Eirik Endeve Computational Astrophysicist Contact 865.576.6349 | ENDEVEE@ORNL.GOV All Publications Dynamic scan control in STEM: Spiral scans BEAM: A computational workflow system for managing and modeling material characterization data in HPC environments The Multi-Dimensional Character of Core-Collapse Supernovae... Convection- and SASI-driven flows in parametrized models of core-collapse supernova explosions Convection- and SASI-driven flows in parametrized models of core-collapse supernova explosions... The Development of Explosions in Axisymmetric Ab Initio Core-Collapse Supernova Simulations of 12--25 Msun Stars BEAM: A Computational Workflow System for Managing and Modeling Material Characterization Data in HPC Environments Multidimensional simulations of core-collapse supernovae and implications for nucleosynthesis Gravitational wave signatures of ab initio two-dimensional core collapse supernova explosion models for 12–25  M stars Accelerating Our Understanding of Supernova Explosion Mechanism via Simulations and Visualizations with GenASiS Three-dimensional core-collapse supernova simulated using a 15 solar mass progenitor... Bound-preserving discontinuous Galerkin methods for conservative phase space advection in curvilinear coordinates Two- and Three-Dimensional Multi-Physics Simulations of Core Collapse Supernovae: A Brief Status Report and Summary of Result... Essential Ingredients in Core-collapse Supernovae... Turbulence and magnetic field amplification from spiral SASI modes in core-collapse supernovae... Conservative 3+1 General Relativistic Boltzmann Equation... Conservative 3+1 General Relativistic Variable Eddington Tensor Radiation Transport Equations Axisymmetric Ab Initio Core-Collapse Supernova Simulations of 12--25 Solar Mass Stars... Turbulent Magnetic Field Amplification from Spiral SASI Modes: Implications for Core-Collapse Supernovae and Proto-Neutron St... Towards the Core-Collapse Supernova Explosion Mechanism... Towards Exascale Supernova Simulations with GenASiS Generation of Magnetic Fields by the Stationary Accretion Shock Instability Magnetic Field Generation by the Stationary Accretion Shock Instability... MHD Models of Stellar Core Collapse with GenASiS Pagination First page « First Previous page ‹â¶Ä¹ Page 1 Current page 2 Key Links Organizations Computing and Computational Sciences Directorate Computer Science and Mathematics Division Mathematics in Computation Section Multiscale Methods and Dynamics Group
