Physics – Nuclear Physics – Nuclear Theory
Scientist
Physics
Nuclear Physics
Nuclear Theory
Scientist
Universitaet Muenchen
NSCL, Michigan State University
U Muenchen
Ludwig Maximilians Universität München, Germany
Gesellschaft für Schwerionenforschung mbH, Planckstr. 1, 64291 Darmstadt, Germany
Laboratori Nazionali del Sud-INFN, Catania, Italy
Institut für Theoretische Physik I, Westfälische Wilhelms-Universität, Wilhelm-Klemm-Strasse 9, D-48149 Münster, Germany
Gesellschaft für Schwerionenforschung mbH, Darmstadt, Germany
GSI, Postfach 110552, D-64220 Darmstadt, Germany
Sektion Physik, Ludwig-Maximilians Universität-München, Germany
GSI, Planckstrasse 1, 64291 Darmstadt, Germany
Excellence Cluster Universe - Technische Universität München, Garching, Germany ; GSI Helmholtzzentrum für Schwerionenforschung GmbH - Theorie Darmstadt Germany
National Superconducting Cyclotron Laboratory, Michigan State University, East Lansing, MI.
Gesellschaft für Schwerionenforschung mbH, Theorie, Darmstadt, Germany
GSI mbH, Darmstadt, Germany
Dipartimento di Metodologie Fisiche e Chimiche per l'Ingegneria - Università di Catania, Catania, Italy
NSCL, Michigan State University, East Lansing MI 48824 USA
National Superconducting Cyclotron Laboratory, Michigan State University, MI, USA
National Superconducting Cyclotron Laboratory and Department of Physics and Astronomy, Michigan State University, East Lansing, Michigan 48824-1321, USA
Dipartimento di Metodologie Fisiche e Chimiche per l'Ingegneria, Università di Catania, Catania, Italy
National Superconducting Cyclotron Laboratory, East Lansing, MI 48824-1321 Theorie, Planckstrasse 1, D-64291 Darmstadt, Germany
Sektion Physik, Universität München, Am Coulombwall 1, D-85748 Garching bei München, Germany
Accessibility of color superconducting quark matter phases in heavy-ion collisions
Astronuclear physics with Coulomb dissociation
Astrophysical S(E)-factor of the ^15N(p,α)^12C reaction at sub-Coulomb energies via the Trojan-horse method
Bare astrophysical S(E)-factor for the 6Li(d, α)4He and 7Li(p, α)4He reactions at astrophysical energies
Bare nucleus S(E) factor of the 2H(d,p)3H and 2H(d,n)3He reactions via the Trojan Horse Method
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