Suppression of non-axisymmetric field-induced α-particle loss channels in a quasi-axisymmetric stellarator

Author:

Zhang Yichao1,Liu Haifeng1ORCID,Huang Jie1,Xu Yuhong1ORCID,Zhang Jian1,Shimizu Akihiro23,Satake Shinsuke2ORCID,Isobe Mitsutaka23ORCID,Wang Xianqu1ORCID,Cheng Jun2ORCID,Liu Hai1ORCID,Zhang Xin1,Tang Changjian14

Affiliation:

1. Institute of Fusion Science, School of Physical Science and Technology, Southwest Jiaotong University, Chengdu 610031, China

2. National Institute for Fusion Science, National Institutes of Natural Sciences, Toki 509-5292, Japan

3. The Graduate University for Advanced Studies, SOKENDAI, Toki 509-5292, Japan

4. College of Physics, Sichuan University, Chengdu 610065, China

Abstract

In future fusion reactors, the confinement of α-particles is a crucial issue. The perfect omnigenity may be difficult to achieve in the quasi-isodynamic and quasi-symmetric stellarators when a multi-objective optimization is considered. Non-axisymmetric field can result in collisionless particles’ transport via localized trapping by ripples. Specific loss channels have been revealed to essentially exist in quasi-axisymmetric stellarators [Yang et al., Europhys. Lett. 129, 35001 (2020)] and W7-X [J. M. Faustin et al., Nucl. Fusion 56, 092006 (2016)]. It indicates a drastic loss of collisionless ions through these channels. This paper is devoted to investigate the effects of axisymmetry-breaking magnetic fields on collisionless α-particle transport in the CFQS (Chinese First Quasi-axisymmetric Stellarator) -like reactor configuration. A semi-analytic representation of radial and poloidal drifts in Boozer coordinates is given, by which we found an effective route to mitigate α-particle losses, i.e., adjusting the location of the quasi-axisymmetric radial position. Such a route enables the enhancement of the poloidal drift and decrease of radial drift in peripheral regions of the identified loss channels. The particles launched inside the quasi-axisymmetric radial surface can be well confined because localized particles that may fall in loss channels can transit into blocked particles near the quasi-axisymmetric surface, escaping from loss channels, which is beneficial for the improvement of the particle confinement. Moreover, this paper may provide a set of proxy functions for suppression of energetic particle losses to optimize stellarator configurations.

Funder

National Natural Science Foundation of China

National Key Research and Development Program of China

Fundamental Research Funds for the Central Universities

Advanced Foreign Expert Introduction Program

Central Government Funds of Guiding Local Scientific and Technological Development for Sichuan Province

Publisher

AIP Publishing

Subject

General Physics and Astronomy

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