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, accretion, stellar evolution and similar phenomena. Qualifications: A Ph.D. in Physics or Astronomy. Experience with hydrodynamical, stellar evolution, or radiation-transfer simulations. Benefits: Full
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Group , Elementary Particle Physics , Elementary Particle Theory , Engineering , Environment , Enzymology , evolution , Experimental Astroparticle Physics , Experimental Astrophysics , Experimental Atomic
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of the models in solid state physics • development of the existing C++ code library • applications of the above mentioned simulations to the description of the topological phenomena at the interface between
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