Study on the effect of neutron shielding design on tritium breeding based on water-cooled ceramic blanket for CFETR

Author:

Li Jie1ORCID,Li Hang1ORCID,Wu Muquan1ORCID,Zhu Xiang1ORCID,Yan Peiguang1ORCID,Lin Xiaodong1,Zhang Jie2,Gao Xiang12ORCID

Affiliation:

1. College of Physics and Optoelectronic Engineering, Shenzhen University 1 , Shenzhen 518060, China

2. Institute of Plasma Physics, Chinese Academic Sciences 2 , Hefei 230026, China

Abstract

The Chinese Fusion Engineering Test Reactor (CFETR) is a magnetic confinement fusion reactor independently designed and developed by China, which is based on the ITER design experience. As one of the candidates for the CFETR, the water cooled ceramic blanket (WCCB) mainly carries out many important tasks, such as tritium breeding and radiation shielding. The high tritium breeding ability is one of the most significant goals of the blanket. For the design of the CFETR, in addition to meeting the requirements of tritium breeding, the design of the blanket must also consider meeting relevant shielding limits. Due to the limited space of the blanket, the improvement in tritium breeding space will inevitably lead to the reduction in neutron shielding space behind the breeding area, and vice versa. Therefore, under the premise of meeting the requirements of neutron shielding, increasing the tritium breeding space as much as possible is the focus of research. In this work, a three-dimensional neutronics model containing the WCCB blanket is developed, and the neutronics performance is calculated based on 1.5 GW fusion power. A set of nuclear analyses are carried out by the MCNP code, including analysis of the neutron wall load, tritium breeding ratio (TBR), and fast neutron fluence of the TF coil. It is found that the shielding space of certain blanket modules could be optimized. After the shielding optimization, the global TBR increased from 1.168 to 1.186, an increase of 0.018 TBR. The current research has important guiding significance for the future design and optimization of the WCCB for the CFETR.

Funder

National Key Research and Development Program of China

National Natural Science Foundation of China-Guangdong Joint Fund

Publisher

AIP Publishing

Subject

General Physics and Astronomy

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