Nucleosynthesis in Massive Stars With Improved Nuclear and Stellar Physics

Abstract

We present the first calculations to follow the evolution of all stable nuclei and their radioactive progenitors in stellar models computed from the onset of central hydrogen burning through explosion as Type II supernovae. Calculations are performed for Pop I stars of 15, 19, 20, 21, and 25 M_sun using the most recently available experimental and theoretical nuclear data, revised opacity tables, neutrino losses, and weak interaction rates, and taking into account mass loss due to stellar winds. A novel ``adaptive'' reaction network is employed with a variable number of nuclei (adjusted each time step) ranging from about 700 on the main sequence to more than 2200 during the explosion. The network includes, at any given time, all relevant isotopes from hydrogen through polonium (Z=84). Even the limited grid of stellar masses studied suggests that overall good agreement can be achieved with the solar abundances of nuclei between 16O and 90Zr. Interesting discrepancies are seen in the 20 M_sun model and, so far, only in that model, that are a consequence of the merging of the oxygen, neon, and carbon shells about a day prior to core collapse. We find that, in some stars, most of the ``p-process'' nuclei can be produced in the convective oxygen burning shell moments prior to collapse; in others, they are made only in the explosion. Serious deficiencies still exist in all cases for the p-process isotopes of Ru and Mo.

53 pages, 17 color figures (3 as separate GIF images), slightly extended discussion and references, accepted by ApJ

Cited by in corpus (430)

• Modules for Experiments in Stellar Astrophysics (MESA)
• MESA Isochrones and Stellar Tracks (MIST). I: Solar-Scaled Models
• Core-Collapse Supernovae from 9 to 120 Solar Masses Based on Neutrino-powered Explosions
• Pre-Supernova Evolution of Massive Single and Binary Stars
• The r-process of stellar nucleosynthesis: Astrophysics and nuclear physics achievements and mysteries
• Presupernova Evolution of Differentially Rotating Massive Stars Including Magnetic Fields
• The s Process: Nuclear Physics, Stellar Models, Observations
• Radioactive 26Al and massive stars in the Galaxy
• Nucleosynthesis Yields of Core-Collapse Supernovae and Hypernovae, and Galactic Chemical Evolution
• Nucleosynthesis and Remnants in Massive Stars of Solar Metallicity
• Nucleosynthesis and Evolution of Massive Metal-Free Stars
• Chemical enrichment in cosmological, smoothed particle hydrodynamics simulations
• Galactic Evolution of Sr, Y, Zr: A Multiplicity of Nucleosynthetic Processes
• The Birth Environment of the Solar System
• The nucleosynthesis of Al26 and Fe60 in solar metallicity stars extending in mass from 11 to 120 Msun: the hydrostatic and explosive contributions
• Type II Supernovae: Model Light Curves and Standard Candle Relationships
• The r-process nucleosynthesis in the various jet-like explosions of magnetorotational core-collapse supernovae
• Sub-Chandrasekhar Mass Models For Type Ia Supernovae
• The Remarkable Deaths of 9 - 11 Solar Mass Stars
• Galactic Chemical Evolution and solar s-process abundances: dependence on the 13C-pocket structure
• The Compactness of Presupernova Stellar Cores
• Constraining the astrophysical origin of the p-nuclei through nuclear physics and meteoritic data
• Stellar Abundances in the Solar Neighborhood: The Hypatia Catalog
• Evolution, Explosion and Nucleosynthesis of Core Collapse Supernovae
• Stellar evolution with rotation XII: Pre-supernova models
• The evolution of the Milky Way from its earliest phases : constraints on stellar nucleosynthesis
• High Resolution Study of Presupernova Compactness
• Nucleosynthesis in multi-dimensional SNIa explosions
• The Evolution of Massive Helium Stars Including Mass Loss
• Nucleosynthesis in Early Supernova Winds II: The Role of Neutrinos
• $s$-process production in rotating massive stars at solar and low metallicities
• A Simple Approach to the Supernova Progenitor-Explosion Connection
• Short-lived Nuclei in the Early Solar System: Possible AGB Sources
• NuGrid stellar data set I. Stellar yields from H to Bi for stars with metallicities Z = 0.02 and Z = 0.01
• Composition of the Innermost Core Collapse Supernova Ejecta
• Rapid formation of large dust grains in the luminous supernova SN 2010jl
• Non-standard s process in low metallicity massive rotating stars
• The s process in massive stars at low metallicity. Effect of primary N14 from fast rotating stars
• Neutrino Nucleosynthesis
• The Pair-Instability Mass Gap for Black Holes
• A stubbornly large mass of cold dust in the ejecta of Supernova 1987A
• Ab initio alpha-alpha scattering
• Galactic evolution of rapid neutron capture process abundances: the inhomogeneous approach
• Aluminum-, Calcium- And Titanium-Rich Oxide Stardust In Ordinary Chondrite Meteorites
• Neutrino-nucleus reactions and nuclear structure
• Self-consistent 3D Supernova Models From -7 Minutes to +7 Seconds: a 1-bethe Explosion of a ~19 Solar-mass Progenitor
• Type Ia Supernovae as Sites of p-process: Two-Dimensional Models Coupled to Nucleosynthesis
• Nucleosynthesis in the Innermost Ejecta of Neutrino-Drive Supernova Explosions in Two Dimensions
• Sensitivity of p-Process Nucleosynthesis to Nuclear Reaction Rates in a 25 Solar Mass Supernova Model
