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@ARTICLE{Heidbrink:1026967,
author = {Heidbrink, W. W. and Baylor, L. R. and Büscher, Markus and
Engels, Ralf W. and Garcia, A. V. and Ghiozzi, A. G. and
Miller, G. W. and Sandorfi, A. M. and Wei, X. and Zheng, X.},
title = {{A} research program to measure the lifetime of spin
polarized fuel},
journal = {Frontiers in physics},
volume = {12},
issn = {2296-424X},
address = {Lausanne},
publisher = {Frontiers Media},
reportid = {FZJ-2024-03546},
pages = {1355212},
year = {2024},
abstract = {The use of spin polarized fuel could increase the
deuterium-tritium (D-T) fusion cross section by a factor of
1.5 and, owing to alpha heating, increase the fusion power
by an even larger factor. Issues associated with the use of
polarized fuel in a reactor are identified. Theoretically,
nuclei remain polarized in a hot fusion plasma. The
similarity between the Lorentz force law and the Bloch
equations suggests polarization can be preserved despite the
rich electromagnetic spectrum present in a magnetic fusion
device. The most important depolarization mechanisms can be
tested in existing devices. The use of polarized deuterium
and $^3$He in an experiment avoids the complexities of
handling tritium, while encompassing the same nuclear
reaction spin-physics, making it a useful proxy to study
issues associated with full D-T implementation. $^3$He fuel
with 65\% polarization can be prepared by permeating
optically-pumped $^3$He into a shell pellet. Dynamically
polarized 7Li-D pellets can achieve 70\% vector polarization
for the deuterium. Cryogenically-frozen pellets can be
injected into fusion facilities by special injectors that
minimize depolarizing field gradients. Alternatively,
polarized nuclei could be injected as a neutral beam. Once
injected, the lifetime of the polarized fuel is monitored
through measurements of escaping charged fusion products.
Multiple experimental scenarios to measure the polarization
lifetime in the DIII-D tokamak and other
magnetic-confinement facilities are discussed, followed by
outstanding issues that warrant further study.},
cin = {IKP-2 / PGI-6},
ddc = {530},
cid = {I:(DE-Juel1)IKP-2-20111104 / I:(DE-Juel1)PGI-6-20110106},
pnm = {612 - Cosmic Matter in the Laboratory (POF4-612)},
pid = {G:(DE-HGF)POF4-612},
typ = {PUB:(DE-HGF)16},
UT = {WOS:001248687500001},
doi = {10.3389/fphy.2024.1355212},
url = {https://juser.fz-juelich.de/record/1026967},
}