Michael S Smith Distinguished Scientist Contact smithms@ornl.gov | 865.576.5037 All Publications Measurement of charge state distributions using a scintillation screen Proton branching ratios in 22Mg for X-ray bursts First Direct Measurement Constraining the 34Ar(α,p)37K Reaction Cross Section for Mixed Hydrogen and Helium Burning in Accreting Neutron Stars A technique for studying (n,p) reactions of astrophysical interest using radioactive beams with SECAR... First (p,n) reaction measurement in inverse kinematics with SECAR... The complex momentum representation approach and its application to low-lying resonances in 17O and 29,31F Horizons: nuclear astrophysics in the 2020s and beyond... Nuclear Data for High Energy Ion Interactions and Secondary Particle Production... Online Bayesian optimization for a recoil mass separator Current nuclear data needs for applications Estimation of the NiCu Cycle Strength and Its Impact on Type I X-Ray Bursts Study of the deformed halo nucleus 31Ne with Glauber model based on microscopic self-consistent structures Neutron transfer reactions on the ground state and isomeric state of a Sn130 beam... SECAR: A recoil separator for nuclear astrophysics Proton branching ratios of 23Mg levels Self-consistent description of the halo nature of 31Ne with continuum and pairing correlations... Online Bayesian Optimization for Beam Alignment in the SECAR Recoil Mass Separator First measurement of proton decay from a transfer reaction to Na21... (alpha,n) nuclear data scoping study... Proton Decay of 21Na for 20Ne Energy Levels... Proton Decay of 21Na for 20Ne Energy Levels... Proceedings of the Workshop for Applied Nuclear Data: WANDA 2020 Nuclear Data Scoping Studies for Nonproliferation - paper Report from the A.I. For Nuclear Physics Workshop... WANDA: AI/ML for Nuclear Data... Pagination Current page 1 Page 2 Page 3 … Next page ›› Last page Last » Key Links ORCID Organizations Physical Sciences Directorate Physics Division Nuclear Science and Advanced Technology Section Nuclear Structure and Nuclear Astrophysics Group