• 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
• Nucleosynthesis in the Early Galaxy
• Neutron-rich chromium isotope anomalies in supernova nanoparticles
• SPI observations of the diffuse 60Fe emission in the Galaxy
• Luminous Blue Variables and superluminous supernovae from binary mergers
• Different to the core: the pre-supernova structures of massive single and binary-stripped stars
• Neutron Reactions in Astrophysics
• Presolar grains from meteorites: Remnants from the early times of the solar system
• Integrated Nucleosynthesis in Neutrino Driven Winds
• Condensation of dust in the ejecta of type II-P supernovae
• Astronuclear Physics: a Tale of the Atomic Nuclei in the Skies
• Uncertainties in the nu p-process: supernova dynamics versus nuclear physics
• The signature of 44Ti in Cassiopeia A revealed by IBIS/ISGRI on INTEGRAL
• The Path to Improved Reaction Rates for Astrophysics
• Branchings in the gamma-process path revisited
• The 12C + 12C reaction and the impact on nucleosynthesis in massive stars
• On Variations Of Pre-Supernova Model Properties
• Yields of rotating stars at solar metallicity
• Radioactive nuclei from cosmochronology to habitability
• Nucleosynthesis in the Hot Convective Bubble in Core-Collapse Supernovae
• Frontiers in Nuclear Astrophysics
• Coordinated Analyses of Presolar Grains in the Allan Hills 77307 and Queen Elizabeth Range 99177 Meteorites
• The Irradiation Origin of Beryllium Radioisotopes and Other Short-lived Radionuclides
• LUNA: a Laboratory for Underground Nuclear Astrophysics
• The Chandra ACIS Survey of M33: X-ray, Optical and Radio Properties of the Supernova Remnants
• PUSHing Core-Collapse Supernovae to Explosions in Spherical Symmetry III: Nucleosynthesis Yields
• Pushing 1D CCSNe to explosions: model and SN 1987A
• The Branchings of the Main s-process: Their Sensitivity to alpha-induced Reactions on 13C and 22Ne and to the Uncertainties of the Nuclear Network
• Production of 26Al, 44Ti, and 60Fe in Core-Collapse Supernovae: Sensitivity to the Rates of the Triple Alpha and 12C(a,g)16O Reactions
• Iron-Group Abundances in the Metal-Poor Main Sequence Turnoff Star HD~84937
• Abundances of neutron-capture elements in stars of the galactic disk substructures
• Neutrino-Nucleus Reaction Cross Sections for Light Element Synthesis in Supernova Explosions
• The Uncertainties in the 22Ne + alpha-capture Reaction Rates and the Production of the Heavy Magnesium Isotopes in Asymptotic Giant Branch Stars of Intermediate Mass
• The origin of short-lived radionuclides and the astrophysical environment of solar system formation
• The chemical evolution of Barium and Europium in the Milky Way
• High angular resolution ALMA images of dust and molecules in the SN 1987A ejecta
• The production of proton-rich isotopes beyond iron: The $\gamma$ process in stars
• Intermediate Element Abundances in Galaxy Clusters
• The chemically controlled synthesis of dust in type II-P supernovae
• Millihertz Quasi-Periodic Oscillations from Marginally Stable Nuclear Burning on an Accreting Neutron Star
• Idealised hydrodynamic simulations of turbulent oxygen-burning shell convection in 4π geometry
• Type Ib Supernova 2008D associated with the Luminous X-ray Transient 080109: An Energetic Explosion of a Massive Helium Star
• Non standard s-process in massive rotating stars. Yields of $10-150$ $M_{\odot }$ models at $Z=10^{-3}$
• Evolution of Fluorine Abundances with the ν-Process
• PUSHing Core-Collapse Supernovae to Explosions in Spherical Symmetry II: Explodability and Global Properties
• Neutrino-nucleus reactions and their role for supernova dynamics and nucleosynthesis
• Alpha-induced cross sections of 106Cd for the astrophysical p-process
• The impact of fallback on the compact remnants and chemical yields of core-collapse supernovae
• Stellar origin of the 182Hf cosmochronometer and the presolar history of solar system matter
• The Slow X-Ray Expansion of the Northwestern Rim of the Supernova Remnant RX J0852.0-4622
• The light curve of SN 1987A revisited: constraining production masses of radioactive nuclides
• Possible Charge-Exchange X-Ray Emission in the Cygnus Loop Detected with Suzaku
• Phosphorus in the Young Supernova Remnant Cassiopeia A
• New estimates of the contribution of Wolf--Rayet stellar winds to the Galactic 26Al
• Large-Scale Mixing in a Violent Oxygen-Neon Shell Merger Prior to a Core-Collapse Supernova
• Automated NanoSIMS Measurements of Spinel Stardust from the Murray Meteorite
• The stellar (n,gamma) cross section of 62Ni
• On the Sensitivity of Massive Star Nucleosynthesis and Evolution to Solar Abundances and to Uncertainties in Helium Burning Reaction Rates
• Uncertainties in the production of $p$ nuclei in massive stars obtained from Monte Carlo variations
• Supernova Neutrino Nucleosynthesis of Light Elements with Neutrino Oscillations
• Nebular phase observations of the type-Ib supernova iPTF13bvn favour a binary progenitor
• On the origin of nitrogen
• Astrophysical constraints from gamma-ray spectroscopy
• The effect of 12C + 12C rate uncertainties on the evolution and nucleosynthesis of massive stars
• Constraining the Spectrum of Supernova Neutrinos from Neutrino-Process-Induced Light-Element Synthesis
• Radioactive Probes of the Supernova-Contaminated Solar Nebula: Evidence that the Sun was Born in a Cluster
• Odd p isotope 113In: Measurement of alpha-induced reactions
