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Theory of core-collapse supernovae
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Nucleosynthesis and remnants in massive stars of solar metallicity
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Observational Constraints on the Progenitors of Core-Collapse Supernovae: The Case for Missing High-Mass Stars
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The Status of Multi-Dimensional Core-Collapse Supernova Models
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The first gravitational-wave source from the isolated evolution of two stars in the 40–100 solar mass range
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Quark deconfinement as a supernova explosion engine for massive blue supergiant stars
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Conditions for shock revival by neutrino heating in core-collapse supernovae
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Radiation hydrodynamics with neutrinos: Variable Eddington factor method for core-collapse supernova simulations
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Neutrino‐driven Convection versus Advection in Core‐Collapse Supernovae
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SUPERNOVA 2008bk AND ITS RED SUPERGIANT PROGENITOR
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Delayed Neutrino-Driven Supernova Explosions Aided by the Standing Accretion-Shock Instability
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The Isotropic Diffusion Source Approximation for Supernova Neutrino Transport
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Black hole Formation in Failing Core-Collapse Supernovae
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A Global Turbulence Model for Neutrino-Driven Convection in Core-Collapse Supernovae
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The Physics of the Neutrino Mechanism of Core-Collapse Supernovae
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Turbulent Magnetic Field Amplification from Spiral sasi Modes: Implications for Core-Collapse Supernovae and Proto-Neutron star Magnetization
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Is Strong sasi Activity the key to Successful Neutrino-Driven Supernova Explosions?
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A new Multi-Dimensional General Relativistic Neutrino Hydrodynamics code for Core-Collapse Supernovae. ii. Relativistic Explosion Models of Core-Collapse Supernovae
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THE RED SUPERGIANT PROGENITOR OF SUPERNOVA 2012aw (PTF12bvh) IN MESSIER 95
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Progenitor-Explosion Connection and Remnant Birth Masses for Neutrino-Driven Supernovae of Iron-Core Progenitors
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Missing Black Holes Unveil the Supernova Explosion Mechanism
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The Progenitor Dependence of the Pre-Explosion Neutrino Emission in Core-Collapse Supernovae
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Dimensional Dependence of the Hydrodynamics of Core-Collapse Supernovae
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Very low Energy Supernovae from Neutrino mass loss
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May 2013 |
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The Dominance of Neutrino-Driven Convection in Core-Collapse Supernovae
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June 2013 |
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Equation of State and Neutron star Properties Constrained by Nuclear Physics and Observation
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Core-Collapse Supernova Equations of State Based on Neutron star Observations
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August 2013 |
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On the Impact of Three Dimensions in Simulations of Neutrino-Driven Core-Collapse Supernova Explosions
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The Compactness of Presupernova Stellar Cores
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High-Resolution Three-Dimensional Simulations of Core-Collapse Supernovae in Multiple Progenitors
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The role of Turbulence in Neutrino-Driven Core-Collapse Supernova Explosions
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The Black hole Formation Probability
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The Landscape of the Neutrino Mechanism of Core-Collapse Supernovae: Neutron star and Black hole mass Functions, Explosion Energies, and Nickel Yields
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Pushing Core-Collapse Supernovae to Explosions in Spherical Symmetry. i. the Model and the case of sn 1987a
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Beyond Mixing-Length Theory: a step Toward 321d
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Modules for Experiments in Stellar Astrophysics (Mesa): Planets, Oscillations, Rotation, and Massive Stars
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An Open-Source Neutrino Radiation Hydrodynamics code for Core-Collapse Supernovae
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Turbulence in core-collapse supernovae
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Global comparison of core-collapse supernova simulations in spherical symmetry
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AXISYMMETRIC AB INITIO CORE-COLLAPSE SUPERNOVA SIMULATIONS OF 12-25 M ☉ STARS
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March 2013 |
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THE PROGENITOR OF SUPERNOVA 2011dh HAS VANISHED
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July 2013 |
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Revival of the Stalled Core-Collapse Supernova Shock Triggered by Precollapse Asphericity in the Progenitor star
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October 2013 |
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THREE-DIMENSIONAL CORE-COLLAPSE SUPERNOVA SIMULATED USING A 15 M ⊙ PROGENITOR
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July 2015 |
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The Three-Dimensional Evolution to core Collapse of a Massive star
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July 2015 |
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Neutrino-Driven Explosion of a 20 Solar-Mass star in Three Dimensions Enabled by Strange-Quark Contributions to Neutrino–Nucleon Scattering
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July 2015 |
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Stochasticity and Efficiency in Simplified Models of Core-Collapse Supernova Explosions
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October 2015 |
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Characterizing SASI- and convection-dominated core-collapse supernova explosions in two dimensions
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April 2014 |
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Non-radial instabilities and progenitor asphericities in core-collapse supernovae
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February 2015 |
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The dynamics of neutrino-driven supernova explosions after shock revival in 2D and 3D
