FLAIM: A reduced volume ignition model for the compression and thermonuclear burn of spherical fuel capsules

IF 1.6 3区 物理与天体物理 Q3 PHYSICS, FLUIDS & PLASMAS
Abd Essamade Saufi, Hannah Bellenbaum , Martin Read, Nicolas Niasse, Sean Barrett, Nicholas Hawker, Nathan Joiner, David Chapman
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Abstract

We present the “First Light Advanced Ignition Model” (FLAIM), a reduced model for the implosion, adiabatic compression, volume ignition and thermonuclear burn of a spherical DT fuel capsule utilising a high-Z metal pusher. FLAIM is characterised by a highly modular structure, which makes it an appropriate tool for optimisations, sensitivity analyses and parameter scans. One of the key features of the code is the 1D description of the hydrodynamic operator, which has a minor impact on the computational efficiency, but allows us to gain a major advantage in terms of physical accuracy. We demonstrate that a more accurate treatment of the hydrodynamics plays a primary role in closing most of the gap between a simple model and a general 1D rad-hydro code, and that only a residual part of the discrepancy is attributable to the heat losses. We present a detailed quantitative comparison between FLAIM and 1D rad-hydro simulations, showing good agreement over a large parameter space in terms of temporal profiles of key physical quantities, ignition maps and typical burn metrics.
FLAIM:球形燃料囊压缩和热核燃烧的减容点火模型
我们介绍了 "第一光先进点火模型"(FLAIM),这是一个利用高 Z 金属推杆对球形 DT 燃料囊进行内爆、绝热压缩、体积点火和热核燃烧的简化模型。FLAIM 的特点是高度模块化结构,这使其成为优化、敏感性分析和参数扫描的合适工具。代码的主要特点之一是流体力学算子的一维描述,这对计算效率影响不大,但使我们在物理精度方面获得了重大优势。我们证明,更精确的流体动力学处理在缩小简单模型与一般一维雷达-流体动力学代码之间的大部分差距方面发挥了主要作用,只有剩余部分的差异可归因于热损失。我们对 FLAIM 和 1D rad-hydro 模拟进行了详细的定量比较,结果表明,在很大的参数空间内,关键物理量的时间曲线、点火图和典型燃烧指标都非常吻合。
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来源期刊
High Energy Density Physics
High Energy Density Physics PHYSICS, FLUIDS & PLASMAS-
CiteScore
4.20
自引率
6.20%
发文量
13
审稿时长
6-12 weeks
期刊介绍: High Energy Density Physics is an international journal covering original experimental and related theoretical work studying the physics of matter and radiation under extreme conditions. ''High energy density'' is understood to be an energy density exceeding about 1011 J/m3. The editors and the publisher are committed to provide this fast-growing community with a dedicated high quality channel to distribute their original findings. Papers suitable for publication in this journal cover topics in both the warm and hot dense matter regimes, such as laboratory studies relevant to non-LTE kinetics at extreme conditions, planetary interiors, astrophysical phenomena, inertial fusion and includes studies of, for example, material properties and both stable and unstable hydrodynamics. Developments in associated theoretical areas, for example the modelling of strongly coupled, partially degenerate and relativistic plasmas, are also covered.
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