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@PHDTHESIS{Salmagne:668621,
      author       = {Salmagne, Christian},
      othercontributors = {Kull, Hans-Jörg and Reiter, Detlev},
      title        = {{A}b initio {S}imulation der {P}lasma-{W}and-{K}ontaktzone
                      : {E}ntwicklung und {B}ewertung gitterfreier {A}lgorithmen},
      school       = {RWTH Aachen University},
      type         = {Dissertation},
      address      = {Aachen},
      reportid     = {RWTH-2016-06901},
      pages        = {1 Online-Ressource (IX, 183 Seiten) : Illustrationen,
                      Diagramme},
      year         = {2016},
      note         = {Veröffentlicht auf dem Publikationsserver der RWTH Aachen
                      University; Dissertation, RWTH Aachen University, 2016},
      abstract     = {The plasma edge region has a significant influence on the
                      magnetic confinement in fusion plasmas, which in turn
                      determines the efficiency of a possible future fusion
                      reactor. Thus, the processes taking place in this region
                      have to be understood in detail to be able to accurately
                      control the edge region. A numerical way to gain deeper
                      insights into the complex processes within the plasma sheath
                      region is the ab intio kinetic particle simulation. The
                      kinetic description is capable of resolving even the
                      smallest scales of interest in time and space. The
                      Particle-in-Cell scheme is a grid based representative of
                      this class of simulations. It has been used for simulations
                      of the plasma sheath for a considerable time. Within this
                      work, another concept of kinetic particle simulations is
                      used – the Barnes-Hut Tree Code. This method has been
                      successfully used for simulations of laser plasmas as well
                      as for simulations of galaxy formation before. Due to
                      intrinsic properties of this method, it should be well
                      suited for treating typical plasmas in the plasma wall
                      interaction region. However, contradictions to analytical as
                      well as numerical results were found in previous attempts to
                      simulate the edge region with a Tree Code. These
                      contradictions had not been resolved so far. In the present
                      work the massively parallel Barnes-Hut Tree Code PEPC is
                      used to develop and evaluate a numerical model of the plasma
                      wall interaction region. The discrepancies have been
                      understood and completely dispelled. An artificially
                      increased collisionality within the simulation plasma and
                      numerical heating of the electrons were identified as the
                      cause aforementioned contradictions. For the first time,
                      these effects have been measured and parametrized by plasma
                      density, plasma temperature and several numerical input
                      parameters in a wide parameter range. Using the obtained
                      results, the electron and ion kinetics within the plasma
                      sheath region have been self-consistently modeled from first
                      principles as a proof of concept.Given this proof of
                      concept, we developed a guideline that helps to evaluate, if
                      a given plasma edge problem can be tackled with the grid
                      free particle simulation. This guideline is based upon two
                      criteria. First, the aforementioned parametrization of the
                      collision and heating times in a simulation plasma as well
                      as additional stability criteria are used to exclude
                      numerical parameters that lead to incorrect results. Second,
                      considerations regarding the runtime of the massively
                      parallel simulations are used to define a maximum system
                      size and simulation length. Finally, usage of the developed
                      guideline is demonstrated by means of several relevant
                      examples.},
      cin          = {056500 / 133510 / 135220 / 130000},
      ddc          = {530},
      cid          = {$I:(DE-82)056500_20140620$ / $I:(DE-82)133510_20140620$ /
                      $I:(DE-82)135220_20140620$ / $I:(DE-82)130000_20140620$},
      typ          = {PUB:(DE-HGF)11},
      urn          = {urn:nbn:de:hbz:82-rwth-2016-069013},
      url          = {https://publications.rwth-aachen.de/record/668621},
}