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August 2015 |
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A simple approach to the supernova progenitor–explosion connection
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May 2016 |
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Supernova simulations from a 3D progenitor model – Impact of perturbations and evolution of explosion properties
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August 2017 |
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Gravitational wave signals from 3D neutrino hydrodynamics simulations of core-collapse supernovae
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March 2017 |
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The search for failed supernovae with the Large Binocular Telescope: constraints from 7 yr of data
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April 2017 |
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The antesonic condition for the explosion of core-collapse supernovae – I. Spherically symmetric polytropic models: stability and wind emergence
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September 2018 |
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A successful 3D core-collapse supernova explosion model
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September 2018 |
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Mass ejection in failed supernovae: variation with stellar progenitor
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February 2018 |
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Revival of the fittest: exploding core-collapse supernovae from 12 to 25 M⊙
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March 2018 |
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Three-dimensional simulations of neutrino-driven core-collapse supernovae from low-mass single and binary star progenitors
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January 2019 |
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The overarching framework of core-collapse supernova explosions as revealed by 3D fornax simulations
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The mechanism(s) of core-collapse supernovae
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Medium modification of the charged-current neutrino opacity and its implications
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Probing the gravitational well: No supernova explosion in spherical symmetry with general relativistic Boltzmann neutrino transport
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Weak magnetism for antineutrinos in supernovae
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Protoneutron Star Cooling with Convection: The Effect of the Symmetry Energy
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Observation of Gravitational Waves from a Binary Black Hole Merger
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Muon Creation in Supernova Matter Facilitates Neutrino-Driven Explosions
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Symmetry energy impact in simulations of core-collapse supernovae
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Explosion Mechanisms of Core-Collapse Supernovae
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The Physics of Supernova Explosions
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THE DEVELOPMENT OF EXPLOSIONS IN AXISYMMETRIC AB INITIO CORE-COLLAPSE SUPERNOVA SIMULATIONS OF 12–25 ${M}_{\odot }$ STARS
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A Two-Parameter Criterion for Classifying the Explodability of Massive Stars by the Neutrino-Driven Mechanism
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February 2016 |
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Neutrino-Driven Convection in Core-Collapse Supernovae: High-Resolution Simulations
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March 2016 |
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Core-Collapse Supernovae from 9 to 120 Solar Masses Based on Neutrino-Powered Explosions
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April 2016 |
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Progenitor-Dependent Explosion Dynamics in Self-Consistent, Axisymmetric Simulations of Neutrino-Driven Core-Collapse Supernovae
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June 2016 |
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General-Relativistic Three-Dimensional Multi-Group Neutrino Radiation-Hydrodynamics Simulations of Core-Collapse Supernovae
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October 2016 |
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The last Minutes of Oxygen Shell Burning in a Massive star
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December 2016 |
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An Integral Condition for Core-Collapse Supernova Explosions
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January 2017 |
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Rotation-supported Neutrino-driven Supernova Explosions in Three Dimensions and the Critical Luminosity Condition
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January 2018 |
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Two-dimensional Core-collapse Supernova Explosions Aided by General Relativity with Multidimensional Neutrino Transport
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February 2018 |
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How Turbulence Enables Core-collapse Supernova Explosions
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March 2018 |
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Confronting Models of Massive Star Evolution and Explosions with Remnant Mass Measurements
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March 2018 |
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Equation of State Dependent Dynamics and Multi-messenger Signals from Stellar-mass Black Hole Formation
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April 2018 |
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Exploring Fundamentally Three-dimensional Phenomena in High-fidelity Simulations of Core-collapse Supernovae
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September 2018 |
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PUSHing Core-collapse Supernovae to Explosions in Spherical Symmetry. II. Explodability and Remnant Properties
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PUSHing Core-collapse Supernovae to Explosions in Spherical Symmetry. III. Nucleosynthesis Yields
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December 2018 |
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Convection-aided Explosions in One-dimensional Core-collapse Supernova Simulations. I. Technique and Validation
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On Variations of Pre-Supernova Model Properties
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Black Hole Formation and Fallback during the Supernova Explosion of a 40 M ⊙ Star
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The Progenitor Dependence of Core-collapse Supernovae from Three-dimensional Simulations with Progenitor Models of 12–40 M ⊙
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February 2018 |
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Characterizing the Gravitational Wave Signal from Core-collapse Supernovae
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April 2019 |