Using failed supernovae to constrain the Galactic r-process element production
arXiv:1908.05617 · doi:10.1093/mnras/stz1310
Abstract
Rapid neutron capture process (r-process) elements have been detected in a large fraction of metal-poor halo stars, with abundances relative to iron (Fe) that vary by over two orders of magnitude. This scatter is reduced to less than a factor of 3 in younger Galactic disc stars. The large scatter of r-process elements in the early Galaxy suggests that the r-process is made by rare events, like compact binary mergers and rare sub-classes of supernovae. Although being rare, neutron star mergers alone have difficulties to explain the observed enhancement of r-process elements in the lowest metallicity stars compared to Fe. The supernovae producing the two neutron stars already provide a substantial Fe abundance where the r-process ejecta from the merger would be injected. In this work we investigate another complementary scenario, where the r-process occurs in neutron star-black hole mergers in addition to neutron star mergers. Neutron star-black hole mergers would eject similar amounts of r-process matter as neutron star mergers, but only the neutron star progenitor would have produced Fe. Furthermore, a reduced efficiency of Fe production from single stars significantly alters the age-metallicity relation, which shifts the onset of r-process production to lower metallicities. We use the high-resolution [(20 pc)3/cell] inhomogeneous chemical evolution tool `ICE' to study the outcomes of these effects. In our simulations, an adequate combination of neutron star mergers and neutron star-black hole mergers qualitatively reproduces the observed r-process abundances in the Galaxy.
References in corpus (117)
- GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral
- The Global Schmidt Law in Star Forming Galaxies
- Multi-messenger Observations of a Binary Neutron Star Merger
- Gravitational Waves and Gamma-rays from a Binary Neutron Star Merger: GW170817 and GRB 170817A
- How Massive Single Stars End their Life
- Simulating Galaxy Formation with the IllustrisTNG Model
- Nucleosynthesis in Chandrasekhar Mass Models for Type Ia Supernovae and Constraints on Progenitor Systems and Burning-Front Propagation
- Stellar Multiplicity
- Origin of the heavy elements in binary neutron-star mergers from a gravitational wave event
- Core-Collapse Supernovae from 9 to 120 Solar Masses Based on Neutrino-powered Explosions
- The Electromagnetic Counterpart of the Binary Neutron Star Merger LIGO/VIRGO GW170817. II. UV, Optical, and Near-IR Light Curves and Comparison to Kilonova Models
- The r-process of stellar nucleosynthesis: Astrophysics and nuclear physics achievements and mysteries
- The s Process: Nuclear Physics, Stellar Models, Observations
- The Universal Stellar Mass-Stellar Metallicity Relation for Dwarf Galaxies
- The Emergence of a Lanthanide-Rich Kilonova Following the Merger of Two Neutron Stars
- Density Perturbations and Black Hole Formation in Hybrid Inflation
- Nucleosynthesis and Remnants in Massive Stars of Solar Metallicity
- Double Compact Objects I: The Significance Of The Common Envelope On Merger Rates
- Formation of Double Neutron Star Systems
- Gusty, gaseous flows of FIRE: galactic winds in cosmological simulations with explicit stellar feedback
- Production of all the r-process nuclides in the dynamical ejecta of neutron star mergers
- Comprehensive nucleosynthesis analysis for ejecta of compact binary mergers
- 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
- On the astrophysical robustness of neutron star merger r-process
- The Combined Ultraviolet, Optical, and Near-Infrared Light Curves of the Kilonova Associated with the Binary Neutron Star Merger GW170817: Unified Data Set, Analytic Models, and Physical Implications
- The Electromagnetic Counterpart of the Binary Neutron Star Merger LIGO/VIRGO GW170817. IV. Detection of Near-infrared Signatures of r-process Nucleosynthesis with Gemini-South
- Systematics of dynamical mass ejection, nucleosynthesis, and radioactively powered electromagnetic signals from neutron-star mergers
- Neutron-Capture Elements in the Early Galaxy: Insights from a Large Sample of Metal-Poor Giants
- Magnetorotationally driven Supernovae as the origin of early galaxy -process elements?
