Use of tritium-rich fuel to improve the yield of layered deuterium/tritium inertial fusion capsules

IF 1.6 3区 物理与天体物理 Q3 PHYSICS, FLUIDS & PLASMAS High Energy Density Physics Pub Date : 2024-06-04 DOI:10.1016/j.hedp.2024.101118
B.J. Albright, W. Daughton, B.M. Haines, N.M. Hoffman, J.J. Kuczek, R. Lester, K.D. Meaney, J.P. Sauppe
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Abstract

In deuterium–tritium (DT) ice layered implosions, nearly all hot spot mass at peak burn comes from the dense fuel. Accurate prediction of the fuel mass ablation, including the enthalpy associated with mass inflow into the hot spot from the dense fuel, is essential to understanding the energetics and ignition of the hot spot in layered implosions. A recently published boundary layer analysis (Daughton et al., 2023) indicates a faster mass ablation rate than in previous analyses of layered implosions. Inclusion of this effect provides a better match to simulations and leads to a new ignition threshold where the temperature of the dense fuel plays a critical role. This analysis motivates possible new directions for improved capsule performance. Here, the authors present evidence in support of one such approach: the use of tritium-rich ice to decrease 14 MeV neutron scattering and heating of the dense fuel, resulting in less mass ablation and more robust burn of the hot spot. It is found from numerical simulations that despite a less favorable D:T ratio in the ice, the use of a 40:60 D:T ratio leads to an increase in capsule yield of 17% percent compared with that of a 50:50 D:T ratio fuel for capsules resembling those of the recent N210808 ignition experiment on the NIF (Abu-Shawareb et al., 2022) and an increase of 74% compared with that of a 60:40 D:T ratio fuel capsule. These results are potentially important for modeling all layered implosions, since some degree of DT fractionization may arise naturally during the beta layering process. In addition, this physics is important for the feasibility of high-gain capsule designs that seek to minimize tritium usage, as in some inertial fusion energy concepts.

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利用富氚燃料提高分层氘/氚惯性聚变胶囊的产量
在氘-氚(DT)冰分层内爆中,燃烧峰值时几乎所有的热点质量都来自于致密燃料。准确预测燃料质量烧蚀,包括与高密度燃料质量流入热点相关的焓,对于理解层内爆中热点的能量学和点火至关重要。最近发表的边界层分析(Daughton 等人,2023 年)表明,质量烧蚀速率比以前的分层内爆分析要快。考虑到这一影响,可以更好地与模拟结果相匹配,并得出一个新的点火阈值,在这个阈值中,高密度燃料的温度起着至关重要的作用。这一分析为提高太空舱性能提供了新的方向。在此,作者提出了支持其中一种方法的证据:使用富含氚的冰来减少 14 MeV 中子散射和致密燃料的加热,从而减少质量烧蚀,使热点的燃烧更强劲。数值模拟发现,尽管冰中的 D:T 比值较低,但使用 40:60 的 D:T 比值与 50:50 D:T 比值的燃料胶囊相比,胶囊产量增加了 17%,这与最近在 NIF 上进行的 N210808 点火实验(Abu-Shawareb 等人,2022 年)的胶囊类似;与 60:40 D:T 比值的燃料胶囊相比,胶囊产量增加了 74%。这些结果对于所有分层内爆建模具有潜在的重要意义,因为在β分层过程中可能会自然产生某种程度的 DT 分馏。此外,这种物理学原理对于寻求尽量减少氚用量的高增益胶囊设计(如某些惯性聚变能概念)的可行性也很重要。
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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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