Presupernova evolution and explosive nucleosynthesis of rotating massive stars in the metallicity range -3 <=[Fe/H]<= 0

Abstract

We present a new grid of presupernova models of massive stars extending in mass between 13 and 120 Msun, covering four metallicities (i.e. [Fe/H]=0, -1, -2 and -3) and three initial rotation velocities (i.e. 0, 150 and 300 km/s). The explosion has been simulated following three different assumptions in order to show how the yields depend on the remnant mass - initial mass relation. An extended network from H to Bi is fully coupled to the physical evolution of the models. The main results can be summarized as follows. a) At solar metallicity the maximum mass exploding as Red Super Giant (RSG) is of the order of 17 Msun in the non rotating case, all the more massive stars exploding as WR stars. All rotating models, vice versa, explode as Wolf-Rayet (WR) stars. b) The interplay between the core He burning and the H burning shell, triggered by the rotation induced instabilities, drives the synthesis of a large primary amount of all the products of the CNO, not just N14. A fraction of them enriches enormously the radiative part of the He core (and is responsible of the large production of F) and a fraction enters the convective core leading therefore to an important primary neutron flux able to synthesize heavy nuclei up to Pb. c) In our scenario, remnant masses of the order of those inferred by the first detections of the gravitational waves (GW150914, GW151226, GW170104, GW170814) are predicted at all metallicities for none or moderate initial rotation velocities.