- Three-dimensional delayed-detonation models with nucleosynthesis for Type Ia supernovae
- VLT/UVES Abundances in Four Nearby Dwarf Spheroidal Galaxies: I. Nucleosynthesis and Abundance Ratios
- The Hamburg/ESO R-process Enhanced Star survey (HERES) II. Spectroscopic analysis of the survey sample
- Progenitor-Explosion Connection and Remnant Birth Masses for Neutrino-Driven Supernovae of Iron-Core Progenitors
- A Search for Stars of Very Low Metal Abundance. VI. Detailed Abundances of 313 Metal-Poor Stars
- Physics of Core-Collapse Supernovae in Three Dimensions: a Sneak Preview
- The nucleosynthesis of Al26 and Fe60 in solar metallicity stars extending in mass from 11 to 120 Msun: the hydrostatic and explosive contributions
- The Stellar Abundances for Galactic Archeology (SAGA) Database - Compilation of the Characteristics of Known Extremely Metal-Poor Stars
- Perspectives on Core-Collapse Supernova Theory
- R-process enrichment from a single event in an ancient dwarf galaxy
- A two-parameter criterion for classifying the explodability of massive stars by the neutrino-driven mechanism
- Collapsars as a major source of r-process elements
- The Rise of the s-Process in the Galaxy
- Neutron star mergers versus core-collapse supernovae as dominant r-process sites in the early Galaxy
- Neutron Star Mergers and Nucleosynthesis of Heavy Elements
- Kilonova from post-merger ejecta as an optical and near-infrared counterpart of GW170817
- First Stars VIII -- Enrichment of the neutron-capture elements in the early Galaxy
- On Variations in the Peak Luminosity of Type Ia Supernovae
- Galactic Chemical Evolution and solar s-process abundances: dependence on the 13C-pocket structure
- A large scale dynamo and magnetoturbulence in rapidly rotating core-collapse supernovae
- The long-term evolution of neutron star merger remnants - I. The impact of r-process nucleosynthesis
- Magnetorotational Core-Collapse Supernovae in Three Dimensions
- The rates of Type Ia Supernovae. I. Analytical Formulations
- Very low metallicity massive star models: Pre-SN evolution and primary nitrogen production
- Chemodynamical Simulations of the Milky Way Galaxy
- Neutron Star Mergers Might not be the Only Source of r-Process Elements in the Milky Way
- Nucleosynthesis in Early Supernova Winds II: The Role of Neutrinos
- A high resolution VLT/FLAMES study of individual stars in the centre of the Fornax dwarf spheroidal galaxy
- Composition of the Innermost Core Collapse Supernova Ejecta
- Impact of ejecta morphology and composition on the electromagnetic signatures of neutron star mergers
- The Chemical Evolution of the Draco Dwarf Spheroidal Galaxy
- Double neutron stars: merger rates revisited
- Advanced burning stages and fate of 8-10 Mo stars
- The Role of Fission in Neutron Star Mergers and its Impact on the r-Process Peaks
- GRB110721A: An extreme peak energy and signatures of the photosphere
- 'Sculptor'-ing the Galaxy? The Chemical Compositions of Red Giants in the Sculptor Dwarf Spheroidal Galaxy
- The rp-Process in Neutrino-driven Winds
- Galactic evolution of rapid neutron capture process abundances: the inhomogeneous approach
- The intermediate r-process in core-collapse supernovae driven by the magneto-rotational instability
- Chemistry of the Sagittarius Dwarf Galaxy: a Top-Light IMF, Outflows and the R-Process
- From Nuclei to the Cosmos: Tracing Heavy-Element Production with the Oldest Stars
- Europium production: neutron star mergers versus core-collapse supernovae
- The Ubiquity of the Rapid Neutron-Capture Process
- The r-process in proto-neutron-star wind revisited
- The first direct double neutron star merger detection: implications for cosmic nucleosynthesis
- Neutron Star Mergers as sites of r-process Nucleosynthesis and Short Gamma-Ray Bursts
- Galactic r-process enrichment by neutron star mergers in cosmological simulations of a Milky Way-mass galaxy
- Neutrino-driven wind simulations and nucleosynthesis of heavy elements
- Massive double compact object mergers: gravitational wave sources and r-process-element production sites
- Stellar evolution with rotation XIII: Predicted GRB rates at various Z
- The -Process Alliance: First Release from the Southern Search for -Process-Enhanced Stars in the Galactic Halo
- The History of R-Process Enrichment in the Milky Way
- Explosive Nucleosynthesis in Near-Chandrasekhar Mass White Dwarf Models for Type Ia Supernovae: Dependence on Model Parameters
- The role of neutron star mergers in the chemical evolution of the Galactic halo
- Nucleosynthesis in the Hot Convective Bubble in Core-Collapse Supernovae
- Crucial Physical Dependencies of the Core-Collapse Supernova Mechanism
- PUSHing Core-Collapse Supernovae to Explosions in Spherical Symmetry III: Nucleosynthesis Yields
- The Stellar Abundances for Galactic Archaeology (SAGA) Database II - Implications for Mixing and Nucleosynthesis in Extremely Metal-Poor Stars and Chemical Enrichment of the Galaxy
- Pushing 1D CCSNe to explosions: model and SN 1987A
- Enrichment of r-process elements in dwarf spheroidal galaxies in chemo-dynamical evolution model
