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 Thermonuclear Reaction Rate Libraries and Software Tools for Nuclear Astrophysics Research... 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... 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... Measurement of the 183 keV Resonance in <sup>17</sup>O(p,alpha)<sup>14</sup>N using a Novel Technique... The 25Al(p,gamma)26Si Reaction Rate in Novae... 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