Galaxies in the Epoch of Reionization
• Parameterisations of thermal bomb explosions for core-collapse supernovae and 56Ni production
• The Chemical Evolution of Iron-Peak Elements with Hypernovae
• The formation of the Milky Way halo and its dwarf satellites: a NLTE-1D abundance analysis. IV. Segue 1, Triangulum II, and Coma Berenices UFDs
• Radio confirmation of Galactic supernova remnant G308.3-1.4
• Physical Conditions of Five O VI Absorption Systems Towards PG $1522+101$
• Spatially Resolved X-ray Study of Supernova Remnant G306.3$-$0.9 with Unusually High Calcium Abundance
• A multi-wavelength study of the radio source G296.7-0.9: confirmation as a Galactic supernova remnant
• Hydrodynamic simulations of the Disk of Gas Around Supermassive black holes (HDGAS) -I; Molecular Gas Dynamics
• Connecting Primordial Star Forming Regions and Second Generation Star Formation in the Phoenix Simulations
• Chemical evolution models: GRB host identification and cosmic dust predictions
• The Circumgalactic Medium in Massive Halos
• Are the Formation and Abundances of Metal-Poor Stars the Result of Dust Dynamics?
• Metal-Poor Stars Observed with the Southern African Large Telescope II. An Extended Sample
• Empirical Constraints on Core Collapse Supernova Yields using Very Metal Poor Damped Lyman Alpha Absorbers
• Spatial Distribution of Abundance Patterns in the Starburst Galaxy NGC 3079 Revealed with Chandra and Suzaku
• A Monte Carlo based simulation of the galactic chemical evolution of the Milky Way galaxy
• Numerical relativity simulations of black hole and relativistic jet formation
• Galactic Outflows and Evolution of the Interstellar Medium
• Metal Enrichment in the Fermi Bubbles as a Probe of Their Origin
• Mapping the Milky Way with Gaia Bp/Rp spectra I: Systematic flux corrections and atmospheric parameters for 68 million stars
• X-ray Properties of Young Early Type Galaxies: II. Abundance Ratio in the Hot ISM
• The environments and hosts of metal absorption at z>5
• The role of massive stars in galactic chemical evolution
• On the effects of microphysical grain properties on the yields of carbonaceous dust from type II SNe
• Suzaku Observation of the Metallicity in the Interstellar Medium of NGC 4258
• The Abundance Pattern of O, Ne, Mg, and Fe in the Interstellar Medium of S0 Galaxy NGC 4382 Observed with Suzaku
• Spatial Distribution of Mg-Rich Ejecta in LMC Supernova Remnant N49B
• Probing the nature of Dark Matter through the metal enrichment of the intergalactic medium
• The initial mass-remnant mass relation for core collapse supernovae
• Predictions for Complex Distributions of Stellar Elemental Abundances in Low-Mass Galaxies
• A new model for the origin of very metal poor stars and their chemical composition
• ORIGIN: Metal Creation and Evolution from the Cosmic Dawn
• The Chemical Evolution of Very Metal-Poor Damped Lyman-$\alpha$ Systems
• Investigation of the Prompt SNe Ia progenitor nature through the analysis of the chemical composition of globular clusters and circumgalactic clouds
• Nucleosynthesis Contribution of Neutrino-dominated Accretion Flows to the Chemical Evolution of Active Galactic Nuclei
• Does the chemical signature of TYC 8442-1036-1 originate from a rotating massive star that died in a faint explosion?
• Chemical diversity of gas in distant galaxies: The metal and dust enrichment and variations within absorbing galaxies
• Impact of star formation models on the growth of simulated galaxies at high redshifts
• O, Ne, Mg, and Fe Abundances in Hot X-Ray-emitting Halos of Galaxy Clusters, Groups, and Giant Early-type Galaxies with XMM-Newton RGS Spectroscopy
• Stellar population and dust extinction in an ultraluminous infrared galaxy at z=1.135
• Binary Systems of core collapse supernova polluting a giant companion
• Using chemical evolution models of the Milky Way disk to constrain Type Ia supernova progenitors
• Black hole mass function shift in proto-stellar-clusters driven by gas accretion
• Individual element sensitivity for stellar evolutionary isochrones
• Potential contributions of Pop III and intermediate-mass Pop II stars to cosmic chemical enrichment
• Be, V and Cu in the halo star CS 31082-001 from near-UV spectroscopy
• A Chandra X-ray Study of Supernova Remnant N63A in the Large Magellanic Cloud
• Timescales of Solar System Formation Based on Al-Ti Isotope Correlation by Supernova Ejecta
• A Study of the Merger History of the Galaxy Group HCG 62 Based on X-Ray Observations and SPH Simulations
• Heavy element contributions of rotating massive stars to Interstellar Medium
• A Suzaku X-ray study of the mixed-morphology supernova remnant Kes 69 and searching for its gamma-ray counterpart
• On the origin of the $10^7$ K hot emitting gas in the Circumgalactic medium of the Milky Way
• Transition Elements in Supernova Presolar Grains: Condensation vs. Implantation
• SPI Analysis and Abundance Calculations of DEM L71, and Comparison to SN explosion Models
• Large-scale geometry and topology of gas fields: Effects of AGN and stellar feedback
• Parameters of the type-IIP supernova SN 2012aw
• Impacts of Black-Hole-Forming Supernova Explosions on the Diffuse Neutrino Background
• Revisiting the Perseus Cluster I: Resolving the Si/S/Ar/Ca ratios by Stellar Convection
• The demographics of core-collapse supernovae. The role of binary evolution and CSM interaction
• Growth of Light Seed Black Holes in the Early Universe
• A theoretical color-velocity correlation for supernovae associated with gamma-ray bursts
• First Detection of Ar-K Line Emission from the Cygnus Loop
• Chemical Yields from Supernovae and Hypernovae
• Core to Cosmic Edge: SIMBA-C's New Take on Abundance Profiles in the Intragroup Medium at z = 0
• The imprint of bursty star formation on alpha-element abundance patterns in Milky Way-like galaxies
• The Origin of the Stellar Mass-Stellar Metallicity Relation in the Milky Way Satellites and beyond
• First Light: A Brief Review
• The dawn is quiet here: Rise in [$\alpha$/Fe] is a signature of massive gas accretion that fueled proto-Milky Way
• Is the stellar mass-stellar metallicity relation universal in the Milky Way satellites and beyond?
