Eric J Lingerfelt Contact LINGERFELTEJ@ORNL.GOV All Publications Distributed Workflows for Modeling Experimental Data Big, deep, and smart data in scanning probe microscopy BEAM: A computational workflow system for managing and modeling material characterization data in HPC environments 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 A domain-specific analysis system for examining nuclear reactor simulation data for light-water and sodium-cooled fast react... Gravitational wave signatures of ab initio two-dimensional core collapse supernova explosion models for 12–25 M stars Two- and Three-Dimensional Multi-Physics Simulations of Core Collapse Supernovae: A Brief Status Report and Summary of Result... Near Real-time Data Analysis of Core-Collapse Supernova Simulations With Bellerophon Axisymmetric Ab Initio Core-Collapse Supernova Simulations of 12--25 Solar Mass Stars... Comparison of Nuclear Mass Models at Nuclearmasses.org. A Multitier System for the Verification, Visualization and Management of CHIMERA Bottlenecks and Waiting Points in Nucleosynthesis in X‐ray bursts and Novae Big Bang Nucleosynthesis: Impact of Nuclear Physics Uncertainties on Baryonic Matter Density Constraints Waiting Points in Nova and X-ray Burst Nucleosynthesis... Big Bang Nucleosynthesis: Impact of Nuclear Physics Uncertainties on Baryonic Matter Density... Thermonuclear Reaction Rate Libraries and Software Tools for Nuclear Astrophysics Research... Nuclear Data for Astrophysics: Resources, Challenges, Strategies, and Software Solutions... Modeling the Effects of Land Use on the Quality of Water, Air, Noise, and Habitat for a Five-County Region in Georgia... The 25Al(p,gamma)26Si Reaction Rate in Novae... Measurement of the 183 keV Resonance in <sup>17</sup>O(p,alpha)<sup>14</sup>N using a Novel Technique... Astrophysically Important <sup>26</sup>Si States Studied with the <sup>28</sup>Si(p,t)<sup>26</sup>Si Reaction - II. Spin of... New Features in the Computational Infrastructure for Nuclear Astrophysics... Nuclear Data on Unstable Nuclei for Astrophysics Key Links
