W Raphael Hix Group Leader (TCP) Contact RAPH@ORNL.GOV All Publications The Role of Neutrinos in r-Process Nucleosynthesis in Supernovae and Gamma-ray Bursts... Fission Cycling in a Supernova r-Process... Nuclear Physics in Core-Collapse Supernovae... Effects of Inelastic Neutrino-Nucleus Scattering on Supernova Dynamics and Radiated Neutrino Spectra <sup>30</sup>S Studied with the <sup>32</sup>S(<i>p,t</i>)<sup>30</sup>S Reaction and the <sup>29</sup>P(<i>p</i>,{gamma})<sup>30</sup>S Reaction Rate The Effects of Changes in Reaction Rates on Simulations of Nova Explosions... The QSE-reduced Nuclear Reaction Network for Silicon Burning Production of Intermediate-Mass and Heavy Nuclei... Astrophysically Important <sup>31</sup>S States Studied with the <sup>32</sup>S(p,d)<sup>31</sup>S Reaction The 25Al(p,gamma)26Si Reaction Rate in Novae... Ascertaining the Core Collapse Supernova Mechanism: An Emerging Picture?... Petascale Supernova Simulation with CHIMERA ... Measurement of the 183 keV Resonance in <sup>17</sup>O(p,alpha)<sup>14</sup>N using a Novel Technique... Explosive Nucleosynthesis in Different Ye Conditions Astrophysically Important <sup>26</sup>Si States Studied with the <sup>28</sup>Si(p,t)<sup>26</sup>Si Reaction - II. Spin of... Neutrinos and Nucleosynthesis in Gamma Ray Bursts The QSE-Reduced Network for Silicon Burning New Features in the Computational Infrastructure for Nuclear Astrophysics... Neutral-Current Neutrino-Nucleus Inelastic Reactions for Core Collapse Supernovae Fission Cycling in Supernova Nucleosynthesis: Active-Sterile Neutrino Oscillations Nuclear Data on Unstable Nuclei for Astrophysics Element Synthesis Calculations for Stellar Explosions: Robust Uncertainties, Sensitivities, and Radioactive Ion Beam Measure... Pagination First page « First Previous page ‹‹ … Page 2 Page 3 Current page 4 Key Links ORCID Organizations Physical Sciences Directorate Physics Division Fundamental Nuclear and Particle Physics Section Theoretical and Computational Physics Group
News Frontier simulations provide new insights into calcium-48’s controversial nuclear magnetic excitation