• Chemical evolution library for galaxy formation simulation
• New Neutron-Capture Site in Massive Pop III and Pop II Stars as a Source for Heavy Elements in the Early Galaxy
• The Supernova Triggered Formation and Enrichment of Our Solar System
• Electron-capture supernovae as sources of 60Fe
• Sensitivity study of explosive nucleosynthesis in Type Ia supernovae: I. Modification of individual thermonuclear reaction rates
• Convective-reactive nucleosynthesis of K, Sc, Cl and p-process isotopes in O-C shell mergers
• Core-collapse Supernova Explosions Driven by the Hadron-quark Phase Transition as a Rare $r$-process Site
• Implications for Post-Processing Nucleosynthesis of Core-Collapse Supernova Models with Lagrangian Particles
• An X-Ray Study of Supernova Remnant N49 and Soft Gamma-Ray Repeater 0526-66 in the Large Magellanic Cloud
• Determination of 141Pr(alpha,n)144Pm cross sections at energies of relevance for the astrophysical p-process using the gamma-gamma coincidence method
• Multimessengers from core-collapse supernovae: multidimensionality as a key to bridge theory and observation
• The s Process and Beyond
• Extremely ${}^{54}$Cr- and ${}^{50}$Ti-rich presolar oxide grains in a primitive meteorite: Formation in rare types of supernovae and implications for the astrophysical context of solar system birth
• Simultaneous Triggered Collapse of the Presolar Dense Cloud Core and Injection of Short-Lived Radioisotopes by a Supernova Shock Wave
• Astrophysical Shrapnel: Discriminating Among Near-Earth Stellar Explosion Sources of Live Radioactive Isotopes
• Nucleosynthesis in magneto-rotational supernovae
• Role of core-collapse supernovae in explaining Solar System abundances of p nuclides
• The $\nu$ process in the light of an improved understanding of supernova neutrino spectra
• On Heavy Element Enrichment in Classical Novae
• Stellar Origins of Extremely ${}^{\text{13}}C$- and ${}^{15}N$-enriched Presolar SiC Grains: Novae or Supernovae?
• Dependence of S-Process Nucleosynthesis in Massive Stars on Triple-Alpha and 12C(a,g)16O Reaction Rate Uncertainties
• 3D hydrodynamic simulations of C ingestion into a convective O shell
• Survival of Nature's Rarest Isotope 180Ta under Stellar Conditions
• PUSHing core-collapse supernovae to explosions in spherical symmetry IV: Explodability, remnant properties and nucleosynthesis yields of low metallicity stars
• Coulomb suppression of the stellar enhancement factor
• Low and intermediate mass star yields: The evolution of carbon abundances
• Matter Mixing in Aspherical Core-collapse Supernovae: Three-dimensional Simulations with Single Star and Binary Merger Progenitor Models for SN 1987A
• Injection of Short-Lived Radionuclides into the Early Solar System from a Faint Supernova with Mixing-Fallback
• Triggering Collapse of the Presolar Dense Cloud Core and Injecting Short-Lived Radioisotopes with a Shock Wave. I. Varied Shock Speeds
• Supernova Reverse Shocks and SiC Growth
• Alpha-induced reaction cross section measurements on 151Eu for the astrophysical gamma-process
• Supernova Propagation And Cloud Enrichment: A new model for the origin of ${}^{60}$Fe in the early solar system
• Uncertainties in Galactic Chemical Evolution Models
• Nucleosynthesis of Light Elements and Heavy r-Process Elements through the nu-Process in Supernova Explosion
• Uncertainties in s-process nucleosynthesis in massive stars determined by Monte Carlo variations
• Neutron capture cross section of unstable 63Ni: implications for stellar nucleosynthesis
• Direct determination of photodisintegration cross sections and the p-process
• Production of the p-Process Nuclei in the Carbon-Deflagration Model for Type Ia Supernovae
• The X-ray Afterglows of GRB 020813 and GRB 021004 with Chandra HETGS: Possible Evidence for a Supernova Prior to GRB 020813
• Contrasting copper evolution in Omega Centauri and the Milky Way
• X-ray Emitting Ejecta in Puppis A Observed with Suzaku
• Isotopic enrichment of forming planetary systems from supernova pollution
• The quest for blue supergiants: binary merger models for the evolution of the progenitor of SN 1987A
• Pulsational pair-instability supernovae: gravitational collapse, black-hole formation, and beyond
• The final core collapse of pulsational pair instability supernovae
• Production of carbon-rich presolar grains from massive stars
• Radioactive Al26 and Fe60 in the Milky Way: implications of the RHESSI detection of Fe60
• Code dependencies of pre-supernova evolution and nucleosynthesis in massive stars: Evolution to the end of core helium burning
• Testing the role of SNe Ia for Galactic chemical evolution of p-nuclei with 2D models and with s-process seeds at different metallicities
• Gamma-ray Emission of 60Fe and 26Al Radioactivities in our Galaxy
• A nearby recent supernova that ejected the runaway star zeta Oph, the pulsar PSRB1706-16, and 60-Fe found on Earth
• Uncertainties in the production of p nuclides in thermonuclear supernovae determined by Monte Carlo variations
• Cross section measurements of $\alpha$-induced reactions on ${}^{92,94}$Mo and ${}^{112}$Sn for $p$-process studies
• Proton induced reaction cross section measurements on Se isotopes for the astrophysical p process
• Are Models for Core-Collapse Supernova Progenitors Consistent with the Properties of Supernova Remnants?