• Carbon from massive binary-stripped stars over cosmic time: effect of metallicity
• Self-Organization In Stellar Evolution: Size-Complexity Rule
• Gamma-ray line measurements from supernova explosions
• CHEERS: Future perspectives for abundance measurements in clusters with XMM-Newton
• Population III Star Formation in an X-ray background: II. Protostellar Discs, Multiplicity and Mass Function of the Stars
• Enhancing Compton telescope imaging with maximum a posteriori estimation: a modified Richardson-Lucy algorithm for the Compton Spectrometer and Imager
• Milky Way Mapper decoded abundances -- I. Shared disc enrichment patterns
• GRB 180728A and SN 2018fip: the nearest high-energy cosmological gamma-ray burst with an associated supernova
• Kennicutt-Schmidt relation of galaxies over 13 billion years in the COLIBRE hydrodynamical simulations
• MARTA: The connection between chemical enrichment, feedback, and dust in a Wolf-Rayet galaxy at z$\sim$2
• A theoretical investigation of far-infrared fine structure lines at $z>6$ and of the origin of the [OIII]88/[CII]158 enhancement
• Can supernova from runaway stars mimic the signs of absorbing `super-virial' gas?
• APEX survey of interstellar HCl: ${}^{35}$Cl/${}^{37}$Cl isotopic ratios in dense cores and outflows
• Circular polarization of gravitational waves from magnetorotational supernovae
• The Early Solar System - Chapter 6
• The timescales of chemical enrichment in the Galaxy
• Pressure-driven fragmentation of clouds at high redshift
• Nuclear Criticality as a Contributor to Gamma Ray Burst Events
• New families in our Solar neighborhood: applying Gaussian Mixture models for objective classification of structures in the Milky Way and in simulations
• Stellar population modelling of neutron stars and black holes: spatially-resolved graveyards in MaNGA/SDSS-IV galaxies
• Using CSST and ejecta-wind interaction in type II-P supernovae to constrain the wind-mass loss of red supergiant stars
• The contribution of stars, dust, neutral gas and supermassive black holes in galaxies to the cosmic baryon inventory
• Supernova Nucleosynthesis in the Early Universe
• Rapid early gas accretion for the inner Galactic disc
• Ranking Theoretical Supernovae Explosion Models from Observations of the Intracluster Gas
• First Stars -- Type Ib Supernovae Connection
• Ultraviolet Spectroscopy and TARDIS Models of the Broad-lined Type-Ic Supernova 2014ad
• Metals in the Intracluster Medium of MS 1512.4+3647 Observed with Suzaku: Implications for the Metal Enrichment History
• SNR G292.0+1.8: A Remnant of a Low-Mass Progenitor Stripped-Envelope Supernova
• Multimessenger Constraints on the Central Engine in SN 2023ixf: Neutron Star or Black Hole?
• Indicatives of Early Stages of Star Formation in the Universe
• The Connection between Gamma-Ray Bursts and Extremely Metal-Poor Stars as Nucleosynthetic Probes of the Early Universe
• Better Alternative to "Astronomical Silicate": Laboratory-Based Optical Functions of Chondritic/Solar Abundance Glass With Application to HD161796
• Metallicity Structure in Galactic Longitude-Velocity Diagrams of the Milky Way Disk and FIRE-2 Simulations
• 3D elemental abundances of stars at formation across the histories of Milky Way-mass galaxies in the FIRE simulations
• Chemical enrichment of ICM within the A3266 cluster I: radial profiles