- Neutron Star Mergers as the Origin of r-Process Elements in the Galactic Halo Based on the Sub-halo Clustering Scenario
- The extremely low-metallicity tail of the Sculptor dwarf spheroidal galaxy
- Advanced LIGO Constraints on Neutron Star Mergers and R-Process Sites
- The Diversity of Kilonova Emission in Short Gamma-Ray Bursts
- Neutron-Capture Nucleosynthesis in the First Stars
- PUSHing Core-Collapse Supernovae to Explosions in Spherical Symmetry II: Explodability and Global Properties
- -Process Nucleosynthesis from Three-dimensional Jet-driven Core-Collapse Supernovae with Magnetic Misalignments
- Metallicity effect in multi-dimensional SNIa nucleosynthesis
- The Stellar Abundances for Galactic Archaeology (SAGA) Database III - Analysis of Enrichment Histories for Elements and Two Modes of Star Formation during the Early Evolution of Milky Way
- Distinguishing the nature of comparable-mass neutron star binary systems with multimessenger observations: GW170817 case study
- Nucleosynthesis in Magnetically Driven Jets from Collapsars
- The Origins of Two Classes of Carbon-Enhanced, Metal-Poor Stars
- HST Measurements of the Expansion of NGC 6543: Parallax Distance and Nebular Evolution
- Nine New Metal-Poor Stars on the Subgiant and Red Horizontal Branches with High Levels of r-process Enhancement
- A new Fokker-Planck approach for relaxation-driven evolution of galactic nuclei
- Metallicity as a source of dispersion in the SNIa bolometric light curve luminosity-width relationship
- The Neutrino Signal in Stellar Core Collapse and Postbounce Evolution
- Unraveling the Helix Nebula: Its Structure and Knots
- Galactic Simulations of r-process Elemental Abundances
- GW170817/GRB 170817A/AT2017gfo association: some implications for physics and astrophysics
- Contribution of Neutron Star Mergers to the R-process Chemical Evolution in the Hierarchical Galaxy Formation
- On the maximum magnetic field amplification by the magnetorotational instability in core-collapse supernovae
- Core collapse with magnetic fields and rotation
- Stochastic Chemical Evolution of Galactic Subhalos and the Origin of r-Process Elements
- The Evolution and Impacts of Magnetorotational Instability in Magnetized Core-Collapse Supernovae
- The Nature of the Red Giant Branches in the Ursa Minor and Draco Dwarf Spheroidal Galaxies
- Nucleosynthesis of Fe60 in massive stars
Cited by in corpus (25)
- Origin of the Heaviest Elements: the Rapid Neutron-Capture Process
- Numerical Relativity Simulations of the Neutron Star Merger GW170817: Long-Term Remnant Evolutions, Winds, Remnant Disks, and Nucleosynthesis
- Chemical evolution with rotating massive star yields II. A new assessment of the solar s- and r- process components
- Axisymmetric Radiative Transfer Models of Kilonovae
- Neutron star mergers and rare core-collapse supernovae as sources of r-process enrichment in simulated galaxies
- Is GW190425 consistent with being a neutron starblack hole merger?
- The R-Process Alliance: Abundance Universality among Some Elements at and between the First and Second R-Process Peaks
- Correlations of r-Process Elements in Very Metal-Poor Stars as Clues to their Nucleosynthesis Sites
- Simulating Metal Mixing of Both Common and Rare Enrichment Sources in a Low Mass Dwarf Galaxy
- Common envelope jets supernova r-process yields can reproduce abundance evolution in the Galaxy
- QCD phase transition drives supernova explosion of a very massive star
- Neutron Star Mergers as the Main Source of R-process: Natal Kicks And Inside-Out Evolution to The Rescue
- Inhomogeneous enrichment of radioactive nuclei in the Galaxy: Deposition of live Mn-53, Fe-60, Hf-182, and Pu-244 into deep-sea archives. Surfing the wave?
- Enrichment of the Galactic disc with neutron-capture elements: Mo and Ru
- The chemical evolution of the solar neighbourhood for planet-hosting stars
- Observational constraints on the origin of the elements. VI. Origin and evolution of neutron-capture elements as probed by the Gaia-ESO survey
- Neutron-capture elements in dwarf galaxies III: A homogenized analysis of 13 dwarf spheroidal and ultra-faint galaxies
- r-Process enrichment in the Galactic halo characterized by nucleosynthesis variation in the ejecta of coalescing neutron star binaries
- Primordial black-hole formation and heavy r-process element synthesis from the cosmological QCD transition. Two aspects of an inhomogeneous early Universe
- The neutron-capture and alpha-elements abundance ratios scatter in old stellar populations. Cosmological simulations of the stellar halo
- Recent Advances in Understanding R-Process Nucleosynthesis in Metal-Poor Stars and Stellar Systems
- The R-Process Alliance: Hunting for gold in the near-UV spectrum of 2MASS J05383296-5904280
- Galactic chemical evolution with the short-lived isotopes Mn-53, Fe-60, Hf-182, and Pu-244
- Th/Eu abundance ratio of red giants in the Kepler Field
- Universality and variability of the heavy r-process element abundance pattern from a nonequilibrium approach