• Horizons: Nuclear Astrophysics in the 2020s and Beyond
• Opportunities to constrain astrophysical reaction rates for the s-process through determination of the ground state cross sections
• Suppression of the stellar enhancement factor and the reaction 85Rb(p,n)85Sr
• Short-lived p-nuclides in the early solar system and implications on the nucleosynthetic role of X-ray binaries
• Radiogenic p-isotopes from SNIa, nuclear physics uncertainties and Galactic chemical evolution compared with values in primitive meteorites
• Deep-Ocean Crusts as Telescopes: Using Live Radioisotopes to Probe Supernova Nucleosynthesis
• Thermonuclear Bursts with Short Recurrence Times from Neutron Stars Explained by Opacity-Driven Convection
• Elastic alpha-scattering of 112Sn and 124Sn at astrophysically relevant energies
• Successful prediction of total $\alpha$-induced reaction cross sections at astrophysically relevant sub-Coulomb energies using a novel approach
• The 40Ca(alpha,gamma)44Ti reaction in the energy regime of supernova nucleosynthesis
• Molecules and dust in Cas A: I - Synthesis in the supernova phase and processing by the reverse shock in the clumpy remnant
• ALMA spectral survey of Supernova 1987A --- molecular inventory, chemistry, dynamics and explosive nucleosynthesis
• Neutrino Oscillation Effects on Supernova Light Element Synthesis
• Origin of the p-process radionuclides 92Nb and 146Sm in the early Solar System and inferences on the birth of the Sun
• Numerical studies on the link between radioisotopic signatures on Earth and the formation of the Local Bubble. I. 60Fe transport to the solar system by turbulent mixing of ejecta from nearby supernovae into a locally homogeneous ISM
• Photon-induced Nucleosynthesis: Current Problems and Experimental Approaches
• SNR-calibrated Type Ia supernova models
• Three-dimensional mixing and light curves: constraints on the progenitor of supernova 1987A
• The abundance of 36S in IRC+10216 and its production in the Galaxy
• The Gaia-ESO Survey: A new approach to chemically characterising young open clusters II. Abundances of the neutron-capture elements Cu, Sr, Y, Zr, Ba, La, and Ce
• Nucleosynthesis of binary-stripped stars
• The physics of Core-Collapse Supernovae: explosion mechanism and explosive nucleosynthesis
• The Impact of Nuclear Reaction Rate Uncertainties On The Evolution of Core-Collapse Supernova Progenitors
• Can Ejecta-Dominated Supernova Remnants be Typed from their X-ray Spectra? The Case of G337.2-0.7
• Discovery of Fast-Moving X-Ray--Emitting Ejecta Knots in the Oxygen-Rich Supernova Remnant Puppis A
• The $\nu$-process with fully time-dependent supernova neutrino emission spectra
• Pulsational Analysis of the Cores of Massive Stars and its Relevance to Pulsar Kicks
• Sensitivity of the C and O production on the 3-alpha rate
• Discovery of X-Ray-Emitting O-Ne-Mg-Rich Ejecta in the Galactic Supernova Remnant Puppis A
• ${}^{62}$Ni($n,\gamma$) and ${}^{63}$Ni($n,\gamma$) cross sections measured at n_TOF/CERN
• Mercury (Hg) in meteorites: variations in abundance, thermal release profile, mass-dependent and mass-independent isotopic fractionation
• The stellar and wind parameters of six prototypical HMXBs and their evolutionary status
• The Plasma Structure of the Cygnus Loop from the Northeastern Rim to the Southwestern Rim
• Mass Measurements of Neutron-Deficient Y, Zr, and Nb Isotopes and Their Impact on $rp$ and $\nu p$ Nucleosynthesis Processes
• Galaxy Genesis -- unravelling the epoch of dissipation in the early disk
• ${}^{60}$Fe in core-collapse supernovae and prospects for X-ray and $\gamma$-ray detection in supernova remnants
• Co-production of light p-, s- and r-process isotopes in the high-entropy wind of type II supernovae
• Challenges in nucleosynthesis of trans-iron elements
• Neutrino-Driven Explosions in GRBs and Hypernovae
• The Impact of Helium-Burning Reaction Rates on Massive Star Evolution and Nucleosynthesis
• Empirical Abundance Scaling Laws and Implications for the Gamma-Process in Core-Collapse Supernovae
• Investigation of the reaction 74Ge(p,gamma)75As using the in-beam method to improve reaction network predictions for p nuclei
• Solution of the alpha-potential mystery in the gamma-process and its impact on the Nd/Sm ratio in meteorites
