Physics – Nuclear Physics – Nuclear Experiment
Scientist
Physics
Nuclear Physics
Nuclear Experiment
Scientist
MSU
Michigan State University, USA
IPNO
University of Michigan
National Superconducting Cyclotron Laboratory and Department of Physics and Astronomy, Michigan State University, East Lansing, Michigan 48824
National Superconducting Cyclotron Facility, Michigan State University, East Lansing, Michigan 48824, USA
Institut für Kernphysik, Technische Universität Wien, Wiedner Hauptstrasse 8-10, A-1040 Wien, Austria
Institut für Kernchemie, Universität Mainz, Mainz, Germany
National Superconducting Cyclotron Laboratory, and Department of Physics and Astronomy, Michigan State University, East Lansing, Michigan 48824, USA
Department of Physics and Astronomy, National Superconducting Cyclotron Laboratory and the Joint Institute for Nuclear Astrophysics, Michigan State University, East Lansing, Michigan 48824, USA
N.S.C.L. and Department of Physics and Astronomy, Michigan State University
Department of Physics and Astronomy, University of Kansas, Lawrence, Kansas 66045
Department of Physics and Astronomy and National Superconducting Cyclotron Laboratory, Michigan State University, East Lansing, Michigan 48824
Department of Physics and Astronomy, and National Superconducting Cyclotron Laboratory, Michigan State University, East Lansing, Michigan 48824
Department of Physics and Astronomy, and National Superconducting Cyclotron Laboratory, Michigan State University, East Lansing, Michigan 48824-1321, USA
Department of Physics, University of Notre Dame, Notre Dame, IN 46556, USA
National Superconducting Cyclotron Laboratory, Michigan State University, East Lansing, Michigan 48824, USA
Department of Physics and Astronomy and National Superconducting Cyclotron Laboratory, Michigan State University East Lansing, Michigan 48824-1321, USA
Department of Physics and Astronomy and National Superconducting Cyclotron Laboratory, Michigan State University, East Lansing, Michigan 48824-1321,
22Mg and the 21Na(p,γ) reaction rate
Absolute Spectroscopic Factors from Single-Nucleon Knockout Reactions
Applications of the USD Hamiltonians to rapid-proton capture rates for sd-shell nuclei
Astrophysical S factors for CNO reactions ^11C(p,γ)^12N and ^14N(p,γ)^15O from asymptotic normalization coefficients
Asymptotic normalization coefficients for 14N+p15O and the astrophysical S factor for 14N(p,γ)15O
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