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Use of mesh based variance reduction technique for shielding calculations of the stellarator power reactor HELIAS

  • André Häußler (Corresponding author)
  • , Ulrich Fischer
  • , Felix Warmer

Onderzoeksoutput: Bijdrage aan tijdschriftTijdschriftartikelAcademicpeer review

Samenvatting

The shielding capability is an important aspect of a fusion power plant. The neutron flux decreases in areas far away from the plasma chamber while at the same time the statistical error in Monte Carlo particle transport simulations increases significantly in such regions. This requires variance reduction methods to guide the particles in regions of interest and improve the statistical accuracy. The mesh based weight window technique, applied with ADVANTG, is investigated in this paper and successfully applied for the first neutronic investigation of the shielding performance for the HELIAS stellarator. The obtained results are in an area with high neutron wall load and reduced material thickness. They will be evaluated against the design requirements specified for the EU DEMO tokamak fusion reactor. The results show that the current HELIAS design cannot fulfill the shielding limits specified for DEMO in the investigated area, which is mainly due to the limited space available in the stellarator and should be overcome by improved design solutions for blanket and shield.Save

Originele taal-2Engels
Pagina's (van-tot)671-675
Aantal pagina's5
TijdschriftFusion Engineering and Design
Volume146
DOI's
StatusGepubliceerd - sep. 2019
Extern gepubliceerdJa

Bibliografische nota

Publisher Copyright:
© 2019 Elsevier B.V.

Financiering

This work has been carried out within the framework of the EUROfusion Consortium and has received funding from the Euratom research and training programme 2014-2018 under grant agreement No 633053 . The views and opinions expressed herein do not necessarily reflect those of the European Commission. This work was performed on the computational resource ForHLR II funded by the Ministry of Science, Research and the Arts Baden-Württemberg and DFG ("Deutsche Forschungsgemeinschaft") . This work has been carried out within the framework of the EUROfusion Consortium and has received funding from the Euratom research and training programme 2014-2018 under grant agreement No 633053. The views and opinions expressed herein do not necessarily reflect those of the European Commission. This work was performed on the computational resource ForHLR II funded by the Ministry of Science, Research and the Arts Baden-W?rttemberg and DFG (?Deutsche Forschungsgemeinschaft?).

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