• On the asymptotic giant branch star origin of peculiar spinel grain OC2
• The first direct measurement of 12C(12C,n)23Mg at stellar energies
• Solving the stellar 62Ni problem with AMS
• Silicon carbide grains of type C provide evidence for the production of the unstable isotope ${}^{32}$Si in supernovae
• Resonance analysis of ${}^{147}$Sm(n,alpha) cross sections: Comparison to optical model calculations and indications of non-statistical effects
• Coordinated Analysis of Two Graphite Grains from the CO3.0 LAP 031117 Meteorite: First Identification of a CO Nova Graphite and a Presolar Iron Sulfide Subgrain
• Fast neutrino flavor conversions in a supernova: Emergence, evolution, and effects
• Mass and Metallicity Requirement in Stellar Models for Galactic Chemical Evolution Applications
• Astronomical Oxygen Isotopic Evidence for Supernova Enrichment of the Solar System Birth Environment by Propagating Star Formation
• Total and partial cross sections of the ${}^{112}$Sn($\alpha ,\gamma$)${}^{116}$Te reaction measured via in-beam $\gamma$-ray spectroscopy
• 128Xe and 130Xe: Testing He-shell burning in AGB stars
• The $\gamma$-process nucleosynthesis in core-collapse supernovae. I. A novel analysis of $\gamma$-process yields in massive stars
• Evolution and Nucleosynthesis of Massive Stars and Related Nuclear Uncertainties
• The Impact of Black Hole Formation on Population Averaged Supernova Yields
• Distributions of Short-Lived Radioactive Nuclei Produced by Young Embedded Stellar Clusters
• High precision ${}^{113}$In($\alpha ,\alpha$)${}^{113}$In elastic scattering at energies around the Coulomb barrier for the astrophysical $\gamma$ process
• The peculiar Ca-rich SN 2019ehk: Evidence for a Type IIb core-collapse supernova from a low mass stripped progenitor
• A Solar System formation analogue in the Ophiuchus star-forming complex
• 11B and Constraints on Neutrino Oscillations and Spectra from Neutrino Nucleosynthesis
• Cross sections for proton-induced reactions on Pd isotopes at energies relevant for the gamma process
• The photometric variability of massive stars due to gravity waves excited by core convection
• The Role of the Hadron-Quark Phase Transition in Core-Collapse Supernovae
• Investigation of $\alpha$-induced reactions on Sb isotopes relevant to the astrophysical $\gamma$-process
• Experimental cross sections of 165Ho(α,n)168Tm and 166Er(α,n)169Yb for optical potential studies relevant for the astrophysical γ-process
• The Impact of Hydrodynamic Mixing on Supernova Progenitors
• $p$-Process simulations with a modified reaction library
• The p-process in exploding rotating massive stars
• Measurement of the 187Re(α,n)190Ir reaction cross section at sub-Coulomb energies using the Cologne Clover Counting Setup
• Bayes' theorem and early solar short-lived radionuclides: the case for an unexceptional origin for the solar system
• Discovery Prospects for a Supernova Signature of Biogenic Origin
• New \textsl{s}-process Mechanism in Rapidly-Rotating Massive Pop II Stars
• Measurements of ${}^{152}$Gd(p,$\gamma$)${}^{153}$Tb and ${}^{152}$Gd(p,n)${}^{152}$Tb reaction cross sections for the astrophysical $\gamma$ process
• Simulating X-ray bursts during a transient accretion event
• On the internal pollution mechanisms in the globular cluster NGC 6121 (M4): heavy-element abundances and AGB models
• The synthesis of Ti44 and Ni56 in massive stars
• Photoactivation at a clinical LINAC: The 197Au(gamma,n)196Au reaction slightly above threshold
• Intermediate-mass asymptotic giant branch stars and sources of ${}^{26}$Al, ${}^{60}$Fe, ${}^{107}$Pd, and ${}^{182}$Hf in the solar system
• Nucleosynthesis in Neutrino-Driven Supernovae
• Investigation of alpha-induced reactions on 127I for the astrophysical gamma process
• Progenitor mass and ejecta asymmetry of SN 2023ixf from nebular spectroscopy
• Massive Star Evolution: Nucleosynthesis and Nuclear Reaction Rate Uncertainties
• Common Occurrence of Explosive Hydrogen Burning in Type II Supernovae
• The Search for Supernova-produced Radionuclides in Terrestrial Deep-sea Archives
• Hard X-ray emissions from Cassiopeia A observed by INTEGRAL
• Ground-state ammonia and water in absorption towards Sgr B2
• Astrophysical analysis of the measurement of (alpha,gamma) and (alpha,n) cross sections of 169Tm
