% IMPORTANT: The following is UTF-8 encoded. This means that in the presence % of non-ASCII characters, it will not work with BibTeX 0.99 or older. % Instead, you should use an up-to-date BibTeX implementation like “bibtex8” or % “biber”. @INPROCEEDINGS{Engels:848192, author = {Engels, Ralf W. and Awwad, Hani and Grigoryev, Kirill and Huxold, Lukas and Büscher, Markus and Engin, Ilhan and Hützen, Anna and Ciullo, Giuseppe and Fotyev, V. D. and Ivshin, K. A. and Komarov, E. N. and Kotchenda, Leonid and Kravchenko, P. V. and Kravtsov, P. A. and Sherman, S. G. and Soloviev, A. N. and Soloviev, I. N. and Trofimov, V. A. and Vasilyev, A. A. and Vznuzdaev, M. E. and Toporkov, D. and Rachek, I. A. and Shestakov, Yu. V. and Rakitzis, T. P. and Sofikitis, D. and Kannis, C. S. and Boulogiannis, G. K.}, title = {{A}dvantages of {N}uclear {F}usion with {P}olarized {F}uel}, volume = {324}, address = {Italy}, reportid = {FZJ-2018-03458}, series = {Proceedings of Science}, pages = {031}, year = {2018}, abstract = {The use of nuclear polarized fuel, i.e. polarized D, T or 3He, for coming fusion reactors promises to increase their energy output and to optimize the complete fusion process in various ways. But before these advantages can be utilized, several questions must be answered and technical issues must be overcome. Among others, the members of the PREFER collaboration started to investigate the different challenges of “polarized fusion”.}, month = {Oct}, date = {2017-10-16}, organization = {The XVII International Workshop on Polarized Sources, Targets and Polarimetry, Daejeon (South Korea), 16 Oct 2017 - 20 Oct 2017}, cin = {IKP-2 / PGI-6}, cid = {I:(DE-Juel1)IKP-2-20111104 / I:(DE-Juel1)PGI-6-20110106}, pnm = {612 - Cosmic Matter in the Laboratory (POF3-612)}, pid = {G:(DE-HGF)POF3-612}, typ = {PUB:(DE-HGF)8 / PUB:(DE-HGF)7}, url = {https://juser.fz-juelich.de/record/848192}, }