245 pages, 31 tables, 38 figures. Submitted to ApJS

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• The s process in massive stars, a benchmark for neutron capture reaction rates
• Abundance of zirconium in the globular cluster 47 Tuc: a possible Zr-Na correlation?
• The $\gamma$-process nucleosynthesis in core-collapse supernovae II. Effect of the explosive recipe
• Close binary evolution based on Gaia DR2: the origin of late WC-type Wolf-Rayet stars with low luminosity
• Chemical evolution imprints in the rare isotopes of nearby M dwarfs
• Parameter Distributions of Binary Black Hole Mergers Near Supermassive Black Holes as Seen by Advanced Gravitational Wave Detectors
• Galaxy Formation and Symbiotic Evolution with the Inter-Galactic Medium in the Age of ELT-ANDES
• Theoretical Distributions of Short-Lived Radionuclides for Star Formation in Molecular Clouds
• Massive stars in the young cluster VVV CL074
• Constraints on key ${}^{17}$O($\alpha ,\gamma$)${}^{21}$Ne resonances and impact on the weak s-process
• Using chemical evolution models of the Milky Way disk to constrain Type Ia supernova progenitors
• Hydrogen-free Wolf-Rayet stars: Helium stars with envelope-inflation structure and rotation
• On the Contribution of Very Massive Stars to the Sulfur Abundance in Star-Forming Galaxies: the Role of PISN
• Exploring fluorine chemical evolution in the Galactic disk: the open cluster perspective
• Nucleosynthesis in early rotating massive stars and chemical composition of CEMP stars
• Impact of Newly Measured Nuclear Reaction Rates on ${}^{26}$Al Ejected Yields from Massive Stars
• Neutron-Capture Element Signatures in Globular Clusters: Insights from the Gaia-ESO Survey
• Shaping Galactic Habitability: the impact of stellar migration and gas giants
• The drastic impact of Eddington-limit induced mass ejections on massive star populations
• The ALPINE-ALMA [CII] Survey: Unveiling the baryon evolution in the ISM of $z\sim 5$ star-forming galaxies
• Dating N loud AGNs at high redshift: GS3073 as a snapshot of wCen like evolution of a nuclear star cluster
• Explosive Nucleosynthesis: What we learned and what we still do not understand
• A Systematic Observational Study on Galactic Interstellar Ratio 18O/17O. II. C18O and C17O J=2-1 Data Analysis
• Heavy element contributions of rotating massive stars to Interstellar Medium
• Exploring the Stellar Rotation of Early-type Stars in the LAMOST Medium-resolution Survey. III. Evolution
• The origin of elements: the need for UV spectra
• Abundances of disk and bulge giants from high-resolution optical spectra V. Molybdenum -- the p-process element
• Chlorine and Potassium Enrichment in the Cassiopeia A Supernova Remnant
• Magnesium isotope ratios in Milky Way and dwarf galaxy stars
• Binary stellar evolution yields in galactic chemical evolution calculations
• Gamma-ray line emission from the Local Bubble
• Silicon Isotopic Composition of Mainstream Presolar SiC Grains Revisited: The Impact of Nuclear Reaction Rate Uncertainties
• Evolving massive stars to core collapse with GENEC: Extension of equation of state, opacities and effective nuclear network
• Wolf-Rayet -- compact object binaries as progenitors of binary compact objects
• The structure and evolution of a high-mass stellar merger in the Hertzsprung gap
• The multi-zone chemical evolution of the Galactic bulge: predicting abundances for different radial zones
• Abundance of barium in the atmospheres of red giants in the Galactic globular cluster NGC 104 (47 Tuc)
• The neutron-capture and alpha-elements abundance ratios scatter in old stellar populations. Cosmological simulations of the stellar halo
• Assessing stellar yields in Galaxy chemical evolution: observational stellar abundance patterns
• The SPAr burning: proton captures powering carbon-oxygen shell mergers in massive stars
• Rubidium abundances in solar metallicity stars
• Yields from massive stars in binaries. Chemical evolution of the Milky Way disk
• A constant upper luminosity limit of cool supergiant stars down to the extremely low metallicity of I Zw 18
• Chandra X-ray Measurement of Heavy Element Abundances of Wolf-Rayet Stars in the Galactic Center
• Chemical evolution of close massive binaries -- tidally-enhanced or tidally-suppressed mixing?
• The Missing Link: Testing Galactic Chemical Evolution Models with the First Multi-Isotopic Abundances in Solar Twin Stars
• Fluorine abundances in CEMP stars at the lowest metallicity: Hints on the nature of the first stars
• Aluminium-26 production in low- and intermediate-mass binary systems
• Production of heavy $\alpha$-elements and ${}^{44}$Ti in Cas A: comparison to abundances from 1D core-collapse supernova models and evidence for Carbon-Oxygen shell mergers
• Nitrogen enhancement of GN-z11 by metal pollution from supermassive stars
• Radioactive Decay
• Modelling the chemical evolution of the Milky Way
• The chemical DNA of the Magellanic Clouds V. R-process dominates neutron capture elements production in the oldest SMC stars
• Aeos: The Impact of Population III Initial Mass Function and Star-by-Star Models in Galaxy Simulations
• The metal-poorest tail of the Galactic halo: hypothesis on its origin from precise spectral analysis
• The impact of rare events on the chemical enrichment in dwarf galaxies
• Abundance of strontium in the Galactic globular cluster 47 Tuc
• Predicting interstellar radiation fields from chemical evolution models
• Stellar population modelling of neutron stars and black holes: spatially-resolved graveyards in MaNGA/SDSS-IV galaxies
• Self-consistent Conditions for ${}^{26}$Al Injection into Protosolar Disk from a Nearby Supernova
• MUSEQuBES: Physical conditions, origins, and multi-element abundances of the circumgalactic medium of an isolated, star-forming dwarf galaxy at z=0.57
• A Sequoia stellar candidate with very high 7Li and 9Be
• Unveiling the nature of the unidentified gamma-ray sources 4FGL J1908.6+0915e, HESS J1907+089/HOTS J1907+091, and 3HWC J1907+085 in the sky region of the magnetar SGR 1900+14
• Impact of the latest 22Ne+α reaction rates on nucleosynthesis in massive stars and galactic chemical evolution
• The influence of rotation and metallicity on the explodability of massive stars
• Nuclear astrophysics
• Revisiting the Perseus Cluster II: Metallicity-Dependence of Massive Stars and Chemical Enrichment History
• Two faces of Gaia-Sausage-Enceladus: Mining the chemical abundance space with graph attention networks
• Testing Evolutionary Models with Red Supergiant and Wolf-Rayet Populations
• The impact of new ($\alpha$, n) reaction rates on the weak s-process in metal-poor massive stars
• A statistical method for the identification of stars enriched in neutron-capture elements from medium-resolution spectra
• Cosmic Radioactivity and Galactic Chemical Evolution
• The impact of metallicity-dependent dust destruction on the dust-to-metals ratio in galaxies
• Deviations from the universal Initial Mass Function in binary star clusters
• A Near-Infrared and Optical Study of NGC 5822: An Open Cluster Hosting Barium-stars and Lithium-Enriched Giant Stars
• Quantifying Element Importance for Mass Recovery from Population III Supernova Yield Fits
• Oxygen and silicon abundances in Cygnus OB2: Chemical homogeneity in a sample of OB slow rotators
• Modeling the outcome of supernova explosions in binary population synthesis using the stellar compactness
• Primordial helium-3 redux: The helium isotope ratio of the Orion nebula
• An ancient system hidden in the Galactic plane?
• Barium lines in high-quality spectra of two metal-poor giants in the Galactic halo
• A non-uniform metal distribution in the ram-pressure stripped circumgalactic medium of M86
• Gas and dust from extremely metal-poor AGB stars
• Modeling the Remnants of Core-collapse Supernovae from Luminous Blue Variable stars
• UVES analysis of red giants in the bulge globular cluster NGC 6522
• Search for Axion-Like Particles from Nearby Pre-Supernova Stars
• A two-step strategy to identify episodic sources of gravitational waves and high energy neutrinos in starburst galaxies
• EDGE-INFERNO: How chemical enrichment assumptions impact the individual stars of a simulated ultra-faint dwarf galaxy
• The Two-infall Model Revisited: Constraints on Milky Way Bulge Assembly from >30,000 Galactic Chemical Evolution Models and Machine Learning
• Astrophysical Black holes: An Explanation for the Galaxy Quenching
• The chemical DNA of the Magellanic Clouds VI. Origin and evolution of neutron-capture elements in the SMC
• Observational constraints on the origin of the elements. X. Combining NLTE and machine learning for chemical diagnostics of 4 million stars in the 4MIDABLE-HR survey
• The Impact of the New ${}^{59}$Fe Decay Rates on ${}^{60}$Fe and ${}^{26}$Al Nucleosynthesis in Massive Stars
• Discovery of sulfur oxides in the ejecta of a B[e] supergiant