• nu-Process Nucleosynthesis in Population III Core-Collapse Supernovae
• Massive Stars and their Supernovae
• Cluster analysis of presolar silicon carbide grains: evaluation of their classification and astrophysical implications
• Suzaku Observations of Thermal and Non-Thermal X-Ray Emission from the Middle-Aged Supernova Remnant G156.2+5.7
• Experimental (n,$\gamma$) cross sections of the p-process nuclei ${}^{74}$Se and ${}^{84}$Sr
• Detailed Iron-Peak Element Abundances in Three Very Metal-Poor Stars
• Radioactive nuclei in the early Solar System: analysis of the 15 isotopes produced by core-collapse supernovae
• The interplay between chemistry and nucleation in the formation of carbonaceous dust in supernova ejecta
• Explosive nucleosynthesis in the neutrino-driven aspherical supernova explosion of a non-rotating 15$M_{\odot }$ star with solar metallicity
• Nucleosynthesis of Fe60 in massive stars
• Far-flung Filaments of Ejecta in the Young Supernova Remnant G292.0+1.8
• Measurement of the ${}^{90,92}$Zr(p,$\gamma$)${}^{91,93}$Nb reactions for the nucleosynthesis of elements around A=90
• Reaction Rate Sensitivity of the Production of $\gamma$-ray Emitting Isotopes in Core-Collapse Supernova
• Asymptotic normalization coefficients of resonant and bound states from the phase shifts for $\alpha \alpha$ and ${\alpha }^{12}\mathrm{C}$ scattering
• Completing the nuclear reaction puzzle of the nucleosynthesis of 92Mo
• Metallicity-Dependent Galactic Isotopic Decomposition for Nucleosynthesis
• Pre-supernova mixing in CEMP-no source stars
• FUSE Deuterium Observations: A Strong Case For Galactic Infall
• Isotope Anomalies in the Fe-group Elements in Meteorites and Connection to Nucleosynthesis in AGB Stars
• C, N, and O Isotopic Heterogeneities in Low-density Supernova Graphite Grains from Orgueil
• Carbon monoxide formation and cooling in supernovae
• A Deep Near-Infrared [Fe II]+[Si I] Emission Line Image of the Supernova Remnant Cassiopeia A
• They Came From the Deep in the Supernova: The Origin of TiC and Metal Subgrains in Presolar Graphite Grains
• Heavy Elements Nucleosynthesis On Accreting White Dwarfs: building seeds for the p-process
• alpha-induced reactions on 115In: cross section measurements and statistical model analysis
• Formation, distribution, and IR emission of dust in the clumpy ejecta of Type II-P core-collapse supernovae, in isotropic and anisotropic scenarios
• Measurement of (alpha,n) reaction cross sections of erbium isotopes for testing astrophysical rate predictions
• Simultaneous measurement of beta-delayed proton and gamma emission of ${}^{26}$P for ${}^{25}$Al($p,\gamma$)${}^{26}$Si reaction rate
• Cross-section measurement of the ${}^{130}$Ba(p,$\gamma$)${}^{131}$La reaction for $\gamma$-process nucleosynthesis
• Stellar (n,gamma) cross sections of p-process isotopes PartI: 102Pd, 120Te, 130,132Ba,and 156Dy
• Nucleosynthesis in neutrino-driven winds in hypernovae
• Effective Helium Burning Rates and the Production of the Neutrino Nuclei
• Freeze-out yields of radioactivities in core-collapse supernovae
• Neutron Capture Cross Sections for the Weak s Process
• Galactic Chemical Evolution of Radioactive Isotopes with an s-process Contribution
• Reverse and Forward Shock X-ray Emission in an Evolutionary Model of Supernova Remnants undergoing Efficient Diffusive Shock Acceleration
• Stellar evolution of massive stars at very low metallicities
• Chemical evolution of 244Pu in the solar vicinity and its implication for the properties of r-process production
• Study of (${}^6$Li, $d$) and (${}^6$Li, $t$) reactions on ${}^{22}$Ne and implications for $s$-process nucleosynthesis
• Dark Matter from Monogem
• Core-collapse supernova simulations with reduced nucleosynthesis networks
• A Way Out of the Bubble Trouble? - Upon Reconstructing the Origin of the Local Bubble and Loop I via Radioisotopic Signatures on Earth
• 138La-138Ce-136Ce nuclear cosmochronometer of supernova neutrino process
• Sensitivity of ${}^{44}$Ti and ${}^{56}$Ni production in CCSN shock-driven nucleosynthesis to reaction rates
• Cross section of $\alpha$-induced reactions on ${}^{197}$Au at sub-Coulomb energies
• Experimental study of the astrophysical gamma-process reaction 124Xe(alpha,gamma)128Ba
