Showing 1–20 of 78 results
/ Date/ Name
Apr 27, 2026Core Collapse Supernova Modeling: The Next Ten YearsAug 22, 2022Core Collapse Supernova Gravitational Wave Emission for Progenitors of 9.6, 15, and 25 Solar MassesOct 18, 2020Physical, numerical, and computational challenges of modeling neutrino transport in core-collapse supernovaeOct 4, 2004The Core Collapse Supernova Mechanism: Current Models, Gaps, and the Road AheadJul 29, 2020Gravitational-wave signal of a core-collapse supernova explosion of a 15 Solar mass starApr 17, 1997Simulations of Core Collapse Supernovae In One and Two Dimemsions Using Multigroup Neutrino TransportJul 20, 2015A Neutrino-Driven Core Collapse Supernova Explosion of a 15 M StarMay 26, 2022Toward Realistic Models of Core Collapse Supernovae: A Brief ReviewMay 27, 2014Two- and Three-Dimensional Multi-Physics Simulations of Core Collapse Supernovae: A Brief Status Report and Summary of Results from the "Oak Ridge" GroupJan 22, 2024Gravitational Waves from Neutrino-Driven Core Collapse Supernovae: Predictions, Detection, and Parameter EstimationJan 7, 2015Recent Progress on Ascertaining the Core Collapse Supernova Explosion MechanismAug 6, 1998The Effects of General Relativity on Core Collapse SupernovaeSep 18, 1997Investigation of Neutrino-Driven Convection and the Core Collapse Supernova Mechanism Using Multigroup Neutrino TransportOct 27, 2000Simulations of Stellar Core Collapse, Bounce, and Postbounce Evolution with Boltzmann Neutrino Transport, and Implications for the Core Collapse Supernova MechanismMay 5, 2010Gravitational Waves from Core Collapse SupernovaeNov 16, 2010Core Collapse Supernovae using CHIMERA: Gravitational Radiation from Non-Rotating ProgenitorsNov 20, 2008Generation of Magnetic Fields by the Stationary Accretion Shock InstabilityJun 11, 2018Global Comparison of Core-Collapse Supernova Simulations in Spherical SymmetrySep 28, 2020A Discontinuous Galerkin Method for General Relativistic Hydrodynamics in thornadoNov 9, 2020thornado-hydro: a discontinuous Galerkin method for supernova hydrodynamics with nuclear equations of state