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Neutrino-Driven Turbulent Convection and Standing Accretion Shock Instability in Three-Dimensional Core-Collapse Supernovae
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An Open-Source Neutrino Radiation Hydrodynamics code for Core-Collapse Supernovae
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THREE-DIMENSIONAL CORE-COLLAPSE SUPERNOVA SIMULATED USING A 15 M ⊙ PROGENITOR
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The Three-Dimensional Evolution to core Collapse of a Massive star
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Towards a realistic explosion landscape for binary population synthesis
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The search for failed supernovae with the Large Binocular Telescope: a new candidate and the failed SN fraction with 11 yr of data
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The final core collapse of pulsational pair instability supernovae
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March 2021 |
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Three-dimensional simulation of a core-collapse supernova for a binary star progenitor of SN 1987A
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A force explosion condition for spherically symmetric core-collapse supernovae
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The essential character of the neutrino mechanism of core-collapse supernova explosions
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The force explosion condition is consistent with spherically symmetric CCSN explosions
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On the treatment of phenomenological turbulent effects in one-dimensional simulations of core-collapse supernovae
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Three-dimensional simulations of SASI- and convection-dominated core-collapse supernovae
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July 2015 |
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A simple approach to the supernova progenitor–explosion connection
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May 2016 |
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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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A critical assessment of turbulence models for 1D core-collapse supernova simulations
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June 2019 |
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The overarching framework of core-collapse supernova explosions as revealed by 3D fornax simulations
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November 2019 |
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Three-dimensional simulations of rapidly rotating core-collapse supernovae: finding a neutrino-powered explosion aided by non-axisymmetric flows
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May 2016 |
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Neutrino-nucleon scattering in supernova matter from the virial expansion
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February 2017 |
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Remnant masses from 1D+ core-collapse supernovae simulations: Bimodal neutron star mass distribution and black holes in the low-mass gap
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July 2024 |
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Weak magnetism for antineutrinos in supernovae
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January 2002 |
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The evolution and explosion of massive stars
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November 2002 |
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Explosion Mechanisms of Core-Collapse Supernovae
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November 2012 |
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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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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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Exploring Fundamentally Three-dimensional Phenomena in High-fidelity Simulations of Core-collapse Supernovae
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September 2018 |
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Three-dimensional Core-collapse Supernova Simulations with Multidimensional Neutrino Transport Compared to the Ray-by-ray-plus Approximation
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March 2019 |
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One-, Two-, and Three-dimensional Simulations of Oxygen-shell Burning Just before the Core Collapse of Massive Stars
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August 2019 |
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Convection-aided Explosions in One-dimensional Core-collapse Supernova Simulations. I. Technique and Validation
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December 2019 |
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Simulating Turbulence-aided Neutrino-driven Core-collapse Supernova Explosions in One Dimension
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February 2020 |
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Large-scale Mixing in a Violent Oxygen–Neon Shell Merger Prior to a Core-collapse Supernova
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February 2020 |
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General Relativistic Neutrino-driven Turbulence in One-dimensional Core-collapse Supernovae
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April 2021 |
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Self-consistent 3D Supernova Models From −7 Minutes to +7 s: A 1-bethe Explosion of a ∼19 M ⊙ Progenitor
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June 2021 |
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Three-dimensional Hydrodynamic Simulations of Convective Nuclear Burning in Massive Stars Near Iron Core Collapse
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October 2021 |
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Equation-of-state Dependence of Gravitational Waves in Core-collapse Supernovae
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December 2021 |
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Effect of the Nuclear Equation of State on Relativistic Turbulence-induced Core-collapse Supernovae
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February 2022 |
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The Effect of Supernova Convection On Neutron Star and Black Hole Masses
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May 2022 |
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Explosion Mechanism of Core-collapse Supernovae: Role of the Si/Si–O Interface
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May 2023 |
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On Variations of Pre-Supernova Model Properties
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December 2016 |
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Applications of Machine Learning to Predicting Core-collapse Supernova Explosion Outcomes
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September 2022 |
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Progenitor Stars Calculated with Small Reaction Networks should not be Used as Initial Conditions for Core Collapse
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journal
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June 2024 |
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Including Neutrino-driven Convection into the Force Explosion Condition to Predict Explodability of Multi-dimensional Core-collapse Supernovae (FEC+)
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preprint
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January 2023 |
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Three-dimensional Magneto-hydrodynamic Simulations of Core-collapse Supernovae: I. Hydrodynamic evolution and protoneutron star properties
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preprint
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January 2024 |
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Long-Time 2D Simulations of Fallback Supernovae: A Systematic Investigation of Explosions Dynamics and Mass Ejections
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preprint
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January 2024 |
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Black Hole Supernovae, their Equation of State Dependence and Ejecta Composition
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preprint
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January 2024 |