• A detailed look at the thermal and non-thermal X-ray emission from the Vela supernova remnant with SRG/eROSITA
• Enrichment of the Galactic disc with neutron-capture elements: Mo and Ru
• Dust Production in a Thin Dense Shell in Supernovae with Early Circumstellar Interactions
• Formation Scenario of the Progenitor of iPTF13bvn Revisited
• Neutron activation of natural zinc samples at kT = 25 keV
• Presolar Grains from Novae: Evidence from Neon and Helium Isotopes in Comet Dust Collections
• Abundance Inhomogeneity in the Northeastern Rim of the Cygnus Loop Revealed by Suzaku Observatory
• SNII enrichment and the star cluster mass function
• Boron Synthesis in Type Ic Supernovae
• Nucleosynthesis in Primordial Hypernovae
• Single and binary evolution of Population III stars and their supernovae light curves
• Systematic study of (p,γ) reactions on Ni isotopes
• The interaction of young massive stars with their environment: A millimeter and submillimeter line study of NGC6334 FIR II
• New attempts to understand nanodiamond stardust
• A strong neutron burst in jet-like supernovae of spinstars
• Type Ia Supernova Nucleosynthesis: Metallicity-Dependent Yields
• The chemical evolution of the solar neighbourhood for planet-hosting stars
• Reducing Uncertainties in the Production of the Gamma Emitting Nuclei 26Al, 44Ti, and 60Fe in Core Collapse Supernovae by Using Effective Helium Burning Rates
• Signatures of a surviving helium-star companion in Type Ia supernovae and constraints on the progenitor companion of SN 2011fe
• The nebular spectra of SN 2023ixf: A lower mass, partially stripped progenitor may be the result of binary interaction
• Chemo-dynamical simulations of dwarf galaxy evolution
• A Decade-Baseline Study of the Plasma States of Ejecta Knots in Cassiopeia A
• Constraining the Astrophysical p Process: Cross Section Measurement of the 84Kr(p,g)85Rb Reaction in Inverse Kinematics
• Presolar grain dynamics: creating nucleosynthetic variations through a combination of drag and viscous evolution
• ASASSN-18am/SN 2018gk : An overluminous Type IIb supernova from a massive progenitor
• Neutron Star Planets: Atmospheric processes and habitability
• NanoSIMS, TEM, and XANES studies of a Unique Presolar Supernova Graphite Grain
• The Occurrence and Impact of Carbon-Oxygen Shell Mergers in Massive Stars
• Measurements of ${}^{160}$Dy($p,\gamma$) at energies relevant for astrophysical $\gamma$ process
• Massive stars evolution with new C12+C12 nuclear reaction rate -- the core carbon-burning phase
• The 106Cd(alpha,alpha)106Cd elastic scattering in a wide energy range for gamma-process studies
• Comparison between core-collapse supernova nucleosynthesis and meteoric stardust grains: investigating magnesium, aluminium, and chromium
• Limits on the Number of Galactic Young Supernova Remnants Emitting in the Decay Lines of 44Ti
• Convective overshooting and production of s-nuclei in massive stars during their core He-burning phase
• Collateral Effects on Solar Nebula Oxygen Isotopes due to Injection of 26Al by a Nearby Supernova
• 44Ti radioactivity in young supernova remnants: Cas A and SN 1987A
• The metamorphosis of the Type Ib SN 2019yvr: late-time interaction
• Molecules in supernova ejecta
• The Chemical Evolution of Iron-Peak Elements with Hypernovae
• Insights into thermonuclear supernovae from the incomplete silicon burning process
• Anomalous dynamics triggered by a non-convex equation of state in relativistic flows
• Constraining the onset density for the QCD phase transition with the neutrino signal from core-collapse supernovae
• Rotating massive stars: Pre-SN models and stellar yields at solar metallicity
• The impact of asymmetric neutrino emissions on nucleosynthesis in core-collapse supernovae
• The Galactic 26Al Problem and The Close Binary SNIb/c Solution?
• (n,$\gamma$) Cross Sections of Light p Nuclei -- Towards an Updated Database for the p Process
• First direct measurement of the ${}^{13}$N($\alpha$,$p$)${}^{16}$O reaction relevant for core-collapse supernovae nucleosynthesis
• Unveiling the chemical fingerprint of phosphorus-rich stars I. In the infrared region of APOGEE-2
• Can Galactic chemical evolution explain the oxygen isotopic variations in the Solar System?
