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Prevention of core particle depletion in stellarators by turbulence

Abstract:
In reactor-relevant plasmas, neoclassical transport drives an outward particle flux in the core of large stellarators and predicts strongly hollow density profiles. However, this theoretical prediction is contradicted by experiments. In particular, in Wendelstein 7-X, the first large optimized stellarator, flat or weakly peaked density profiles are generally measured, indicating that neoclassical theory is not sufficient and that an inward contribution to the particle flux is missing in the core. In this Research Letter, it is shown that the turbulent contribution to the particle flux can explain the difference between experimental measurements and neoclassical predictions. The results of this Research Letter also prove that theoretical and numerical tools are approaching the level of maturity needed for the prediction of equilibrium density profiles in stellarator plasmas, which is a fundamental requirement for the design of operation scenarios of present devices and future reactors.
Publication status:
Published
Peer review status:
Peer reviewed

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Publisher copy:
10.1103/PhysRevResearch.5.L022053

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Role:
Author
ORCID:
0000-0002-0327-0853
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Role:
Author
ORCID:
0000-0001-7632-3357
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Author
ORCID:
0000-0003-3118-3463
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ORCID:
0000-0001-6863-8578
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Role:
Author
ORCID:
0000-0001-8510-1422


Publisher:
American Physical Society
Journal:
Physical Review Research More from this journal
Volume:
5
Issue:
2
Article number:
L022053
Publication date:
2023-06-13
Acceptance date:
2023-05-10
DOI:
EISSN:
2643-1564


Language:
English
Keywords:
Pubs id:
1464904
Local pid:
pubs:1464904
Deposit date:
2023-08-21

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