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低收敛比直接驱动惯性约束聚变内爆的一维流体动力学模拟。

One-dimensional hydrodynamic simulations of low convergence ratio direct-drive inertial confinement fusion implosions.

作者信息

Paddock R W, Martin H, Ruskov R T, Scott R H H, Garbett W, Haines B M, Zylstra A B, Aboushelbaya R, Mayr M W, Spiers B T, Wang R H W, Norreys P A

机构信息

Clarendon Laboratory, University of Oxford, Oxford, UK.

University College, University of Oxford, Oxford, UK.

出版信息

Philos Trans A Math Phys Eng Sci. 2021 Jan 25;379(2189):20200224. doi: 10.1098/rsta.2020.0224. Epub 2020 Dec 7.

DOI:10.1098/rsta.2020.0224
PMID:33280567
原文链接:https://pmc.ncbi.nlm.nih.gov/articles/PMC7741005/
Abstract

Indirect drive inertial confinement fusion experiments with convergence ratios below 17 have been previously shown to be less susceptible to Rayleigh-Taylor hydrodynamic instabilities, making this regime highly interesting for fusion science. Additional limitations imposed on the implosion velocity, in-flight aspect ratio and applied laser power aim to further reduce instability growth, resulting in a new regime where performance can be well represented by one-dimensional (1D) hydrodynamic simulations. A simulation campaign was performed using the 1D radiation-hydrodynamics code HYADES to investigate the performance that could be achieved using direct-drive implosions of liquid layer capsules, over a range of relevant energies. Results include potential gains of 0.19 on LMJ-scale systems and 0.75 on NIF-scale systems, and a reactor-level gain of 54 for an 8.5 MJ implosion. While the use of 1D simulations limits the accuracy of these results, they indicate a sufficiently high level of performance to warrant further investigations and verification of this new low-instability regime. This potentially suggests an attractive new approach to fusion energy. This article is part of a discussion meeting issue 'Prospects for high gain inertial fusion energy (part 2)'.

摘要

先前的研究表明,收敛比低于17的间接驱动惯性约束聚变实验对瑞利 - 泰勒流体动力学不稳定性的敏感度较低,这使得该领域对聚变科学极具吸引力。对内爆速度、飞行纵横比和施加的激光功率施加的额外限制旨在进一步减少不稳定性增长,从而形成一种新的状态,在这种状态下,性能可以通过一维(1D)流体动力学模拟很好地体现。使用一维辐射流体动力学代码HYADES进行了一系列模拟,以研究在一系列相关能量下,利用液层胶囊的直接驱动内爆所能实现的性能。结果包括在兆焦耳激光装置(LMJ)规模系统上潜在增益为0.19,在国家点火装置(NIF)规模系统上为0.75,对于8.5兆焦耳的内爆,反应堆级增益为54。虽然使用一维模拟限制了这些结果的准确性,但它们表明了足够高的性能水平,值得对这种新的低不稳定性状态进行进一步研究和验证。这可能暗示了一种有吸引力的聚变能源新方法。本文是“高增益惯性聚变能源前景(第2部分)”讨论会议问题的一部分。

https://cdn.ncbi.nlm.nih.gov/pmc/blobs/454a/7741005/e37aeff82ad4/rsta20200224-g10.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/454a/7741005/ead376d7882e/rsta20200224-g1.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/454a/7741005/ad3b68ccf603/rsta20200224-g2.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/454a/7741005/d6e6b7978e34/rsta20200224-g3.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/454a/7741005/af8c10a31944/rsta20200224-g4.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/454a/7741005/9886160ff5f4/rsta20200224-g5.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/454a/7741005/3576e33fbe2d/rsta20200224-g6.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/454a/7741005/1a774dc92ba8/rsta20200224-g7.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/454a/7741005/ae88181bc2ed/rsta20200224-g8.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/454a/7741005/d6a288450b79/rsta20200224-g9.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/454a/7741005/e37aeff82ad4/rsta20200224-g10.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/454a/7741005/ead376d7882e/rsta20200224-g1.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/454a/7741005/ad3b68ccf603/rsta20200224-g2.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/454a/7741005/d6e6b7978e34/rsta20200224-g3.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/454a/7741005/af8c10a31944/rsta20200224-g4.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/454a/7741005/9886160ff5f4/rsta20200224-g5.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/454a/7741005/3576e33fbe2d/rsta20200224-g6.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/454a/7741005/1a774dc92ba8/rsta20200224-g7.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/454a/7741005/ae88181bc2ed/rsta20200224-g8.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/454a/7741005/d6a288450b79/rsta20200224-g9.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/454a/7741005/e37aeff82ad4/rsta20200224-g10.jpg

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