• A global view of shocked plasma in the supernova remnant Puppis A provided by SRG/eROSITA
• Presolar grains
• Isotopic ratios for C, N, Si, Al, and Ti in C-rich presolar grains from massive stars
• Thermonuclear 17O(n,gamma)18O reaction rate and its astrophysical implications
• Origin of the Chemical Elements
• The impact of asymmetric neutrino emissions on nucleosynthesis in core-collapse supernovae II -- progenitor dependences --
• Alpha-induced reactions for the astrophysical p-process: the case of 151Eu
• Measurement of the 91Zr(p,gamma)92mNb cross section motivated by type Ia supernova nucleosynthesis
• Modelling the composition of a young star cluster ejecta
• $s$-Process in Massive Carbon-Enhanced Metal-Poor Stars
• Chromium Nucleosynthesis and Silicon-Carbon Shell Mergers in Massive Stars
• Distributions of Long-Lived Radioactive Nuclei Provided by Star Forming Environments
• The $\gamma$-process nucleosynthesis in core-collapse supernovae II. Effect of the explosive recipe
• Beta decay and electron capture rates on manganese isotopes in astrophysical environments
• The s process in massive stars, a benchmark for neutron capture reaction rates
• Three-dimensional Supernova Models Provide New Insights into the Origins of Stardust
• High precision half-life measurement of ${}^{125}$Cs and ${}^{125}$Xe with γ-spectroscopy
• Theoretical Distributions of Short-Lived Radionuclides for Star Formation in Molecular Clouds
• Binary Systems of core collapse supernova polluting a giant companion
• Reaction Rate Sensitivity of the gamma-Process Path
• G0.57-0.018: A young supernova remnant? INTEGRAL and VLA observations
• Timescales of Solar System Formation Based on Al-Ti Isotope Correlation by Supernova Ejecta
• Representation of s-process abundances for comparison to data from bulk meteorites
• The birth environment of the solar system constrained by the relative abundances of the solar radionuclides
• The nebular phase of SN 2024ggi: a low-mass progenitor with no signs of interaction
• Transition Elements in Supernova Presolar Grains: Condensation vs. Implantation
• Impact of Newly Measured Nuclear Reaction Rates on ${}^{26}$Al Ejected Yields from Massive Stars
• Near-Infrared Spectroscopy of Dense Ejecta Knots in the Outer Eastern Area of the Cassiopeia A Supernova Remnant
• Yields from massive stars in binaries. Chemical evolution of the Milky Way disk
• Spectral synthesis techniques for supernovae and kilonovae
• The SPAr burning: proton captures powering carbon-oxygen shell mergers in massive stars
• Impact of accretion-induced chemically homogeneous evolution on stellar and compact binary populations
• Evolving massive stars to core collapse with GENEC: Extension of equation of state, opacities and effective nuclear network
• Stellar evolution, SN explosion, and nucleosynthesis
• Alpha-constrained QSE Nucleosynthesis in High-entropy and Fast-expanding Material
• Carbon from massive binary-stripped stars over cosmic time: effect of metallicity
• E0 emission in alpha + ^12C fusion at astrophysical energies
• Constraining the Synthesis of the Lightest p Nucleus 74Se
• Production of radioactive ${}^{22}$Na in core-collapse supernovae: the Ne-E(L) component in presolar grains and its possible consequences on supernova observations
• Photonuclear reactions with Zinc: A case for clinical linacs
• Modeling the emission lines from r-process elements in Supernova nebulae
• Astronomy with Radioactivities: Chapter 9, Nuclear Reactions
• Plasma Instabilities Dominate Radioactive Transients Magnetic Fields: The self-confinement of leptons in Type Ia and Core-Collapse Supernovae, and Kilonovae
• Symmetry/asymmetry within a cylindrical lattice model of nuclear structure predicts cosmic abundance/scarcity
• Radioactive Decay
• Origin of anomalous Xe-H in presolar diamonds: Indications of a "cold" r-process
• Lepton capture rates due to isotopes of vanadium in astrophysical environment
• Strontium-84 Enrichments in Presolar Grains Provide First Evidence of p-process Nucleosynthesis in Core-collapse Supernovae
• Abundance Uncertainties Obtained With the PizBuin Framework For Monte Carlo Reaction Rate Variations
• Galactic abundances as a relic neutrino detection scheme
• From stars to nuclei
• Observational signatures of the surviving donor star in the double detonation model of Type Ia supernovae
• Modeling The Nucleosynthesis Of Massive Stars
• Occurrence of fast neutrino flavor conversions in QCD phase-transition supernovae
• The impact of new ($\alpha$, n) reaction rates on the weak s-process in metal-poor massive stars
• The importance of charged particle reactions in the r-process on supernovae and neutron stars
• The Early Solar System - Chapter 6
• Photo-nuclear reaction rates of ${}^{157,159}$Ho and ${}^{163,165}$Tm and their impact in the $\gamma$--process
• SDSSJ0018-0939: A Clear Signature of Sub-Chandrasekhar Mass Type 1a Supernova
• A unified nucleosynthetic site for the production of heavy isotopes and p-nuclei
• Nuclear data activities for medium mass and heavy nuclei at Los Alamos
• A Large-scale Approach to Modelling Molecular Biosignatures: The Diatomics
• Theory Considerations For Nucleosynthesis Beyond Fe With Special Emphasis On p-Nuclei In Massive Stars
• Revisiting the formation of molecules and dust in core collapse supernovae
• Impact of the latest 22Ne+α reaction rates on nucleosynthesis in massive stars and galactic chemical evolution
• Aggregation of SiC-X Grains in Supernova Ejecta
• 60Fe and Massive Stars
• Production Uncertainties of p-Nuclei in the $\gamma$-Process in Massive Stars Using a Monte Carlo Approach
• Constraints on dark matter boosted by supernova shock within the effective field theory framework from the CDEX-10 experiment
• Uncertainties in the production of iron-group nuclides in core-collapse supernovae from Monte Carlo variations of reaction rates
• SN 2017ati: A luminous type IIb explosion from a massive progenitor
• Earth's accretion inferred from iron isotopic anomalies of supernova nuclear statistical equilibrium origin
• Massive stars as thermonuclear reactors and their explosions following core collapse
• Lepton emission rates of 43-64V isotopes under stellar conditions
• Signatures of anti-social mass-loss in the ordinary Type II SN 2024bch -- A non-interacting supernova with early high-ionisation features